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		<summary type="html">&lt;p&gt;Sk7118: /* Question 4) A reactive F + H2 trajectory */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one of the coordinates is positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately &#039;&#039;&#039;90.77&#039;&#039;&#039; &#039;&#039;&#039;pm&#039;&#039;&#039; for the H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system.&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
For the MEP path, no vibrational motion of the formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is observed unlike in the case of dynamic mode. Over the course of the reaction, some of the initial potential energy is changed into kinetic energy. When molecular hydrogen forms, some of the kinetic energy is converted into vibrational energy, which is indicated by the oscillations on the PE surface. In the case of MEP, the reaction proceeds via a pathway with smallest possible total energy. In order to minimise the total energy, vibrational energy must be minimised as well. Consequently, no vibrational motion is observed in the MEP mode. As the MEP mode corresponds to infinitely slow motion of the nuclei, no changes in momenta or velocities are observed either. Furthermore, total energy of the system is not conserved in the MEP mode. The total potential energy of products is lower than the potential energy at TS but as the system has no kinetic energy at any point, E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; must be equal to E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt;. This seemingly violates the law of conservation of energy, but that it is just the result of assumptions made in the MEP mode. On the other hand, energy is conserved in the dynamics mode as motion of the atoms is not taken to be infinitely slow.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free radical (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as the TS structure described in question 2. Essentially, it is the reverse process of TS structure converting into products.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table below by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C &amp;lt;/sub&amp;gt;but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials even after crossing the TS due to high energy oscillations brought about by the collision, as illustrated by the different initial conditions listed in the table above. &lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The differences between TST predictions and experimental rate constant values are the direct result of assumptions made in calculations based on TST.&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&lt;br /&gt;
# The motion of nuclei is described only by classical mechanics and any quantum effects are neglected. This has a great influence on simple reactions involving light particles (H, D), as possible quantum tunneling is not taken into account. In reality, light particles can tunnel through narrow low energy barriers and this is especially likely in given simple case. Therefore in the case of reaction H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, employing TST will result in underestimation of the rate constant. Nevertheless, other influences of TST assumptions should be considered in conjunction with this one and therefore the rate constant might still be overestimated, regardless of quantum mechanical effects. In reactions involving more massive atoms or higher energy barriers, neglecting quantum behaviour of particles and tunneling will likely have no effect on the predicted rate constant as the probability of tunneling decreases exponentially with increasing particle mass.&lt;br /&gt;
# Every collision with sufficient kinetic energy will definitely cross the TS and will go on to form the products. Furthermore, conversion to products is considered to be irreversible: reactants that have reached the transition state will not revert back to starting materials. In reality, the TS can revert back to starting materials as well. As illustrated by the entries in the table above, products are often able to recross the TS and convert back into starting materials, given a suitable distribution of translational and vibrational energies. Additionally, reactions leading back to starting materials can still occur, although this will have a small effect if the forward equilibrium constant is very large. As a consequence, these assumptions of TST would overestimate the rate constant for reforming starting materials decrease the total reaction rate. &lt;br /&gt;
# The transition state structure is in quasi-equilibrium with the reactants and the particles follow a Boltzmann distribution of energies. In addition, TS structures are sufficiently long-lived to reach a Boltzmann distribution of energies as well before converting to products. Although the thermal equilibrium is not very important in H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system, in very fast reactions the nuclei might not reach a Boltzmann distribution of energies before colliding. Furthermore at very high temperatures, higher energy levels are populated, thus breaking the assumption that only low vibrational states are populated. If the average energies of particles are different from what is predicted, the fraction of sufficiently energetic collisions leading to TS cannot be accurately estimated either. This could result in poor estimates for the rate constant as crossing the energy barrier to form TS is rate limiting.&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; is exothermic, as the energy of the products (HF + H) is lower than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; is endothermic, as the products are higher in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 436 kJ/mol, respectively.&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;  As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps) and that using a larger r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value can give a slightly smaller total energy value, but this is a sufficient approximation.&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by femtosecond absorption spectroscopy, in which molecules are excited electronically by a short laser pulse (lasting ca 1 ps) to a dissociative state. After a short interval, the excited molecule is exposed to another pulse at the absorption wavelength of one of the products. From the presence of dissociation product absorption bands and their relative intensities with respect to the excited molecule absorption bands (HF in this case), composition of gas-phase reaction mixtures can be probed.&amp;lt;sup&amp;gt;3 &amp;lt;/sup&amp;gt;In addition, vibrational or rotational spectroscopy could be used too as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* Conversion to products seems to be more likely at low p values (in the range -2 to 2 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;&#039;&#039;). Although conversion is likely at values around -6.1 and 6.1 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; &#039;&#039;as well, small changes in p value seem to have a great influence on the outcome of the reaction. On the other hand, at small initial momenta values, small changes (+-0.05 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;&#039;&#039;) seem to have little effect on the outcome.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*The products are formed. Increasing p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; has little effect on the outcome until values of ca 2 - 1.6&#039;&#039; &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In endothermic reactions, the TS occurs early in the reactant channel. This means that the TS structure of the starting materials best resembles the TS structure. On the other hand, in exothermic reactions, the TS occurs late in the products channel. This means that the TS structure of the products is more close to the TS structure. According to Polyani&#039;s empirical rules, the translational component of reactant energy is more important in crossing an early TS and vibrational energy is more important in overcoming a late TS.&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;  &lt;br /&gt;
&lt;br /&gt;
As illustrated by the exothermic reaction between F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, products are unlikely to form if the vibrational component of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is high and translational component is low. If H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is just busy oscillating and the colliding species do not have sufficient kinetic energy, the early TS is unlikely to be crossed and the H-H bond is not broken. Although formation of the stronger H-F bond is energetically favoured, it cannot happen if the collision itself is not energetic enough.  &lt;br /&gt;
&lt;br /&gt;
Conversely, in the endothermic reaction between H and HF, the vibrational energy of HF has a key role in the success of the reaction. Even if the kinetic energy of H is high but the vibrational energy of HF is low, products are again unlikely to be formed. In order to cross the late TS, the strong HF bond has to have sufficient vibrational energy in order to be broken upon collision with the free H. As shown previously, the fluorine atom attracts the leaving hydrogen quite strongly so unless the HF bond oscillates heavily before the collision, H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; cannot form as the strong attractive forces of fluorine cannot be overcome even when collisions occur with high kinetic energies.&lt;br /&gt;
&lt;br /&gt;
As a result, reactions might not proceed even if the system has enough energy to overcome the TS barrier or to irreversibly convert to the products having crossed the TS. The key to successful reactions lies among other factors in the distribution of energy between different modes of molecular motion.&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
1. Steinfeld J. I., Francisco J. S., Hase W. L. Chemical Kinetics and Dynamics 2nd Edition, pg 315-318. Prentice-Hall.&lt;br /&gt;
&lt;br /&gt;
2. Atkins P., de Paula J. (2014) Physical Chemistry 10th Edition, pg 985. Oxford University Press.&lt;br /&gt;
&lt;br /&gt;
3. Atkins P., de Paula J. (2014) Physical Chemistry 10th Edition, pg 898. Oxford University Press.&lt;br /&gt;
&lt;br /&gt;
4. Steinfeld J. I., Francisco J. S., Hase W. L. Chemical Kinetics and Dynamics 2nd Edition, pg 272-274. Prentice-Hall.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809985</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809985"/>
		<updated>2020-05-22T12:46:59Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Exercise 1 */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one of the coordinates is positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately &#039;&#039;&#039;90.77&#039;&#039;&#039; &#039;&#039;&#039;pm&#039;&#039;&#039; for the H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system.&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
For the MEP path, no vibrational motion of the formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is observed unlike in the case of dynamic mode. Over the course of the reaction, some of the initial potential energy is changed into kinetic energy. When molecular hydrogen forms, some of the kinetic energy is converted into vibrational energy, which is indicated by the oscillations on the PE surface. In the case of MEP, the reaction proceeds via a pathway with smallest possible total energy. In order to minimise the total energy, vibrational energy must be minimised as well. Consequently, no vibrational motion is observed in the MEP mode. As the MEP mode corresponds to infinitely slow motion of the nuclei, no changes in momenta or velocities are observed either. Furthermore, total energy of the system is not conserved in the MEP mode. The total potential energy of products is lower than the potential energy at TS but as the system has no kinetic energy at any point, E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; must be equal to E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt;. This seemingly violates the law of conservation of energy, but that it is just the result of assumptions made in the MEP mode. On the other hand, energy is conserved in the dynamics mode as motion of the atoms is not taken to be infinitely slow.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free radical (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as the TS structure described in question 2. Essentially, it is the reverse process of TS structure converting into products.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table below by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C &amp;lt;/sub&amp;gt;but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials even after crossing the TS due to high energy oscillations brought about by the collision, as illustrated by the different initial conditions listed in the table above. &lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The differences between TST predictions and experimental rate constant values are the direct result of assumptions made in calculations based on TST.&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&lt;br /&gt;
