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		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=723383</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=723383"/>
		<updated>2018-05-18T15:39:22Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances by testing of range of equal distances between the H atoms with 0 momentum and checking if the reaction trajectory still goes to the bottom of the well or stays still. This is easily seen in the internuclear distance vs time plot for the transition state, where the A-B and B-C distance lines overlap completely and show very little oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|350x350px|center|Figure 1: Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|300x300px|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|300x300px|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions were reversed?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|350x350px|thumb|centre|Figure 4: Reversal of final conditions]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources&amp;lt;ref&amp;gt;Atkins, P., de Paula, J., Elements of Physical Chemistry, 5th ed.; Oxford University Press, 2009.&amp;lt;/ref&amp;gt;: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 5 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|350x350px|center|Figure 5: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;br /&gt;
&lt;br /&gt;
For the F + H-H reaction, a MEP calculation has been made from r(F-H)=1.9 Å and r(H-H)=0.75 Å, and the final energy after 2500 has been determined to be -104.008 kcal/mol, which would lead to an activation energy in this direction of 0.256 kcal/mol. &lt;br /&gt;
In an analogue manner, a calculation was run from r(F-H)=1.8 Å and r(H-H)=0.8 Å, and the final energy after 25 seconds was -133.727 kcal/mol. The activation energy in this direction is then 29.975 kcal/mol.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. How could this be confirmed experimentally?}}&lt;br /&gt;
&lt;br /&gt;
The reaction is exothermic, so an excess of energy is produced. From the Animation result, it is quite obvious that the system contains more energy after the H-F molecule is formed, since it oscillates much quicker than the H-H molecule. Since this is quite a simple system and energy must be conserved, it is then obvious that the excess reaction energy is present in the system as vibrational energy. The momentum vs time plot in Figure 6 shows the H-H (B-C) and H-F (A-B) being quickly deformed at the transition state, after which the oscillating H-F momentum is large and constant while the H-H momentum is lost. &lt;br /&gt;
This gain of vibrational energy is also evident in the energy vs time plot in Figure 7, where this excess energy is interplayed between the kinetic and the potential terms periodically. Experimentally, this could be determined using calorimetry to determined the amount of heat energy lost to the environment due to vibrations or through IR spectroscopy, following the intensity of the H-F band over time.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_12.png|thumb|300x300px|left|Figure 6: F+H-H momentum vs time plot]][[File:RCR16_13.png|thumb|300x300px|center|Figure 7:F+H-H energy vs time plot]]&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|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.}}&lt;br /&gt;
&lt;br /&gt;
Polanyi&#039;s empirical rules state that reaching a late transition state can be reached more efficiently by increasing the vibrational energy of the system rather than its translational energy, while the opposite applies for early transition state&amp;lt;ref&amp;gt;Z. Zhang, Y. Zhou, D. H. Zhang, G. Czakó and J. M. Bowman, &#039;&#039;J. Phys. Chem. Lett.&#039;&#039;, 2012, &#039;&#039;&#039;3&#039;&#039;&#039;, 3416–3419.&amp;lt;/ref&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Since the F+ H-H is exothermic, it has an early transition state. Setting r(F-H)=2 Å and r(H-H)=0.74 Å, p(F-H)=-0.5 and p(H-H)=0.1, the reaction goes smoothly to products. This is the case for high translational energy and low vibrational energy and can be seen in Figure 8. When we alter p(H-H) to 2.4 or more, the system gains so much vibrational energy that the reaction goes back to reagents even though the translational energy was enough to cross the energy barrier. Figure 9 shows this case, and it proves the Polanyi assumptions about an early transition state correct.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_15.png|thumb|300x300px|left|Figure 8: Surface plot of high translational E, low vibrational E for F + H-H]][[File:RCR16_16.png|thumb|300x300px|center|Figure 9: Surface plot for low translational E, low vibrational E for F + H-H]]&lt;br /&gt;
&lt;br /&gt;
For the H-F + H reaction, the situation should be reversed, since it has a late transition state. Setting r(F-H)=0.92 Å and r(H-H)=2.0 Å, a low p(H-F)=-0.1, no matter how high the absolute value of p(H-H) is chosen, the reaction won&#039;t take place. Figure 10 shows the case for p(H-H)=-5, a very high translational energy leading to no reaction. Now setting a very low p(H-H)=-0.1 and increasing the vibrational energy by setting p(H-F) up to -10, successful reaction trajectories can be obtained, one of them being shown in Figure 11. Thus, the Polanyi predictions for a late transition state have been confirmed as well.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_18.png|thumb|300x300px|left|Figure 10: Surface plot of high translational E, low vibrational E for H + H-F]][[File:RCR16_17.png|thumb|350x350px|center|Figure 11: Surface plot for low translational E, low vibrational E for H + H-F]]&lt;br /&gt;
&lt;br /&gt;
== References  ==&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=723377</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=723377"/>
		<updated>2018-05-18T15:38:33Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* Trajectories from r1 = r2: locating the transition state */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances by testing of range of equal distances between the H atoms with 0 momentum and checking if the reaction trajectory still goes to the bottom of the well or stays still. This is easily seen in the internuclear distance vs time plot for the transition state, where the A-B and B-C distance lines overlap completely and show very little oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|350x350px|center|Figure 1: Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|300x300px|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|300x300px|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions were reversed?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|350x350px|thumb|centre|Figure 4: Reversal of final conditions]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources&amp;lt;ref&amp;gt;Atkins, P., de Paula, J., Elements of Physical Chemistry, 5th ed.; Oxford University Press, 2009.&amp;lt;/ref&amp;gt;: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 5 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|350x350px|center|Figure 5: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;br /&gt;
&lt;br /&gt;
For the F + H-H reaction, a MEP calculation has been made from r(F-H)=1.9 Å and r(H-H)=0.75 Å, and the final energy after 2500 has been determined to be -104.008 kcal/mol, which would lead to an activation energy in this direction of 0.256 kcal/mol. &lt;br /&gt;
In an analogue manner, a calculation was run from r(F-H)=1.8 Å and r(H-H)=0.8 Å, and the final energy after 25 seconds was -133.727 kcal/mol. The activation energy in this direction is then 29.975 kcal/mol.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. How could this be confirmed experimentally?}}&lt;br /&gt;
&lt;br /&gt;
The reaction is exothermic, so an excess of energy is produced. From the Animation result, it is quite obvious that the system contains more energy after the H-F molecule is formed, since it oscillates much quicker than the H-H molecule. Since this is quite a simple system and energy must be conserved, it is then obvious that the excess reaction energy is present in the system as vibrational energy. The momentum vs time plot in Figure 6 shows the H-H (B-C) and H-F (A-B) being quickly deformed at the transition state, after which the oscillating H-F momentum is large and constant while the H-H momentum is lost. &lt;br /&gt;
This gain of vibrational energy is also evident in the energy vs time plot in Figure 7, where this excess energy is interplayed between the kinetic and the potential terms periodically. Experimentally, this could be determined using calorimetry to determined the amount of heat energy lost to the environment due to vibrations or through IR spectroscopy, following the intensity of the H-F band over time.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_12.png|thumb|300x300px|left|Figure 6: F+H-H momentum vs time plot]][[File:RCR16_13.png|thumb|300x300px|center|Figure 7:F+H-H energy vs time plot]]&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|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.}}&lt;br /&gt;
&lt;br /&gt;
Polanyi&#039;s empirical rules state that reaching a late transition state can be reached more efficiently by increasing the vibrational energy of the system rather than its translational energy, while the opposite applies for early transition state&amp;lt;ref&amp;gt;Z. Zhang, Y. Zhou, D. H. Zhang, G. Czakó and J. M. Bowman, &#039;&#039;J. Phys. Chem. Lett.&#039;&#039;, 2012, &#039;&#039;&#039;3&#039;&#039;&#039;, 3416–3419.&amp;lt;/ref&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Since the F+ H-H is exothermic, it has an early transition state. Setting r(F-H)=2 Å and r(H-H)=0.74 Å, p(F-H)=-0.5 and p(H-H)=0.1, the reaction goes smoothly to products. This is the case for high translational energy and low vibrational energy and can be seen in Figure 8. When we alter p(H-H) to 2.4 or more, the system gains so much vibrational energy that the reaction goes back to reagents even though the translational energy was enough to cross the energy barrier. Figure 9 shows this case, and it proves the Polanyi assumptions about an early transition state correct.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_15.png|thumb|300x300px|left|Figure 8: Surface plot of high translational E, low vibrational E for F + H-H]][[File:RCR16_16.png|thumb|300x300px|center|Figure 9: Surface plot for low translational E, low vibrational E for F + H-H]]&lt;br /&gt;