# The motion of nuclei is described only by classical mechanics and any quantum effects are neglected. This has a great influence on simple reactions involving light particles (H, D), as possible quantum tunneling is not taken into account. In reality, light particles can tunnel through narrow low energy barriers and this is especially likely in given simple case. Therefore in the case of reaction H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, employing TST will result in underestimation of the rate constant. Nevertheless, other influences of TST assumptions should be considered in conjunction with this one and therefore the rate constant might still be overestimated, regardless of quantum mechanical effects. In reactions involving more massive atoms or higher energy barriers, neglecting quantum behaviour of particles and tunneling will likely have no effect on the predicted rate constant as the probability of tunneling decreases exponentially with increasing particle mass.&lt;br /&gt;
# Every collision with sufficient kinetic energy will definitely cross the TS and will go on to form the products. Furthermore, conversion to products is considered to be irreversible: reactants that have reached the transition state will not revert back to starting materials. In reality, the TS can revert back to starting materials as well. As illustrated by the entries in the table above, products are often able to recross the TS and convert back into starting materials, given a suitable distribution of translational and vibrational energies. Additionally, reactions leading back to starting materials can still occur, although this will have a small effect if the forward equilibrium constant is very large. As a consequence, these assumptions of TST would overestimate the rate constant for reforming starting materials decrease the total reaction rate. &lt;br /&gt;
# The transition state structure is in quasi-equilibrium with the reactants and the particles follow a Boltzmann distribution of energies. In addition, TS structures are sufficiently long-lived to reach a Boltzmann distribution of energies as well before converting to products. Although the thermal equilibrium is not very important in H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system, in very fast reactions the nuclei might not reach a Boltzmann distribution of energies before colliding. Furthermore at very high temperatures, higher energy levels are populated, thus breaking the assumption that only low vibrational states are populated. If the average energies of particles are different from what is predicted, the fraction of sufficiently energetic collisions leading to TS cannot be accurately estimated either. This could result in poor estimates for the rate constant as crossing the energy barrier to form TS is rate limiting.&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; is exothermic, as the energy of the products (HF + H) is lower than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; is endothermic, as the products are higher in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 436 kJ/mol, respectively.&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;  As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps) and that using a larger r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value can give a slightly smaller total energy value, but this is a sufficient approximation.&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by femtosecond absorption spectroscopy, in which molecules are excited electronically by a short laser pulse (lasting ca 1 ps) to a dissociative state. After a short interval, the excited molecule is exposed to another pulse at the absorption wavelength of one of the products. From the presence of dissociation product absorption bands and their relative intensities with respect to the excited molecule absorption bands (HF in this case), composition of gas-phase reaction mixtures can be probed.&amp;lt;sup&amp;gt;3 &amp;lt;/sup&amp;gt;In addition, vibrational or rotational spectroscopy could be used too as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* Conversion to products seems to be more likely at low p values (in the range -2 to 2 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;&#039;&#039;). Although conversion is likely at values around -6.1 and 6.1 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; &#039;&#039;as well, small changes in p value seem to have a great influence on the outcome of the reaction. On the other hand, at small initial momenta values, small changes (+-0.05 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;&#039;&#039;) seem to have little effect on the outcome.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*The products are formed. Increasing p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; has little effect on the outcome until values of ca 2 - 1.6&#039;&#039; &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In endothermic reactions, the TS occurs early in the reactant channel. This means that the TS structure of the starting materials best resembles the TS structure. On the other hand, in exothermic reactions, the TS occurs late in the products channel. This means that the TS structure of the products is more close to the TS structure. According to Polyani&#039;s empirical rules, the translational component of reactant energy is more important in crossing an early TS and vibrational energy is more important in overcoming a late TS.&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;  &lt;br /&gt;
&lt;br /&gt;
As illustrated by the exothermic reaction between F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, products are unlikely to form if the vibrational component of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is high and translational component is low. If H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is just busy oscillating and the colliding species do not have sufficient kinetic energy, the early TS is unlikely to be crossed and the H-H bond is not broken. Although formation of the stronger H-F bond is energetically favoured, it cannot happen if the collision itself is not energetic enough.  &lt;br /&gt;
&lt;br /&gt;
Conversely, in the endothermic reaction between H and HF, the vibrational energy of HF has a key role in the success of the reaction. Even if the kinetic energy of H is high but the vibrational energy of HF is low, products are again unlikely to be formed. In order to cross the late TS, the strong HF bond has to have sufficient vibrational energy in order to be broken upon collision with the free H. As shown previously, the fluorine atom attracts the leaving hydrogen quite strongly so unless the HF bond oscillates heavily before the collision, H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; cannot form as the strong attractive forces of fluorine cannot be overcome even when collisions occur with high kinetic energies.&lt;br /&gt;
&lt;br /&gt;
As a result, reactions might not proceed even if the system has enough energy to overcome the TS barrier or to irreversibly convert to the products having crossed the TS. The key to successful reactions lies among other factors in the distribution of energy between different modes of molecular motion.&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
1. Steinfeld J. I., Francisco J. S., Hase W. L. Chemical Kinetics and Dynamics 2nd Edition, pg 315-318. Prentice-Hall.&lt;br /&gt;
&lt;br /&gt;
2. Atkins P., de Paula J. (2014) Physical Chemistry 10th Edition, pg 985. Oxford University Press.&lt;br /&gt;
&lt;br /&gt;
3. Atkins P., de Paula J. (2014) Physical Chemistry 10th Edition, pg 898. Oxford University Press.&lt;br /&gt;
&lt;br /&gt;
4. Steinfeld J. I., Francisco J. S., Hase W. L. Chemical Kinetics and Dynamics 2nd Edition, pg 272-274. Prentice-Hall.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809758</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809758"/>
		<updated>2020-05-22T11:17:18Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 4) A reactive F + H2 trajectory */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately &#039;&#039;&#039;90.77&#039;&#039;&#039; &#039;&#039;&#039;pm&#039;&#039;&#039; for the H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system.&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
For the MEP path, no vibrational motion of the formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is observed unlike in the case of dynamic mode. Over the course of the reaction, some of the initial potential energy is changed into kinetic energy. When molecular hydrogen forms, some of the kinetic energy is converted into vibrational energy, which is indicated by the oscillations on the PE surface. In the case of MEP, the reaction proceeds via a pathway with smallest possible total energy. In order to minimise the total energy, vibrational energy must be minimised as well. Consequently, no vibrational motion can be observed in this case for the MEP mode. As the MEP mode corresponds to infinitely slow motion, no changes in momenta or velocities are observed either. Furthermore, total energy of the system is not conserved in the MEP mode. The total potential energy of products is lower than the potential energy at TS but as the system has no kinetic energy at any point E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; must be equal to E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt;. This seemingly violates the law of conservation of energy, but that it is just the result of assumptions made in the MEP mode. On the other hand, energy is conserved in the dynamics mode as motion of the atoms is not taken to be infinitely slow.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as the TS structure described in question 2. Essentially, it is the reverse process of TS structure converting into products.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table below by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials even after crossing the TS due to high energy oscillations brought about by the collision, as illustrated by the different initial conditions listed in the table above. &lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The differences between TST predictions and experimental rate constant values are the direct result of assumptions made in calculations based on TST.&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&lt;br /&gt;
# The motion of nuclei is described only by classical mechanics and any quantum effects are neglected. This has a great influence on simple reactions involving light particles (H, D), as possible quantum tunneling is not taken into account. In reality, light particles can tunnel through narrow low energy barriers and this is especially likely in given simple case. Therefore in this reaction, TST is likely to underestimate the rate constant. In reactions involving more massive atoms or higher energy barriers, neglecting quantum tunneling will likely have no effect on the predicted rate constant as the probability of tunneling decreases exponentially with increasing particle mass.&lt;br /&gt;
# Conversion to products is considered to be irreversible: reactants that have reached the transition state will only proceed to form the products and not revert back to starting materials. In reality, the TS can revert back to starting materials as well. In other systems, collisions leading back to starting materials can still occur, although this will have a small effect if the forward equilibrium constant is very large. As a consequence, TST would overestimate the rate constant. &lt;br /&gt;
# The transition state structure is in quasi-equilibrium with the reactants.&lt;br /&gt;
# Translation of the nuclei can be separated from vibrational and rotational motion.&lt;br /&gt;
# The reactants and products are at a Boltzmann distribution of energies and the TS structures are sufficiently long-lived to reach Boltzmann distribution as well before converting to products.&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 436 kJ/mol, respectively.&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;  As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps) and that using a larger r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value can give a slightly smaller total energy value, but this is a sufficient approximation.&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by femtosecond absorption spectroscopy, in which molecules are excited electronically by a short laser pulse (lasting ca 1 ps) to a dissociative state. After a short interval, the excited molecule is exposed to another pulse at the absorption wavelength of one of the products. From the presence of dissociation product absorption bands and their relative intensities with respect to the excited molecule absorption bands (HF in this case), composition of gas-phase reaction mixtures can be probed.&amp;lt;sup&amp;gt;3 &amp;lt;/sup&amp;gt;In addition, vibrational or rotational spectroscopy could be used too as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* Conversion to products seems to be more likely at low p values (in the range -2 to 2 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;&#039;&#039;). Although conversion is likely at values around -6.1 and 6.1 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; &#039;&#039;as well, small changes in p value seem to have a great influence on the outcome of the reaction. On the other hand, at small initial momenta values, small changes (+-0.05 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;&#039;&#039;) seem to have little effect on the outcome.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*The products are formed. Increasing p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; has little effect on the outcome until values of ca 2 - 1.6&#039;&#039; &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In endothermic reactions, the TS occurs early in the reactant channel. This means that the TS structure of the starting materials best resembles the TS structure. On the other hand, in exothermic reactions, the TS occurs late in the products channel. This means that the TS structure of the products is more close to the TS structure. According to Polyani&#039;s empirical rules, the translational component of reactant energy is more important in crossing an early TS and vibrational energy is more important in overcoming a late TS.&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;  &lt;br /&gt;
&lt;br /&gt;
As illustrated by the exothermic reaction between F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, products are unlikely to form if the vibrational component of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is high and translational component is low. If H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is just busy oscillating and the colliding species do not have sufficient kinetic energy, the early TS is unlikely to be crossed and the H-H bond is not broken. Although formation of the stronger H-F bond is energetically favoured, it cannot happen if the collision itself is not energetic enough.  &lt;br /&gt;
&lt;br /&gt;