&lt;br /&gt;
For the H-F + H reaction, the situation should be reversed, since it has a late transition state. Setting r(F-H)=0.92 Å and r(H-H)=2.0 Å, a low p(H-F)=-0.1, no matter how high the absolute value of p(H-H) is chosen, the reaction won&#039;t take place. Figure 10 shows the case for p(H-H)=-5, a very high translational energy leading to no reaction. Now setting a very low p(H-H)=-0.1 and increasing the vibrational energy by setting p(H-F) up to -10, successful reaction trajectories can be obtained, one of them being shown in Figure 11. Thus, the Polanyi predictions for a late transition state have been confirmed as well.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_18.png|thumb|300x300px|left|Figure 10: Surface plot of high translational E, low vibrational E for H + H-F]][[File:RCR16_17.png|thumb|350x350px|center|Figure 11: Surface plot for low translational E, low vibrational E for H + H-F]]&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719959</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719959"/>
		<updated>2018-05-17T15:02:12Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|350x350px|center|Figure 1: Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|300x300px|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|300x300px|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions were reversed?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|350x350px|thumb|centre|Figure 4: Reversal of final conditions]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources&amp;lt;ref&amp;gt;Atkins, P., de Paula, J., Elements of Physical Chemistry, 5th ed.; Oxford University Press, 2009.&amp;lt;/ref&amp;gt;: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 5 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|350x350px|center|Figure 5: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;br /&gt;
&lt;br /&gt;
For the F + H-H reaction, a MEP calculation has been made from r(F-H)=1.9 Å and r(H-H)=0.75 Å, and the final energy after 2500 has been determined to be -104.008 kcal/mol, which would lead to an activation energy in this direction of 0.256 kcal/mol. &lt;br /&gt;
In an analogue manner, a calculation was run from r(F-H)=1.8 Å and r(H-H)=0.8 Å, and the final energy after 25 seconds was -133.727 kcal/mol. The activation energy in this direction is then 29.975 kcal/mol.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. How could this be confirmed experimentally?}}&lt;br /&gt;
&lt;br /&gt;
The reaction is exothermic, so an excess of energy is produced. From the Animation result, it is quite obvious that the system contains more energy after the H-F molecule is formed, since it oscillates much quicker than the H-H molecule. Since this is quite a simple system and energy must be conserved, it is then obvious that the excess reaction energy is present in the system as vibrational energy. The momentum vs time plot in Figure 6 shows the H-H (B-C) and H-F (A-B) being quickly deformed at the transition state, after which the oscillating H-F momentum is large and constant while the H-H momentum is lost. &lt;br /&gt;
This gain of vibrational energy is also evident in the energy vs time plot in Figure 7, where this excess energy is interplayed between the kinetic and the potential terms periodically. Experimentally, this could be determined using calorimetry to determined the amount of heat energy lost to the environment due to vibrations or through IR spectroscopy, following the intensity of the H-F band over time.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_12.png|thumb|300x300px|left|Figure 6: F+H-H momentum vs time plot]][[File:RCR16_13.png|thumb|300x300px|center|Figure 7:F+H-H energy vs time plot]]&lt;br /&gt;
&lt;br /&gt;
=== Reaction dynamics ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|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.}}&lt;br /&gt;
&lt;br /&gt;
Polanyi&#039;s empirical rules state that reaching a late transition state can be reached more efficiently by increasing the vibrational energy of the system rather than its translational energy, while the opposite applies for early transition state&amp;lt;ref&amp;gt;Z. Zhang, Y. Zhou, D. H. Zhang, G. Czakó and J. M. Bowman, &#039;&#039;J. Phys. Chem. Lett.&#039;&#039;, 2012, &#039;&#039;&#039;3&#039;&#039;&#039;, 3416–3419.&amp;lt;/ref&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Since the F+ H-H is exothermic, it has an early transition state. Setting r(F-H)=2 Å and r(H-H)=0.74 Å, p(F-H)=-0.5 and p(H-H)=0.1, the reaction goes smoothly to products. This is the case for high translational energy and low vibrational energy and can be seen in Figure 8. When we alter p(H-H) to 2.4 or more, the system gains so much vibrational energy that the reaction goes back to reagents even though the translational energy was enough to cross the energy barrier. Figure 9 shows this case, and it proves the Polanyi assumptions about an early transition state correct.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_15.png|thumb|300x300px|left|Figure 8: Surface plot of high translational E, low vibrational E for F + H-H]][[File:RCR16_16.png|thumb|300x300px|center|Figure 9: Surface plot for low translational E, low vibrational E for F + H-H]]&lt;br /&gt;
&lt;br /&gt;
For the H-F + H reaction, the situation should be reversed, since it has a late transition state. Setting r(F-H)=0.92 Å and r(H-H)=2.0 Å, a low p(H-F)=-0.1, no matter how high the absolute value of p(H-H) is chosen, the reaction won&#039;t take place. Figure 10 shows the case for p(H-H)=-5, a very high translational energy leading to no reaction. Now setting a very low p(H-H)=-0.1 and increasing the vibrational energy by setting p(H-F) up to -10, successful reaction trajectories can be obtained, one of them being shown in Figure 11. Thus, the Polanyi predictions for a late transition state have been confirmed as well.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_18.png|thumb|300x300px|left|Figure 10: Surface plot of high translational E, low vibrational E for H + H-F]][[File:RCR16_17.png|thumb|350x350px|center|Figure 11: Surface plot for low translational E, low vibrational E for H + H-F]]&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719929</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719929"/>
		<updated>2018-05-17T14:59:51Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|350x350px|center|Figure 1: Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|300x300px|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|300x300px|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions were reversed?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|350x350px|thumb|centre|Figure 4: Reversal of final conditions]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources&amp;lt;ref&amp;gt;Atkins, P., de Paula, J., Elements of Physical Chemistry, 5th ed.; Oxford University Press, 2009.&amp;lt;/ref&amp;gt;: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 5 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|350x350px|center|Figure 5: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;br /&gt;
&lt;br /&gt;
For the F + H-H reaction, a MEP calculation has been made from r(F-H)=1.9 Å and r(H-H)=0.75 Å, and the final energy after 2500 has been determined to be -104.008 kcal/mol, which would lead to an activation energy in this direction of 0.256 kcal/mol. &lt;br /&gt;
In an analogue manner, a calculation was run from r(F-H)=1.8 Å and r(H-H)=0.8 Å, and the final energy after 25 seconds was -133.727 kcal/mol. The activation energy in this direction is then 29.975 kcal/mol.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. How could this be confirmed experimentally?}}&lt;br /&gt;
&lt;br /&gt;
The reaction is exothermic, so an excess of energy is produced. From the Animation result, it is quite obvious that the system contains more energy after the H-F molecule is formed, since it oscillates much quicker than the H-H molecule. Since this is quite a simple system and energy must be conserved, it is then obvious that the excess reaction energy is present in the system as vibrational energy. The momentum vs time plot in Figure 6 shows the H-H (B-C) and H-F (A-B) being quickly deformed at the transition state, after which the oscillating H-F momentum is large and constant while the H-H momentum is lost. &lt;br /&gt;
This gain of vibrational energy is also evident in the energy vs time plot in Figure 7, where this excess energy is interplayed between the kinetic and the potential terms periodically. Experimentally, this could be determined using calorimetry to determined the amount of heat energy lost to the environment due to vibrations or through IR spectroscopy, following the intensity of the H-F band over time.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_12.png|thumb|300x300px|left|Figure 6: F+H-H momentum vs time plot]][[File:RCR16_13.png|thumb|300x300px|center|Figure 7:F+H-H energy vs time plot]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|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.}}&lt;br /&gt;
&lt;br /&gt;