Conversely, in the endothermic reaction between H and HF, the vibrational energy of HF has a key role in the success of the reaction. Even if the kinetic energy of H is high but the vibrational energy of HF is low, products are again unlikely to be formed. In order to cross the late TS, the strong HF bond has to have sufficient vibrational energy in order to be broken upon collision with the free H. As shown previously, the fluorine atom attracts the leaving hydrogen quite strongly so unless the HF bond oscillates heavily before the collision, H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; cannot form as the strong attractive forces of fluorine cannot be overcome even when collisions occur with high kinetic energies.&lt;br /&gt;
&lt;br /&gt;
As a result, reactions might not proceed even if the system has enough energy to overcome the TS barrier or to irreversibly convert to the products having crossed the TS. The key to successful reactions lies among other factors in the distribution of energy between different modes of molecular motion.&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
1. Steinfeld J. I., Francisco J. S., Hase W. L. Chemical Kinetics and Dynamics 2nd Edition, pg 315-318. Prentice-Hall.&lt;br /&gt;
&lt;br /&gt;
2. Atkins P., de Paula J. (2014) Physical Chemistry 10th Edition, pg 985. Oxford University Press.&lt;br /&gt;
&lt;br /&gt;
3. Atkins P., de Paula J. (2014) Physical Chemistry 10th Edition, pg 898. Oxford University Press.&lt;br /&gt;
&lt;br /&gt;
4. Steinfeld J. I., Francisco J. S., Hase W. L. Chemical Kinetics and Dynamics 2nd Edition, pg 272-274. Prentice-Hall.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809725</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809725"/>
		<updated>2020-05-22T11:03:36Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 5) Transition state theory */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately &#039;&#039;&#039;90.77&#039;&#039;&#039; &#039;&#039;&#039;pm&#039;&#039;&#039; for the H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system.&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
For the MEP path, no vibrational motion of the formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is observed unlike in the case of dynamic mode. Over the course of the reaction, some of the initial potential energy is changed into kinetic energy. When molecular hydrogen forms, some of the kinetic energy is converted into vibrational energy, which is indicated by the oscillations on the PE surface. In the case of MEP, the reaction proceeds via a pathway with smallest possible total energy. In order to minimise the total energy, vibrational energy must be minimised as well. Consequently, no vibrational motion can be observed in this case for the MEP mode. As the MEP mode corresponds to infinitely slow motion, no changes in momenta or velocities are observed either. Furthermore, total energy of the system is not conserved in the MEP mode. The total potential energy of products is lower than the potential energy at TS but as the system has no kinetic energy at any point E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; must be equal to E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt;. This seemingly violates the law of conservation of energy, but that it is just the result of assumptions made in the MEP mode. On the other hand, energy is conserved in the dynamics mode as motion of the atoms is not taken to be infinitely slow.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as the TS structure described in question 2. Essentially, it is the reverse process of TS structure converting into products.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table below by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials even after crossing the TS due to high energy oscillations brought about by the collision, as illustrated by the different initial conditions listed in the table above. &lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The differences between TST predictions and experimental rate constant values are the direct result of assumptions made in calculations based on TST.&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&lt;br /&gt;
# The motion of nuclei is described only by classical mechanics and any quantum effects are neglected. This has a great influence on simple reactions involving light particles (H, D), as possible quantum tunneling is not taken into account. In reality, light particles can tunnel through narrow low energy barriers and this is especially likely in given simple case. Therefore in this reaction, TST is likely to underestimate the rate constant. In reactions involving more massive atoms or higher energy barriers, neglecting quantum tunneling will likely have no effect on the predicted rate constant as the probability of tunneling decreases exponentially with increasing particle mass.&lt;br /&gt;
# Conversion to products is considered to be irreversible: reactants that have reached the transition state will only proceed to form the products and not revert back to starting materials. In reality, the TS can revert back to starting materials as well. In other systems, collisions leading back to starting materials can still occur, although this will have a small effect if the forward equilibrium constant is very large. As a consequence, TST would overestimate the rate constant. &lt;br /&gt;
# The transition state structure is in quasi-equilibrium with the reactants.&lt;br /&gt;
# Translation of the nuclei can be separated from vibrational and rotational motion.&lt;br /&gt;
# The reactants and products are at a Boltzmann distribution of energies and the TS structures are sufficiently long-lived to reach Boltzmann distribution as well before converting to products.&lt;br /&gt;
--&amp;gt;not able to sample a whole boltzmann distribution in this simulation, just giving initial parameters&lt;br /&gt;
&lt;br /&gt;
thermal equilibrium not always established --&amp;gt; fail at high and low temperatures?&lt;br /&gt;
&lt;br /&gt;
QE assumption: lots of collision happen, but as long as TS is not formed in them, they can reform the reactants&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 436 kJ/mol, respectively.&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;  As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps) and that using a larger r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value can give a slightly smaller total energy value, but this is a sufficient approximation.&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by femtosecond absorption spectroscopy, in which molecules are excited electronically by a short laser pulse (lasting ca 1 ps) to a dissociative state. After a short interval, the excited molecule is exposed to another pulse at the absorption wavelength of one of the products. From the presence of dissociation product absorption bands and their relative intensities with respect to the excited molecule absorption bands (HF in this case), composition of gas-phase reaction mixtures can be probed.&amp;lt;sup&amp;gt;3 &amp;lt;/sup&amp;gt;In addition, vibrational or rotational spectroscopy could be used too as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* Conversion to products seems to be more likely at low p values (in the range -2 to 2 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;&#039;&#039;). Although conversion is likely at values around -6.1 and 6.1 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; &#039;&#039;as well, small changes in p value seem to have a great influence on the outcome of the reaction. On the other hand, at small initial momenta values, small changes (+-0.05 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;&#039;&#039;) seem to have little effect on the outcome.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*The products are formed. Increasing p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; has little effect on the outcome until values of ca 2 &#039;&#039;1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In endothermic reactions, the TS occurs early in the reactant channel and in exothermic reactions, the TS occurs later in the products channel. According to Polyani&#039;s rules, the translational component of reactant energy is more important in crossing an early TS and vibrational energy is more important in overcoming a late TS.&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;  &lt;br /&gt;
&lt;br /&gt;
As illustrated by the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system, products are unlikely to form if the vibrational component of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is high and translational component is low. If H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is just busy oscillating and the collision does not occur with sufficient energy due to lack of kinetic energy of the reactants, the early TS is unlikely to be crossed.  &lt;br /&gt;
&lt;br /&gt;
Conversely, if in the reaction between H and HF the translational energy of H is large and vibrational energy of HF is small, the probability of forming products is again quite low. In order to cross the late TS, the HF bond has to have sufficient vibrational energy in order to be broken upon collision with the free H. As shown previously, the fluorine atom attracts the leaving hydrogen quite strongly so unless the HF bond oscillates heavily before the collision, H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is unlikely to be formed as the strong pull of fluorine cannot be overcome.&lt;br /&gt;
&lt;br /&gt;
As a result, reactions might not proceed even if the system has enough energy to overcome the TS barrier or to irreversibly convert to the products having crossed the TS. The key to successful reactions lies among other factors in the distribution of energy between different modes of molecular motion.&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
1. Steinfeld J. I., Francisco J. S., Hase W. L. Chemical Kinetics and Dynamics 2nd Edition, pg 315-318. Prentice-Hall.&lt;br /&gt;
&lt;br /&gt;
2. Atkins P., de Paula J. (2014) Physical Chemistry 10th Edition, pg 985. Oxford University Press.&lt;br /&gt;
&lt;br /&gt;
3. Atkins P., de Paula J. (2014) Physical Chemistry 10th Edition, pg 898. Oxford University Press.&lt;br /&gt;
&lt;br /&gt;
4. Steinfeld J. I., Francisco J. S., Hase W. L. Chemical Kinetics and Dynamics 2nd Edition, pg 272-274. Prentice-Hall.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809681</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809681"/>
		<updated>2020-05-22T10:46:15Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 5) Transition state theory */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately &#039;&#039;&#039;90.77&#039;&#039;&#039; &#039;&#039;&#039;pm&#039;&#039;&#039; for the H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system.&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
For the MEP path, no vibrational motion of the formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is observed unlike in the case of dynamic mode. Over the course of the reaction, some of the initial potential energy is changed into kinetic energy. When molecular hydrogen forms, some of the kinetic energy is converted into vibrational energy, which is indicated by the oscillations on the PE surface. In the case of MEP, the reaction proceeds via a pathway with smallest possible total energy. In order to minimise the total energy, vibrational energy must be minimised as well. Consequently, no vibrational motion can be observed in this case for the MEP mode. As the MEP mode corresponds to infinitely slow motion, no changes in momenta or velocities are observed either. Furthermore, total energy of the system is not conserved in the MEP mode. The total potential energy of products is lower than the potential energy at TS but as the system has no kinetic energy at any point E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; must be equal to E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt;. This seemingly violates the law of conservation of energy, but that it is just the result of assumptions made in the MEP mode. On the other hand, energy is conserved in the dynamics mode as motion of the atoms is not taken to be infinitely slow.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as the TS structure described in question 2. Essentially, it is the reverse process of TS structure converting into products.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table below by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials even after crossing the TS due to high energy oscillations brought about by the collision, as illustrated by the different initial conditions listed in the table above. &lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The differences between TST predictions and experimental rate constant values are the direct result of assumptions made in calculations based on TST.&amp;lt;sup&amp;gt;1&amp;lt;/sup&amp;gt;&lt;br /&gt;
# The motion of nuclei is described only by classical mechanics and any quantum effects are neglected. This has a great influence on simple reactions involving light particles (H, D), as possible quantum tunneling is not taken into account. In reality, light particles can tunnel through narrow low energy barriers and this is especially likely in given simple case. Therefore in this reaction, TST is likely to underestimate the rate constant. In reactions involving more massive atoms or higher energy barriers, neglecting quantum tunneling will likely have no effect on the predicted rate constant as the probability of tunneling decreases exponentially with increasing particle mass.&lt;br /&gt;
# Conversion to products is considered to be irreversible: reactants that have reached the transition state will only proceed to form the products and not revert back to starting materials. In reality, the TS can revert back to starting materials as well. In other systems, collisions leading back to starting materials can still occur, although this will have a small effect if the forward equilibrium constant is very large. As a consequence, TST would overestimate the rate constant. &lt;br /&gt;
# The transition state structure is in quasi-equilibrium with the reactants.&lt;br /&gt;
# Translation of the nuclei can be separated from vibrational and rotational motion.&lt;br /&gt;
# The reactants and products are at a Boltzmann distribution of energies and the TS structures are sufficiently long-lived to reach Boltzmann distribution as well before converting to products.&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 436 kJ/mol, respectively.&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;  As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps) and that using a larger r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value can give a slightly smaller total energy value, but this is a sufficient approximation.&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by femtosecond absorption spectroscopy, in which molecules are excited electronically by a short laser pulse (lasting ca 1 ps) to a dissociative state. After a short interval, the excited molecule is exposed to another pulse at the absorption wavelength of one of the products. From the presence of dissociation product absorption bands and their relative intensities with respect to the excited molecule absorption bands (HF in this case), composition of gas-phase reaction mixtures can be probed.&amp;lt;sup&amp;gt;3 &amp;lt;/sup&amp;gt;In addition, vibrational or rotational spectroscopy could be used too as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* Conversion to products seems to be more likely at low p values (in the range -2 to 2 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;&#039;&#039;). Although conversion is likely at values around -6.1 and 6.1 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; &#039;&#039;as well, small changes in p value seem to have a great influence on the outcome of the reaction. On the other hand, at small initial momenta values, small changes (+-0.05 &#039;&#039;g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;&#039;&#039;) seem to have little effect on the outcome.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*The products are formed. Increasing p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; has little effect on the outcome until values of ca 2 &#039;&#039;1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In endothermic reactions, the TS occurs early in the reactant channel and in exothermic reactions, the TS occurs later in the products channel. According to Polyani&#039;s rules, the translational component of reactant energy is more important in crossing an early TS and vibrational energy is more important in overcoming a late TS.&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;  &lt;br /&gt;
&lt;br /&gt;
As illustrated by the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system, products are unlikely to form if the vibrational component of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is high and translational component is low. If H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is just busy oscillating and the collision does not occur with sufficient energy due to lack of kinetic energy of the reactants, the early TS is unlikely to be crossed.  &lt;br /&gt;
&lt;br /&gt;
Conversely, if in the reaction between H and HF the translational energy of H is large and vibrational energy of HF is small, the probability of forming products is again quite low. In order to cross the late TS, the HF bond has to have sufficient vibrational energy in order to be broken upon collision with the free H. As shown previously, the fluorine atom attracts the leaving hydrogen quite strongly so unless the HF bond oscillates heavily before the collision, H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is unlikely to be formed as the strong pull of fluorine cannot be overcome.&lt;br /&gt;
&lt;br /&gt;
As a result, reactions might not proceed even if the system has enough energy to overcome the TS barrier or to irreversibly convert to the products having crossed the TS. The key to successful reactions lies among other factors in the distribution of energy between different modes of molecular motion.&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
1. Steinfeld J. I., Francisco J. S., Hase W. L. Chemical Kinetics and Dynamics 2nd Edition, pg 315-318. Prentice-Hall.&lt;br /&gt;
&lt;br /&gt;
2. Atkins P., de Paula J. (2014) Physical Chemistry 10th Edition, pg 985. Oxford University Press.&lt;br /&gt;
&lt;br /&gt;
3. Atkins P., de Paula J. (2014) Physical Chemistry 10th Edition, pg 898. Oxford University Press.&lt;br /&gt;
&lt;br /&gt;
4. Steinfeld J. I., Francisco J. S., Hase W. L. Chemical Kinetics and Dynamics 2nd Edition, pg 272-274. Prentice-Hall.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809519</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809519"/>
		<updated>2020-05-22T09:07:53Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately &#039;&#039;&#039;90.77&#039;&#039;&#039; &#039;&#039;&#039;pm&#039;&#039;&#039; for the H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system.&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
For the MEP path, no vibrational motion of the formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is observed unlike in the case of dynamic mode. Over the course of the reaction, some of the initial potential energy is changed into kinetic energy. When molecular hydrogen forms, some of the kinetic energy is converted into vibrational energy, which is indicated by the oscillations on the PE surface. In the case of MEP, the reaction proceeds via a pathway with smallest possible total energy. In order to minimise the total energy, vibrational energy must be minimised as well. Consequently, no vibrational motion can be observed in this case for the MEP mode. As the MEP mode corresponds to infinitely slow motion, no changes in momenta or velocities are observed either. Furthermore, total energy of the system is not conserved in the MEP mode. The total potential energy of products is lower than the potential energy at TS but as the system has no kinetic energy at any point E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; must be equal to E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt;. This seemingly violates the law of conservation of energy, but that it is just the result of assumptions made in the MEP mode. On the other hand, energy is conserved in the dynamics mode as motion of the atoms is not taken to be infinitely slow.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as the TS structure described in question 2. Essentially, it is the reverse process of TS structure converting into products.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table below by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials even after crossing the TS due to high energy oscillations brought about by the collision, as illustrated by the different initial conditions listed in the table above. &lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The differences between TST predictions and experimental rate constant values are the direct result of assumptions made in calculations based on TST.&lt;br /&gt;
# The motion of nuclei is described only by classical mechanics and any quantum effects are neglected. This has a great influence on simple reactions involving light particles (H, D), as possible quantum tunneling is not taken into account. In reality, light particles can tunnel through narrow low energy barriers and this is especially likely in given simple case. Therefore in this reaction, TST is likely to underestimate the rate constant. In reactions involving more massive atoms or higher energy barriers, neglecting quantum tunneling will likely have no effect on the predicted rate constant as the probability of tunneling decreases exponentially with increasing particle mass.&lt;br /&gt;
# Conversion to products is considered to be irreversible: reactants that have reached the transition state will only proceed to form the products and not revert back to starting materials. In reality, the TS can revert back to starting materials as well. In other systems, collisions leading back to starting materials can still occur, although this will have a small effect if the forward equilibrium constant is very large. As a consequence, TST would overestimate the rate constant. &lt;br /&gt;
# The transition state structure is in quasi-equilibrium with the reactants.&lt;br /&gt;
# Translation of the nuclei can be separated from vibrational and rotational motion.&lt;br /&gt;
# The reactants and products are at a Boltzmann distribution of energies and the TS structures are sufficiently long-lived to reach Boltzmann distribution as well before converting to products.&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps). Note that using a larger r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value can give a slightly smaller total energy value, but this is a sufficient approximation.&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy and E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of free H is not very high, molecular hydrogen can be formed. &lt;br /&gt;
&lt;br /&gt;
In endothermic reactions, the TS occurs early in the reactant channel and in exothermic reactions, the TS occurs later in the products channel. According to Polyanis rules, the translational component of reactant energy is more important in crossing an early TS and vibrational energy is more important in overcoming a late TS. As a result, reactions might not proceed even if the system has enough energy to overcome the TS barrier or to irreversibly convert to the products having crossed the TS.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809135</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809135"/>
		<updated>2020-05-21T21:29:58Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
For the MEP path, no vibrational motion of the formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is observed unlike in the case of dynamic mode. Over the course of the reaction, some of the initial potential energy is changed into kinetic energy. When molecular hydrogen forms, some of the kinetic energy is converted into vibrational energy, which is indicated by the oscillations on the PE surface. In the case of MEP, the reaction proceeds via a pathway with smallest possible total energy. In order to minimise the total energy, vibrational energy must be minimised as well. Consequently, no vibrational motion can be observed in this case for the MEP mode. As the MEP mode corresponds to infinitely slow motion, no changes in momenta or velocities are observed either. Furthermore, total energy of the system is not conserved in the MEP mode. The total potential energy of products is lower than the potential energy at TS but as the system has no kinetic energy at any point E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; must be equal to E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt;. This seemingly violates the law of conservation of energy, but actually it is just a result of the assumptions made in the MEP mode. On the other hand, energy is conserved like normally in the dynamics mode as motion of the atoms is not taken to be infinitely slow.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The differences between TST predictions and experimental rate constant values are the direct result of assumptions made in calculations based on TST.&lt;br /&gt;
# The motion of nuclei is described only by classical mechanics and any quantum effects are neglected. This has a great influence on simple reactions involving light particles (H, D), as possible quantum tunneling is not taken into account. In reality, light particles can tunnel through narrow low energy barriers and this is especially likely in given simple case. Therefore in this reaction, TST is likely to underestimate the rate constant. In reactions involving more massive atoms or higher energy barriers, neglecting quantum tunneling will likely have no effect on the predicted rate constant as the probability of tunneling decreases exponentially with increasing particle mass.&lt;br /&gt;
# Conversion to products is considered to be irreversible: reactants that have reached the transition state will only proceed to form the products and not revert back to starting materials. In reality, the TS can revert back to starting materials as well. In other systems, collisions leading back to starting materials can still occur, although this will have a small effect if the forward equilibrium constant is very large. As a consequence, TST would overestimate the rate constant. &lt;br /&gt;
# The transition state structure is in quasi-equilibrium with the reactants.&lt;br /&gt;
# Translation of the nuclei can be separated from vibrational and rotational motion.&lt;br /&gt;
# The reactants and products are at a Boltzmann distribution of energies and the TS structures are sufficiently long-lived to reach Boltzmann distribution as well before converting to products.&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps). Note that using a larger r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value can give a slightly smaller total energy value, but this is a sufficient approximation.&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy and E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of free H is not very high, molecular hydrogen can be formed. &lt;br /&gt;
&lt;br /&gt;
In endothermic reactions, the TS occurs early in the reactant channel and in exothermic reactions, the TS occurs later in the products channel. According to Polyanis rules, the translational component of reactant energy is more important in crossing an early TS and vibrational energy is more important in overcoming a late TS. As a result, reactions might not proceed even if the system has enough energy to overcome the TS barrier or to irreversibly convert to the products having crossed the TS.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809060</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=809060"/>
		<updated>2020-05-21T20:22:16Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 5) Transition state theory */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