Polanyi&#039;s empirical rules state that reaching a late transition state can be reached more efficiently by increasing the vibrational energy of the system rather than its translational energy, while the opposite applies for early transition state&amp;lt;ref&amp;gt;Z. Zhang, Y. Zhou, D. H. Zhang, G. Czakó and J. M. Bowman, &#039;&#039;J. Phys. Chem. Lett.&#039;&#039;, 2012, &#039;&#039;&#039;3&#039;&#039;&#039;, 3416–3419.&amp;lt;/ref&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Since the F+ H-H is exothermic, it has an early transition state. Setting r(F-H)=2 Å and r(H-H)=0.74 Å, p(F-H)=-0.5 and p(H-H)=0.1, the reaction goes smoothly to products. This is the case for high translational energy and low vibrational energy and can be seen in Figure 8. When we alter p(H-H) to 2.4 or more, the system gains so much vibrational energy that the reaction goes back to reagents even though the translational energy was enough to cross the energy barrier. Figure 9 shows this case, and it proves the Polanyi assumptions about an early transition state correct.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_15.png|thumb|300x300px|left|Figure 8: Surface plot of high translational E, low vibrational E for F + H-H]][[File:RCR16_16.png|thumb|300x300px|center|Figure 9: Surface plot for low translational E, low vibrational E for F + H-H]]&lt;br /&gt;
&lt;br /&gt;
For the H-F + H reaction, the situation should be reversed, since it has a late transition state. Setting r(F-H)=0.92 Å and r(H-H)=2.0 Å, a low p(H-F)=-0.1, no matter how high the absolute value of p(H-H) is chosen, the reaction won&#039;t take place. Figure 10 shows the case for p(H-H)=-5, a very high translational energy leading to no reaction. Now setting a very low p(H-H)=-0.1 and increasing the vibrational energy by setting p(H-F) up to -10, successful reaction trajectories can be obtained, one of them being shown in Figure 11. Thus, the Polanyi predictions for a late transition state have been confirmed as well.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_18.png|thumb|300x300px|left|Figure 10: Surface plot of high translational E, low vibrational E for H + H-F]][[File:RCR16_17.png|thumb|350x350px|center|Figure 11: Surface plot for low translational E, low vibrational E for H + H-F]]&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719887</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719887"/>
		<updated>2018-05-17T14:56:23Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|350x350px|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|350x350px|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|350x350px|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions r1 = rts and  r2 = rts+0.01 instead?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|thumb|centre|Figure 4]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources&amp;lt;ref&amp;gt;Atkins, P., de Paula, J., Elements of Physical Chemistry, 5th ed.; Oxford University Press, 2009.&amp;lt;/ref&amp;gt;: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 5 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|350x350px|center|Figure 5: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;br /&gt;
&lt;br /&gt;
For the F + H-H reaction, a MEP calculation has been made from r(F-H)=1.9 Å and r(H-H)=0.75 Å, and the final energy after 2500 has been determined to be -104.008 kcal/mol, which would lead to an activation energy in this direction of 0.256 kcal/mol. &lt;br /&gt;
In an analogue manner, a calculation was run from r(F-H)=1.8 Å and r(H-H)=0.8 Å, and the final energy after 25 seconds was -133.727 kcal/mol. The activation energy in this direction is then 29.975 kcal/mol.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. How could this be confirmed experimentally?}}&lt;br /&gt;
&lt;br /&gt;
The reaction is exothermic, so an excess of energy is produced. From the Animation result, it is quite obvious that the system contains more energy after the H-F molecule is formed, since it oscillates much quicker than the H-H molecule. Since this is quite a simple system and energy must be conserved, it is then obvious that the excess reaction energy is present in the system as vibrational energy. The momentum vs time plot in Figure 6 shows the H-H (B-C) and H-F (A-B) being quickly deformed at the transition state, after which the oscillating H-F momentum is large and constant while the H-H momentum is lost. &lt;br /&gt;
This gain of vibrational energy is also evident in the energy vs time plot in Figure 7, where this excess energy is interplayed between the kinetic and the potential terms periodically. Experimentally, this could be determined using calorimetry to determined the amount of heat energy lost to the environment due to vibrations or through IR spectroscopy, following the intensity of the H-F band over time.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_12.png|thumb|350x350px|left|Figure 6: F+H-H momentum vs time plot]][[File:RCR16_13.png|thumb|350x350px|center|Figure 7:F+H-H energy vs time plot]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|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.}}&lt;br /&gt;