For the MEP path, no vibrational motion of the formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is observed unlike in the case of dynamic mode. Over the course of the reaction, some of the initial potential energy is changed into kinetic energy. When molecular hydrogen forms, some of the kinetic energy is converted into vibrational energy, which is indicated by the oscillations on the PE surface. In the case of MEP, the reaction proceeds via a pathway with smallest possible total energy. In order to minimise the total energy, vibrational energy must be minimised as well. Consequently, no vibrational motion can be observed in this case for the MEP mode. As the MEP mode corresponds to infinitely slow motion, no changes in momenta or velocities are observed either. Furthermore, total energy of the system is not conserved in the MEP mode. The total potential energy of products is lower than the potential energy at TS but as the system has no kinetic energy at any point E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; must be equal to E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt;. This seemingly violates the law of conservation of energy, but actually it is just a result of the assumptions made in the MEP mode. On the other hand, energy is conserved like normally in the dynamics mode as motion of the atoms is not taken to be infinitely slow.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The differences between TST predictions and experimental rate constant values are the direct result of assumptions made in calculations based on TST.&lt;br /&gt;
# The motion of nuclei is described only by classical mechanics and any quantum effects are neglected. This has a great influence on simple reactions involving light particles (H, D), as possible quantum tunneling is not taken into account. In reality, light particles can tunnel through narrow low energy barriers and this is especially likely in given simple case. Therefore in this reaction, TST is likely to underestimate the rate constant. In reactions involving more massive atoms or higher energy barriers, neglecting quantum tunneling will likely have no effect on the predicted rate constant as the probability of tunneling decreases exponentially with increasing particle mass.&lt;br /&gt;
# Conversion to products is considered to be irreversible: reactants that have reached the transition state will only proceed to form the products and not revert back to starting materials. In reality, the TS can revert back to starting materials as well. In other systems, collisions leading back to starting materials can still occur, although this will have a small effect if the forward equilibrium constant is very large. As a consequence, TST would overestimate the rate constant. &lt;br /&gt;
# The transition state structure is in quasi-equilibrium with the reactants.&lt;br /&gt;
# Translation of the nuclei can be separated from vibrational and rotational motion.&lt;br /&gt;
# The reactants and products are at a Boltzmann distribution of energies and the TS structures are sufficiently long-lived to reach Boltzmann distribution as well before converting to products.&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps). Note that using a larger r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value can give a slightly smaller total energy value, but this is a sufficient approximation.&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808942</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808942"/>
		<updated>2020-05-21T19:00:52Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 5) Transition state theory */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
For the MEP path, no vibrational motion of the formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is observed unlike in the case of dynamic mode. Over the course of the reaction, some of the initial potential energy is changed into kinetic energy. When molecular hydrogen forms, some of the kinetic energy is converted into vibrational energy, which is indicated by the oscillations on the PE surface. In the case of MEP, the reaction proceeds via a pathway with smallest possible total energy. In order to minimise the total energy, vibrational energy must be minimised as well. Consequently, no vibrational motion can be observed in this case for the MEP mode. As the MEP mode corresponds to infinitely slow motion, no changes in momenta or velocities are observed either. Furthermore, total energy of the system is not conserved in the MEP mode. The total potential energy of products is lower than the potential energy at TS but as the system has no kinetic energy at any point E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; must be equal to E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt;. This seemingly violates the law of conservation of energy, but actually it is just a result of the assumptions made in the MEP mode. On the other hand, energy is conserved like normally in the dynamics mode as motion of the atoms is not taken to be infinitely slow.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The differences between TST predictions and experimental rate constant values are the direct result of assumptions made in calculations based on TST.&lt;br /&gt;
# In TST, the motion of nuclei is described only by classical mechanics and any quantum effects are neglected. This has a great influence on simple reactions involving light particles (H, D, e&amp;lt;sup&amp;gt;-&amp;lt;/sup&amp;gt;), as possible quantum tunneling is not taken into account. In reality, light particles can tunnel through narrow low energy barriers and this is especially likely in given simple case. Therefore in this reaction, TST is likely to underestimate the rate constant. In reactions involving more massive atoms or higher energy barriers, neglecting quantum tunneling will likely have no effect on the predicted rate constant as the probability of tunneling decreases exponentially with increasing particle mass.&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808527</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808527"/>
		<updated>2020-05-21T14:45:15Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 3) MEP&amp;amp;dynamic trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
For the MEP path, no vibrational motion of the formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is observed unlike in the case of dynamic mode. Over the course of the reaction, some of the initial potential energy is changed into kinetic energy. When molecular hydrogen forms, some of the kinetic energy is converted into vibrational energy, which is indicated by the oscillations on the PE surface. In the case of MEP, the reaction proceeds via a pathway with smallest possible total energy. In order to minimise the total energy, vibrational energy must be minimised as well. Consequently, no vibrational motion can be observed in this case for the MEP mode. As the MEP mode corresponds to infinitely slow motion, no changes in momenta or velocities are observed either. Furthermore, total energy of the system is not conserved in the MEP mode. The total potential energy of products is lower than the potential energy at TS but as the system has no kinetic energy at any point E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; must be equal to E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt;. This seemingly violates the law of conservation of energy, but actually it is just a result of the assumptions made in the MEP mode. On the other hand, energy is conserved like normally in the dynamics mode as motion of the atoms is not taken to be infinitely slow.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808492</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808492"/>
		<updated>2020-05-21T14:15:43Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 3) MEP&amp;amp;dynamic trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
For the MEP path, no vibrational motion of the formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; is observed unlike in the case of dynamic mode. Over the course of the reaction, some of the initial potential energy is changed into kinetic energy. When molecular hydrogen forms, some of the kinetic energy is converted into vibrational energy, which is indicated by the oscillations on the PE surface. In the case of MEP, the reaction proceeds via a pathway with smallest possible total energy. In order to minimise the total energy, vibrational energy must be minimised as well. Consequently, no vibrational motion can be observed in this case for the MEP mode.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808428</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808428"/>
		<updated>2020-05-21T13:39:33Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 3) MEP&amp;amp;dynamic trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 dynamics INdistvstime.png|thumb|350px|center|Internuclear distances vs time]]&lt;br /&gt;
| [[File:01502946 Ex1 dynamics momentavstime.png|thumb|350px|center|Momenta vs time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:01502946_Ex1_dynamics_momentavstime.png&amp;diff=808426</id>
		<title>File:01502946 Ex1 dynamics momentavstime.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:01502946_Ex1_dynamics_momentavstime.png&amp;diff=808426"/>
		<updated>2020-05-21T13:38:53Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
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		<author><name>Sk7118</name></author>
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		<title>File:01502946 Ex1 dynamics INdistvstime.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:01502946_Ex1_dynamics_INdistvstime.png&amp;diff=808420"/>
		<updated>2020-05-21T13:37:16Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
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	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808406</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808406"/>
		<updated>2020-05-21T13:29:15Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 3) MEP&amp;amp;dynamic trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
| [[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808404</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808404"/>
		<updated>2020-05-21T13:28:45Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 3) MEP&amp;amp;dynamic trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
[[File:01502946 Ex1 valleyfloorDynamics.png|thumb|350px|center|Reaction path by the dynamics mode]]&lt;br /&gt;
[[File:01502946 Ex1 valleyfloorMEP.png|thumb|350px|center|Reaction path by the MEP mode]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:01502946_Ex1_valleyfloorMEP.png&amp;diff=808402</id>
		<title>File:01502946 Ex1 valleyfloorMEP.png</title>
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		<updated>2020-05-21T13:28:06Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
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	<entry>
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		<title>File:01502946 Ex1 valleyfloorDynamics.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:01502946_Ex1_valleyfloorDynamics.png&amp;diff=808398"/>
		<updated>2020-05-21T13:26:28Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
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	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808395</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808395"/>
		<updated>2020-05-21T13:25:16Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 4) A reactive F + H2 trajectory */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2.png|thumb|300px|center|The reactive path]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|thumb|350px|center|Energy as a function of time]]&lt;br /&gt;
| [[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|thumb|300px|center|Momenta of the species as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
*&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808389</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808389"/>
		<updated>2020-05-21T13:23:04Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 2) F + H2 TS position */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre|Location of the TS]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
[[File:01502946 Ex2 reactivepathFplusH2.png|300px]][[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|350px]][[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|300px]]&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808387</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808387"/>
		<updated>2020-05-21T13:22:21Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 2) H + H2 TS position */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
{|style=&amp;quot;margin: 0 auto;&amp;quot;&lt;br /&gt;
| [[File:01502946 Ex1 transition state contourplot.png|thumb|320px|center|Location of the TS]]&lt;br /&gt;
| [[File:01502946 Ex1 TS distvtime.png|thumb|400px|center|Distances as a function of time]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
[[File:01502946 Ex2 reactivepathFplusH2.png|300px]][[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|350px]][[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|300px]]&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808377</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808377"/>
		<updated>2020-05-21T13:10:59Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Question 2) H + H2 TS position */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 transition state contourplot.png|350px]][[File:01502946 Ex1 TS distvtime.png|400px]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
[[File:01502946 Ex2 reactivepathFplusH2.png|300px]][[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|350px]][[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|300px]]&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:01502946_Ex1_transition_state_contourplot.png&amp;diff=808375</id>
		<title>File:01502946 Ex1 transition state contourplot.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:01502946_Ex1_transition_state_contourplot.png&amp;diff=808375"/>
		<updated>2020-05-21T13:09:48Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808354</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808354"/>
		<updated>2020-05-21T12:54:41Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Exercise 1. */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2 ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
[[File:01502946 Ex2 reactivepathFplusH2.png|300px]][[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|350px]][[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|300px]]&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808353</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808353"/>
		<updated>2020-05-21T12:54:04Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== &#039;&#039;&#039;Exercise 1.&#039;&#039;&#039; ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) MEP&amp;amp;dynamic trajectories ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question 4) A nice table ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question 5) Transition state theory ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== &#039;&#039;&#039;Exercise 2&#039;&#039;&#039; ==&lt;br /&gt;
&lt;br /&gt;
=== Question 1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question 2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
=== Question 3) Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question 4) A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
[[File:01502946 Ex2 reactivepathFplusH2.png|300px]][[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|350px]][[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|300px]]&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question 5) Distribution of energy ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808349</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808349"/>
		<updated>2020-05-21T12:50:21Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&lt;br /&gt;
=== Question &#039;&#039;&#039;1)&#039;&#039;&#039; Definition of the TS ===&lt;br /&gt;
&#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
=== Question &#039;&#039;&#039;2) H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
=== Question &#039;&#039;&#039;3) MEP&amp;amp;dynamic trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;&#039;Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== Question &#039;&#039;&#039;4) A nice table&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
=== Question &#039;&#039;&#039;5) Transition state theory&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;&#039;Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&lt;br /&gt;
=== Question &#039;&#039;&#039;1) Energetics of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;&#039;By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
=== Question &#039;&#039;&#039;2) F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; TS position&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;&#039;Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
=== Question &#039;&#039;&#039;3)&#039;&#039;&#039; Activation energies ===&lt;br /&gt;
&#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reaction dynamics&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
=== Question &#039;&#039;&#039;4)&#039;&#039;&#039; A reactive F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; trajectory ===&lt;br /&gt;
&#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
[[File:01502946 Ex2 reactivepathFplusH2.png|300px]][[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|350px]][[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|300px]]&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Question 5) Distribution of energy&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;&#039;Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808326</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808326"/>
		<updated>2020-05-21T12:42:11Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Exercise 2. */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;  (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF (&#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
[[File:01502946 Ex2 reactivepathFplusH2.png|300px]][[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|350px]][[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|300px]]&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808318</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808318"/>
		<updated>2020-05-21T12:39:10Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reaction dynamics */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;      &#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF     &#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
[[File:01502946 Ex2 reactivepathFplusH2.png|300px]][[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|350px]][[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|300px]]&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808313</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808313"/>
		<updated>2020-05-21T12:37:07Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reaction dynamics */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;      &#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF     &#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
[[File:01502946 Ex2 reactivepathFplusH2.png|300px]][[File:01502946 Ex2 reactivepathFplusH2 energyvstime.png|300px]][[File:01502946 Ex2 reactivepathFplusH2 momentavstime.png|300px]]&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:01502946_Ex2_reactivepathFplusH2_momentavstime.png&amp;diff=808307</id>
		<title>File:01502946 Ex2 reactivepathFplusH2 momentavstime.png</title>
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		<updated>2020-05-21T12:35:54Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
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		<title>File:01502946 Ex2 reactivepathFplusH2 energyvstime.png</title>
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		<updated>2020-05-21T12:34:59Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
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		<title>File:01502946 Ex2 reactivepathFplusH2.png</title>
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		<updated>2020-05-21T12:33:43Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
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	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808256</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808256"/>
		<updated>2020-05-21T12:15:20Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Exercise 1. */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* The reactants must be sufficiently high in energy for the reaction to occur, but their energy must be also be suitably distributed between translational and vibrational forms. Otherwise, the reaction can possibly revert back to starting materials due to high energy oscillations brough about by the collision, as illustrated by the different initial conditions listed in the table above.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;      &#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF     &#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808202</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808202"/>
		<updated>2020-05-21T12:00:23Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reaction dynamics */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 181 pm&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74.5 pm&#039;&#039;&#039;, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;      &#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;0.995 kJ/mol&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Reaction:  H + HF     &#039;&#039;&#039;E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; =&#039;&#039;&#039; &#039;&#039;&#039;126.57 kJ/mol&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The activation energies were determined with the help of energy vs time plots by the following procedure.&lt;br /&gt;
# Firstly, the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 74 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 300 pm) on the &amp;quot;starting materials valley&amp;quot; floor was determined. This corresponded to the total energy of starting materials before the reaction (E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt;). The r values correspond to a H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule at equilibrium bond length and a fluorine atom far away from H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Note that p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 (same in further steps).&lt;br /&gt;
# Secondly, the total energy at TS (E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt;) was determined (see the previous question).&lt;br /&gt;
# Finally the total energy at an arbitrarily chosen position (r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 300 pm, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 91.7 pm) on the &amp;quot;products valley&amp;quot; floor was determined. This corresponded to the total energy of products after the reaction (E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;). The r values correspond to a HF molecule at equilibrium bond length and an hydrogen atom far away from HF.&lt;br /&gt;
The difference between E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;SM&amp;lt;/sub&amp;gt; was then calculated to yield the activation energy of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. The activation energy of the reverse reaction was found similarly for E&amp;lt;sub&amp;gt;TS&amp;lt;/sub&amp;gt; and E&amp;lt;sub&amp;gt;PR&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;. The figure below illustrates the outcome of reaction F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808165</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808165"/>
		<updated>2020-05-21T11:44:30Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reaction dynamics */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C). The figure below illustrates the outcome of reaction F + H2 at the following initial conditions: &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808164</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808164"/>
		<updated>2020-05-21T11:43:51Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Exercise 2. */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer). The equilibrium bond lengths of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF are r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; = 74 pm and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; = 91.7 pm, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; The large difference between r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;HF&amp;lt;/sub&amp;gt; and small difference between r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;H2&amp;lt;/sub&amp;gt; indicates an early transition state as the TS structure is highly similar to the starting materials. The reaction is exothermic and an early TS is also predicted by the Hammond postulate: the TS structure (and its energy) must be similar to starting materials (and their energy) as the reaction cannot proceed before the energy barrier leading to the TS has been crossed.[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C). The figure below illustrates the outcome of reaction F + H2 at the following initial conditions: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808067</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=808067"/>
		<updated>2020-05-21T10:47:41Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Exercise 2. */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
In this case, &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
At the transition states, all repulsive and attractive forces are balanced. Consequently, E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; = E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const.&lt;br /&gt;
&lt;br /&gt;
Such conditions are satisfied at: r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm, given p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. This result was obtained through trial and error, but the TS could also be located through decreasing the spacing between isoenergetic contour lines and searching for the saddle point (although in this case even the smallest spacing does not give a very precise answer).[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C). The figure below illustrates the outcome of reaction F + H2 at the following initial conditions: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807986</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807986"/>
		<updated>2020-05-21T10:12:49Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
* All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
* The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. The units for p are g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;What can you conclude from the table?&#039;&#039;&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H, therefore r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm&lt;br /&gt;
[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Similarly to 2), &#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H and therefore  r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C). The figure below illustrates the outcome of reaction F + H2 at the following initial conditions: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 180 pm,  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -1.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 74 pm,    &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = -0.4 g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: the step number must be set higher than 500 at size 0.1 fs to see the outcome.&lt;br /&gt;
&lt;br /&gt;