&lt;br /&gt;
Polanyi&#039;s empirical rules state that reaching a late transition state can be reached more efficiently by increasing the vibrational energy of the system rather than its translational energy, while the opposite applies for early transition state&amp;lt;ref&amp;gt;Z. Zhang, Y. Zhou, D. H. Zhang, G. Czakó and J. M. Bowman, &#039;&#039;J. Phys. Chem. Lett.&#039;&#039;, 2012, &#039;&#039;&#039;3&#039;&#039;&#039;, 3416–3419.&amp;lt;/ref&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Since the F+ H-H is exothermic, it has an early transition state. Setting r(F-H)=2 Å and r(H-H)=0.74 Å, p(F-H)=-0.5 and p(H-H)=0.1, the reaction goes smoothly to products. This is the case for high translational energy and low vibrational energy and can be seen in Figure 8. When we alter p(H-H) to 2.4 or more, the system gains so much vibrational energy that the reaction goes back to reagents even though the translational energy was enough to cross the energy barrier. Figure 9 shows this case, and it proves the Polanyi assumptions about an early transition state correct.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_15.png|thumb|350x350px|left|Figure 8: Surface plot of high translational E, low vibrational E for F + H-H]][[File:RCR16_16.png|thumb|350x350px|center|Figure 9: Surface plot for low translational E, low vibrational E for F + H-H]]&lt;br /&gt;
&lt;br /&gt;
For the H-F + H reaction, the situation should be reversed, since it has a late transition state. Setting r(F-H)=0.92 Å and r(H-H)=2.0 Å, a low p(H-F)=-0.1, no matter how high the absolute value of p(H-H) is chosen, the reaction won&#039;t take place. Figure 10 shows the case for p(H-H)=-5, a very high translational energy leading to no reaction. Now setting a very low p(H-H)=-0.1 and increasing the vibrational energy by setting p(H-F) up to -10, successful reaction trajectories can be obtained, one of them being shown in Figure 11. Thus, the Polanyi predictions for a late transition state have been confirmed as well.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_18.png|thumb|350x350px|left|Figure 10: Surface plot of high translational E, low vibrational E for H + H-F]][[File:RCR16_17.png|thumb|350x350px|center|Figure 11: Surface plot for low translational E, low vibrational E for H + H-F]]&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719851</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719851"/>
		<updated>2018-05-17T14:53:29Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* EXERCISE 2: F - H - H system */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions r1 = rts and  r2 = rts+0.01 instead?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|thumb|centre|Figure 4]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources&amp;lt;ref&amp;gt;Atkins, P., de Paula, J., Elements of Physical Chemistry, 5th ed.; Oxford University Press, 2009.&amp;lt;/ref&amp;gt;: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 5 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 5: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;br /&gt;
&lt;br /&gt;
For the F + H-H reaction, a MEP calculation has been made from r(F-H)=1.9 Å and r(H-H)=0.75 Å, and the final energy after 2500 has been determined to be -104.008 kcal/mol, which would lead to an activation energy in this direction of 0.256 kcal/mol. &lt;br /&gt;
In an analogue manner, a calculation was run from r(F-H)=1.8 Å and r(H-H)=0.8 Å, and the final energy after 25 seconds was -133.727 kcal/mol. The activation energy in this direction is then 29.975 kcal/mol.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. How could this be confirmed experimentally?}}&lt;br /&gt;
&lt;br /&gt;
The reaction is exothermic, so an excess of energy is produced. From the Animation result, it is quite obvious that the system contains more energy after the H-F molecule is formed, since it oscillates much quicker than the H-H molecule. Since this is quite a simple system and energy must be conserved, it is then obvious that the excess reaction energy is present in the system as vibrational energy. The momentum vs time plot in Figure 6 shows the H-H (B-C) and H-F (A-B) being quickly deformed at the transition state, after which the oscillating H-F momentum is large and constant while the H-H momentum is lost. &lt;br /&gt;
This gain of vibrational energy is also evident in the energy vs time plot in Figure 7, where this excess energy is interplayed between the kinetic and the potential terms periodically. Experimentally, this could be determined using calorimetry to determined the amount of heat energy lost to the environment due to vibrations or through IR spectroscopy, following the intensity of the H-F band over time.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_12.png|thumb|left|Figure 6: F+H-H momentum vs time plot]][[File:RCR16_13.png|thumb|center|Figure 7:F+H-H energy vs time plot]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|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.}}&lt;br /&gt;