As the initial momenta are relatively small, the potential energy is approximately equal to the total energy. Initially, there is a small component of kinetic energy, but as the initial momenta are small, its contribution is negligible. As H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; approaches F, the kinetic energy component increases quickly. When HF is formed and atomic hydrogen departs, a portion of the potential energy is converted into vibrational energy. The potential and kinetic energy components change accordingly as the formed diatomic molecule oscillates. The H-F oscillations are considerably stronger than the initial H-H oscillations. Note that the potential energy does not reach the total energy value as the atomic hydrogen will have kinetic energy as well. As the single proton cannot undergo vibrational motion on its own and no force acts upon it (due to increasing r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; value), it will move with constant velocity and therefore constant kinetic energy.&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy as H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and HF give distinct bands in the spectra. This is due to the excitation frequencies of H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; being higher than those of HF as fluorine is ca 19x more massive than hydrogen. It is known from spectroscopy that v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; ∝ √(k/μ) and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ, where vvib and vrot are vibrational and rotational frequencies (Hz), respectively, k is the bond force constant and μ is the reduced mass of the diatomic species. As μ(H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;)&amp;lt;μ(HF), both the values of v&amp;lt;sub&amp;gt;vib &amp;lt;/sub&amp;gt;and v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; are expected to be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. Although k(H2)&amp;lt;k(HF), the difference in reduced masses outweighs the difference in force constants and v&amp;lt;sub&amp;gt;vib&amp;lt;/sub&amp;gt; will nevertheless be greater for H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
NB: The relationship v&amp;lt;sub&amp;gt;rot&amp;lt;/sub&amp;gt; ∝ 1/μ assumes a rigid rotor model, but experimentally any centrifugal distortions must be taken into account.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807964</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807964"/>
		<updated>2020-05-21T09:21:44Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reactive and unreactive trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. (g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory. What can you conclude from the table?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H, therefore r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm&lt;br /&gt;
[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 180 pm ;  p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = -1.4&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74 pm ; p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = -0.4&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807963</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807963"/>
		<updated>2020-05-21T09:21:04Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reactive and unreactive trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory. What can you conclude from the table?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H, therefore r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm&lt;br /&gt;
[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 180 pm ;  p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = -1.4&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74 pm ; p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = -0.4&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807962</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807962"/>
		<updated>2020-05-21T09:20:34Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reactive and unreactive trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;&lt;br /&gt;
into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between&lt;br /&gt;
H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory. What can you conclude from the table?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H, therefore r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm&lt;br /&gt;
[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 180 pm ;  p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = -1.4&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74 pm ; p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = -0.4&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807961</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807961"/>
		<updated>2020-05-21T09:20:08Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reactive and unreactive trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision &lt;br /&gt;
with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;&lt;br /&gt;
into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between&lt;br /&gt;
H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory. What can you conclude from the table?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H, therefore r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm&lt;br /&gt;
[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 180 pm ;  p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = -1.4&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74 pm ; p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = -0.4&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807960</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807960"/>
		<updated>2020-05-21T09:19:06Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reactive and unreactive trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product having high vibrational energy, the starting materials are reformed. The vibrational energy is illustrated by the high energy oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory. What can you conclude from the table?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H, therefore r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm&lt;br /&gt;
[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 180 pm ;  p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = -1.4&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74 pm ; p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = -0.4&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807959</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807959"/>
		<updated>2020-05-21T09:17:48Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reactive and unreactive trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The collision occurs with sufficient energy and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly formed dihydrogen oscillates more heavily than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material (i.e|p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;|) is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy&lt;br /&gt;
&lt;br /&gt;
to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product&lt;br /&gt;
&lt;br /&gt;
having high vibrational energy, the starting &lt;br /&gt;
&lt;br /&gt;
materials are reformed. The vibrational&lt;br /&gt;
&lt;br /&gt;
energy is illustrated by the high energy&lt;br /&gt;
&lt;br /&gt;
oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed. However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory. What can you conclude from the table?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H, therefore r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm&lt;br /&gt;
[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 180 pm ;  p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = -1.4&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74 pm ; p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = -0.4&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807953</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807953"/>
		<updated>2020-05-21T08:52:12Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reactive and unreactive trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The&lt;br /&gt;
&lt;br /&gt;
collision occurs with sufficient energy and&lt;br /&gt;
&lt;br /&gt;
H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly&lt;br /&gt;
&lt;br /&gt;
formed dihydrogen oscillates more heavily &lt;br /&gt;
&lt;br /&gt;
than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material (i.e |p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;|) is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy&lt;br /&gt;
&lt;br /&gt;
to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product&lt;br /&gt;
&lt;br /&gt;
having high vibrational energy, the starting &lt;br /&gt;
&lt;br /&gt;
materials are reformed. The vibrational&lt;br /&gt;
&lt;br /&gt;
energy is illustrated by the high energy&lt;br /&gt;
&lt;br /&gt;
oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed.&lt;br /&gt;
However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory. What can you conclude from the table?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H, therefore r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm&lt;br /&gt;
[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 180 pm ;  p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = -1.4&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74 pm ; p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = -0.4&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807952</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807952"/>
		<updated>2020-05-21T08:50:44Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reactive and unreactive trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The&lt;br /&gt;
&lt;br /&gt;
collision occurs with sufficient energy and&lt;br /&gt;
&lt;br /&gt;
H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly&lt;br /&gt;
&lt;br /&gt;
formed dihydrogen oscillates more heavily &lt;br /&gt;
&lt;br /&gt;
than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material (i.e |p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;|) is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy&lt;br /&gt;
&lt;br /&gt;
to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product&lt;br /&gt;
&lt;br /&gt;
having high vibrational energy, the starting &lt;br /&gt;
&lt;br /&gt;
materials are reformed. The vibrational&lt;br /&gt;
&lt;br /&gt;
energy is illustrated by the high energy&lt;br /&gt;
&lt;br /&gt;
oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed.&lt;br /&gt;
However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays relatively close to the molecule. Upon stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is&lt;br /&gt;
&lt;br /&gt;
reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;. &lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory. What can you conclude from the table?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H, therefore r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm&lt;br /&gt;
[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 180 pm ;  p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = -1.4&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74 pm ; p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = -0.4&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807951</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807951"/>
		<updated>2020-05-21T08:46:57Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reactive and unreactive trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not energetic enough to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The&lt;br /&gt;
&lt;br /&gt;
collision occurs with sufficient energy and&lt;br /&gt;
&lt;br /&gt;
H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly&lt;br /&gt;
&lt;br /&gt;
formed dihydrogen oscillates more heavily &lt;br /&gt;
&lt;br /&gt;
than the initial molecule. The reaction proceeds via a slightly higher energy pathway than in the first case, as the vibrational energy of the starting material (i.e |p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;|) is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy&lt;br /&gt;
&lt;br /&gt;
to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product&lt;br /&gt;
&lt;br /&gt;
having high vibrational energy, the starting &lt;br /&gt;
&lt;br /&gt;
materials are reformed. The vibrational&lt;br /&gt;
&lt;br /&gt;
energy is illustrated by the high energy&lt;br /&gt;
&lt;br /&gt;
oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with &lt;br /&gt;
sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is&lt;br /&gt;
&lt;br /&gt;
small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high&lt;br /&gt;
&lt;br /&gt;
energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed.&lt;br /&gt;
&lt;br /&gt;
However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a&lt;br /&gt;
&lt;br /&gt;
high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays&lt;br /&gt;
&lt;br /&gt;
in relatively close to the molecule. Upon&lt;br /&gt;
&lt;br /&gt;
stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is&lt;br /&gt;
&lt;br /&gt;
reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single &lt;br /&gt;
&lt;br /&gt;
atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.&lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory. What can you conclude from the table?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H, therefore r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm&lt;br /&gt;
[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 180 pm ;  p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = -1.4&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74 pm ; p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = -0.4&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807950</id>
		<title>MRD:01502946</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:01502946&amp;diff=807950"/>
		<updated>2020-05-21T08:42:50Z</updated>

		<summary type="html">&lt;p&gt;Sk7118: /* Reactive and unreactive trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Questions in blue colour raised in the lab script are written here in &#039;&#039;&#039;bold&#039;&#039;&#039; and numbered, rest of the questions are in &#039;&#039;cursive&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
== Exercise 1. ==&lt;br /&gt;