&lt;br /&gt;
Polanyi&#039;s empirical rules state that reaching a late transition state can be reached more efficiently by increasing the vibrational energy of the system rather than its translational energy, while the opposite applies for early transition state&amp;lt;ref&amp;gt;Z. Zhang, Y. Zhou, D. H. Zhang, G. Czakó and J. M. Bowman, &#039;&#039;J. Phys. Chem. Lett.&#039;&#039;, 2012, &#039;&#039;&#039;3&#039;&#039;&#039;, 3416–3419.&amp;lt;/ref&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Since the F+ H-H is exothermic, it has an early transition state. Setting r(F-H)=2 Å and r(H-H)=0.74 Å, p(F-H)=-0.5 and p(H-H)=0.1, the reaction goes smoothly to products. This is the case for high translational energy and low vibrational energy and can be seen in Figure 8. When we alter p(H-H) to 2.4 or more, the system gains so much vibrational energy that the reaction goes back to reagents even though the translational energy was enough to cross the energy barrier. Figure 9 shows this case, and it proves the Polanyi assumptions about an early transition state correct.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_15.png|thumb|left|Figure 8: Surface plot of high translational E, low vibrational E for F + H-H]][[File:RCR16_16.png|thumb|center|Figure 9: Surface plot for low translational E, low vibrational E for F + H-H]]&lt;br /&gt;
&lt;br /&gt;
For the H-F + H reaction, the situation should be reversed, since it has a late transition state. Setting r(F-H)=0.92 Å and r(H-H)=2.0 Å, a low p(H-F)=-0.1, no matter how high the absolute value of p(H-H) is chosen, the reaction won&#039;t take place. Figure 10 shows the case for p(H-H)=-5, a very high translational energy leading to no reaction. Now setting a very low p(H-H)=-0.1 and increasing the vibrational energy by setting p(H-F) up to -10, successful reaction trajectories can be obtained, one of them being shown in Figure 11. Thus, the Polanyi predictions for a late transition state have been confirmed as well.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_18.png|thumb|left|Figure 10: Surface plot of high translational E, low vibrational E for H + H-F]][[File:RCR16_17.png|thumb|center|Figure 11: Surface plot for low translational E, low vibrational E for H + H-F]]&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_18.png&amp;diff=719848</id>
		<title>File:RCR16 18.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_18.png&amp;diff=719848"/>
		<updated>2018-05-17T14:53:05Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_17.png&amp;diff=719843</id>
		<title>File:RCR16 17.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_17.png&amp;diff=719843"/>
		<updated>2018-05-17T14:52:34Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719832</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719832"/>
		<updated>2018-05-17T14:52:00Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions r1 = rts and  r2 = rts+0.01 instead?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|thumb|centre|Figure 4]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources&amp;lt;ref&amp;gt;Atkins, P., de Paula, J., Elements of Physical Chemistry, 5th ed.; Oxford University Press, 2009.&amp;lt;/ref&amp;gt;: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 5 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 5: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;br /&gt;
&lt;br /&gt;
For the F + H-H reaction, a MEP calculation has been made from r(F-H)=1.9 Å and r(H-H)=0.75 Å, and the final energy after 2500 has been determined to be -104.008 kcal/mol, which would lead to an activation energy in this direction of 0.256 kcal/mol. &lt;br /&gt;
In an analogue manner, a calculation was run from r(F-H)=1.8 Å and r(H-H)=0.8 Å, and the final energy after 25 seconds was -133.727 kcal/mol. The activation energy in this direction is then 29.975 kcal/mol.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. How could this be confirmed experimentally?}}&lt;br /&gt;
&lt;br /&gt;
The reaction is exothermic, so an excess of energy is produced. From the Animation result, it is quite obvious that the system contains more energy after the H-F molecule is formed, since it oscillates much quicker than the H-H molecule. Since this is quite a simple system and energy must be conserved, it is then obvious that the excess reaction energy is present in the system as vibrational energy. The momentum vs time plot in Figure 6 shows the H-H (B-C) and H-F (A-B) being quickly deformed at the transition state, after which the oscillating H-F momentum is large and constant while the H-H momentum is lost. &lt;br /&gt;