&#039;&#039;&#039;1)&#039;&#039;&#039; &#039;&#039;&#039;On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The transition state is defined as the maximum located on a minimum energy path. Mathematically, it is a saddle point on the potential energy surface. At TS coordinates, 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&#039;&#039;x&#039;&#039; = 0 and 𝛿&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿y = 0, where in this case x and y are r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; in this case. Additionally at TS coordinates, the second partial derivative with respect to one coordinate must be positive and negative with respect to the other coordinate, i.e either 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;y&#039;&#039; &amp;lt; 0 or 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;lt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;y &amp;gt; 0. This fact allows the saddle point to be simply distinguished from a local minimum as at the latter, both 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x&#039;&#039; &amp;gt; 0 and 𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;V&#039;&#039;(&#039;&#039;x,y&#039;&#039;)/𝛿&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&#039;&#039;x &#039;&#039;&amp;gt; 0.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2)&#039;&#039;&#039; &#039;&#039;&#039;Report your best estimate of the transition state position&#039;&#039;&#039; (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) &#039;&#039;&#039;and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; and p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 0, the atoms are expected to stay still and not oscillate as the attractive and repulsive forces are perfectly balanced. Therefore, E&amp;lt;sub&amp;gt;kin&amp;lt;/sub&amp;gt; of the atoms will be 0, given such initial conditions and E&amp;lt;sub&amp;gt;pot&amp;lt;/sub&amp;gt; = const., as illustrated by the figure below. The TS coordinates can also be estimated by the surface plot and the reaction trajectory, which at mentioned initial conditions will converge into a single spot on the Epot surface, which is the transition state. Using this method, r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; was estimated to be equal to approximately 90.77 pm. Therefore, the transition state would be located at &#039;&#039;V&#039;&#039;(90.77,90.77).&lt;br /&gt;
[[File:01502946 Ex1 TS distvtime.png|centre|thumb]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3) Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Look at the “Internuclear Distances vs Time” and “Momenta vs Time”. What would change if we used the initial conditions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039; and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = &#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;+1 pm instead?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
All three atoms are the same elements and only the definitions of r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; are interchanged, therefore the outcome of the reaction will still be chemically the same. The only difference is that the chemical bond will be formed between the hydrogen in the middle and the proton that previously ended up as a free atom (instead of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;  --&amp;gt; H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, we get H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; + H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;). On Internuclear Dist. vs Time and Momenta vs Time plots, the lines which previously represented parameters associated with r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; now represent r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt; and vice versa (see figures below).&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Take note of the final values of the positions &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) and  &#039;&#039;&#039;p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) &#039;&#039;&#039;p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039;(t) for your trajectory for large enough t. Setup a calculation where the initial positions correspond to the final positions of the trajectory you calculated above, the same final momenta values but with their signs reversed. What do you observe?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The atoms return from the products to the transition state and stay there as three atoms. Essentially, it is the reverse of the previous reaction.&lt;br /&gt;
&lt;br /&gt;
=== &#039;&#039;&#039;Reactive and unreactive trajectories&#039;&#039;&#039; ===&lt;br /&gt;
&#039;&#039;Is there a general way to determine the conditions for a reactive trajectory that starts in the region of the reactants and passes near the TS region?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;4) Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;&#039;&#039;Note:&#039;&#039;&#039;&#039;&#039; In this case, r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; correspond to r&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; and r&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, respectively. H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt;&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
!p&amp;lt;sub&amp;gt;1 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!p&amp;lt;sub&amp;gt;2 &amp;lt;/sub&amp;gt;(g·mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;·pm·fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;)&lt;br /&gt;
!E&amp;lt;sub&amp;gt;tot&amp;lt;/sub&amp;gt; (kJ/mol)&lt;br /&gt;
!Reactive?&lt;br /&gt;
!Description of the dynamics&lt;br /&gt;
!Illustration of the trajectory&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-2.56&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-414.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has very little vibrational energy. &lt;br /&gt;
&lt;br /&gt;
Collision with H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; occurs with sufficient energy&lt;br /&gt;
&lt;br /&gt;
to convert H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, which oscillates&lt;br /&gt;
&lt;br /&gt;
slightly as the distance between H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and the&lt;br /&gt;
&lt;br /&gt;
newly formed H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; increases.&lt;br /&gt;
|[[File:01502946 Ex1 table condition1.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-4.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-420.08&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|No&lt;br /&gt;
|The collision of H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; of H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is not sufficiently&lt;br /&gt;
&lt;br /&gt;
energetic to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The energy barrier&lt;br /&gt;
&lt;br /&gt;
is not crossed and the H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; molecule continues&lt;br /&gt;
&lt;br /&gt;
oscillating as H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; recedes.&lt;br /&gt;
|[[File:01502946 Ex1 table condition2.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-3.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-413.98&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; has some vibrational energy. The&lt;br /&gt;
&lt;br /&gt;
collision occurs with sufficient energy and&lt;br /&gt;
&lt;br /&gt;
H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is converted into H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The newly&lt;br /&gt;
&lt;br /&gt;
formed dihydrogen oscillates more heavily &lt;br /&gt;
&lt;br /&gt;
than the initial molecule. The reaction proceeds&lt;br /&gt;
&lt;br /&gt;
via a slightly higher energy pathway than in&lt;br /&gt;
&lt;br /&gt;
the first case, as the vibrational energy of the&lt;br /&gt;
&lt;br /&gt;
starting material (i.e |p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;|) is greater.&lt;br /&gt;
|[[File:01502946 Ex1 table condition3.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-357.27&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Well yes, &lt;br /&gt;
but no.&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A-B&amp;lt;/sub&amp;gt; with sufficient energy&lt;br /&gt;
&lt;br /&gt;
to form H&amp;lt;sub&amp;gt;B-C&amp;lt;/sub&amp;gt;, but as a result of the product&lt;br /&gt;
&lt;br /&gt;
having high vibrational energy, the starting &lt;br /&gt;
&lt;br /&gt;
materials are reformed. The vibrational&lt;br /&gt;
&lt;br /&gt;
energy is illustrated by the high energy&lt;br /&gt;
&lt;br /&gt;
oscillations seen in the figure on the right.&lt;br /&gt;
|[[File:01502946 Ex1 table condition4.png|350px|]]&lt;br /&gt;
|-&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-5.1&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-10.6&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|&amp;lt;nowiki&amp;gt;-349.48&amp;lt;/nowiki&amp;gt;&lt;br /&gt;
|Yes&lt;br /&gt;
|H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; collides with H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; once again with &lt;br /&gt;
sufficient energy to form H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;, but as r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; is&lt;br /&gt;
&lt;br /&gt;
small enough and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; undergoes high&lt;br /&gt;
&lt;br /&gt;
energy oscillations, H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; is reformed.&lt;br /&gt;
&lt;br /&gt;
However, in this case H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; experiences a&lt;br /&gt;
&lt;br /&gt;
high attractive force to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; and stays&lt;br /&gt;
&lt;br /&gt;
in relatively close to the molecule. Upon&lt;br /&gt;
&lt;br /&gt;
stretching of the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt; bond, H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C &amp;lt;/sub&amp;gt;is&lt;br /&gt;
&lt;br /&gt;
reformed and H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; departs as a single &lt;br /&gt;
&lt;br /&gt;
atom. H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; oscillates heavily, but attractive&lt;br /&gt;
&lt;br /&gt;
forces to H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; decrease continuously due &lt;br /&gt;
&lt;br /&gt;
to increasing r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;.&lt;br /&gt;
|[[File:01502946 Ex1 table condition5.png|350px|]]&lt;br /&gt;
|}&lt;br /&gt;
&#039;&#039;Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory. What can you conclude from the table?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
== Exercise 2. ==&lt;br /&gt;
&#039;&#039;&#039;1) By inspecting the potential energy surfaces, classify the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
The reaction between &#039;&#039;&#039;F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; (reaction 1) is endothermic, as the energy of the products (HF + H) is higher than that of the reactants. Conversely, the reaction &#039;&#039;&#039;H + HF&#039;&#039;&#039; (reaction 2) is endothermic, as the products are lower in energy than the reactants. The bond energies of H-F and H-H bonds are 565 kJ/mol and 432 kJ/mol, respectively.&amp;lt;sup&amp;gt;ref&amp;lt;/sup&amp;gt; As the H-F bond is stronger than the H-H bond, energy is released as heat upon formation of HF from F and H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;. In the reverse reaction, more energy is needed to put into breaking of the H-F bond, which results in the reaction being endothermic.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;2) Locate the approximate position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;A&#039;&#039;&#039; = F, &#039;&#039;&#039;B&#039;&#039;&#039; = &#039;&#039;&#039;C&#039;&#039;&#039; = H, therefore r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r(A-B) and r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r(B-C)&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;=181 pm&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;=74.5 pm&lt;br /&gt;
[[File:01502946 Ex2 FplusH2 TSloc.png|thumb|centre]]&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;3)&#039;&#039;&#039; &#039;&#039;&#039;Report the activation energy for both reactions.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 0.995 kJ/mol&lt;br /&gt;
&lt;br /&gt;
H + HF E&amp;lt;sub&amp;gt;a&amp;lt;/sub&amp;gt; = 126.57 kJ/mol&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&#039;&#039;&#039;4)&#039;&#039;&#039; &#039;&#039;&#039;Identify a set of initial conditions that results in a reactive trajectory for the F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, and look at the “Animation” and “Momenta vs Time”.&#039;&#039;&#039; &#039;&#039;&#039;In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = 180 pm ;  p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = -1.4&lt;br /&gt;
&lt;br /&gt;
r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = 74 pm ; p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = -0.4&lt;br /&gt;
&lt;br /&gt;
Experimentally, the reaction could be confirmed by vibrational or rotational spectroscopy.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;Setup a calculation starting on the side of the reactants of F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;, at the bottom of the well r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 74 pm, with a momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.0 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and explore several values of p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; in the range -6.1 to 6.1 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt; (explore values also close to these limits). What do you observe? Note that we are putting a significant amount of energy (much more than the activation energy) into the system on the H - H vibration.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For the same initial position, increase slightly the momentum p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1.6 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;, and considerably reduce the overall energy of the system by reducing the momentum p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.2 g.mol&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;.pm.fs&amp;lt;sup&amp;gt;-1&amp;lt;/sup&amp;gt;. What do you observe now?&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;5) Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
If HF has very low vibrational energy and H has very high translational energy, the most likely outcome of the reaction is that H splits HF into single atoms and no molecular hydrogen forms. On the other hand, if HF has moderate vibrational energy (p=0.2) and Ekin of free H is lower (p=-16.10), molecular hydrogen can be formed.&lt;/div&gt;</summary>
		<author><name>Sk7118</name></author>
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