This gain of vibrational energy is also evident in the energy vs time plot in Figure 7, where this excess energy is interplayed between the kinetic and the potential terms periodically. Experimentally, this could be determined using calorimetry to determined the amount of heat energy lost to the environment due to vibrations or through IR spectroscopy, following the intensity of the H-F band over time.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_12.png|thumb|left|Figure 6: F+H-H momentum vs time plot]][[File:RCR16_13.png|thumb|center|Figure 7:F+H-H energy vs time plot]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|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.}}&lt;br /&gt;
&lt;br /&gt;
Polanyi&#039;s empirical rules state that reaching a late transition state can be reached more efficiently by increasing the vibrational energy of the system rather than its translational energy, while the opposite applies for early transition state&amp;lt;ref&amp;gt;Z. Zhang, Y. Zhou, D. H. Zhang, G. Czakó and J. M. Bowman, &#039;&#039;J. Phys. Chem. Lett.&#039;&#039;, 2012, &#039;&#039;&#039;3&#039;&#039;&#039;, 3416–3419.&amp;lt;/ref&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
Since the F+ H-H is exothermic, it has an early transition state. Setting r(F-H)=2 Å and r(H-H)=0.74 Å, p(F-H)=-0.5 and p(H-H)=0.1, the reaction goes smoothly to products. This is the case for high translational energy and low vibrational energy and can be seen in Figure 8. When we alter p(H-H) to 2.4 or more, the system gains so much vibrational energy that the reaction goes back to reagents even though the translational energy was enough to cross the energy barrier. Figure 9 shows this case, and it proves the Polanyi assumptions about an early transition state correct.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_15.png|thumb|left|Figure 8: Surface plot of high translational E, low vibrational E for F + H-H]][[File:RCR16_16.png|thumb|center|Figure 9: Surface plot for low translational E, low vibrational E for F + H-H]]&lt;br /&gt;
&lt;br /&gt;
For the H-F + H reaction, the situation should be reversed, since it has a late transition state. Setting r(F-H)=0.92 Å and r(H-H)=2.0 Å, a low p(H-F)=-0.1, no matter how high the absolute value of p(H-H) is chosen, the reaction won&#039;t take place. Figure 10 shows the case for p(H-H)=-5, a very high translational energy leading to no reaction. Now setting a very low p(H-H)=-0.1 and increasing the vibrational energy by setting p(H-F) up to -10, successful reaction trajectories can be obtained, one of them being shown in Figure 11. Thus, the Polanyi predictions for a late transition state have been confirmed as well.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_17.png|thumb|left|Figure 10: Surface plot of high translational E, low vibrational E for H + H-F]][[File:RCR16_18.png|thumb|center|Figure 11: Surface plot for low translational E, low vibrational E for H + H-F]]&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_16.png&amp;diff=719600</id>
		<title>File:RCR16 16.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_16.png&amp;diff=719600"/>
		<updated>2018-05-17T14:31:02Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_15.png&amp;diff=719598</id>
		<title>File:RCR16 15.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_15.png&amp;diff=719598"/>
		<updated>2018-05-17T14:30:43Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719305</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719305"/>
		<updated>2018-05-17T13:58:13Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions r1 = rts and  r2 = rts+0.01 instead?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|thumb|centre|Figure 4]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 5 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 5: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;br /&gt;
&lt;br /&gt;
For the F + H-H reaction, a MEP calculation has been made from r(F-H)=1.9 Å and r(H-H)=0.75 Å, and the final energy after 2500 has been determined to be -104.008 kcal/mol, which would lead to an activation energy in this direction of 0.256 kcal/mol. &lt;br /&gt;
In an analogue manner, a calculation was run from r(F-H)=1.8 Å and r(H-H)=0.8 Å, and the final energy after 25 seconds was -133.727 kcal/mol. The activation energy in this direction is then 29.975 kcal/mol.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. How could this be confirmed experimentally?}}&lt;br /&gt;
&lt;br /&gt;
The reaction is exothermic, so an excess of energy is produced. From the Animation result, it is quite obvious that the system contains more energy after the H-F molecule is formed, since it oscillates much quicker than the H-H molecule. Since this is quite a simple system and energy must be conserved, it is then obvious that the excess reaction energy is present in the system as vibrational energy. The momentum vs time plot in Figure 6 shows the H-H (B-C) and H-F (A-B) being quickly deformed at the transition state, after which the oscillating H-F momentum is large and constant while the H-H momentum is lost. &lt;br /&gt;
This gain of vibrational energy is also evident in the energy vs time plot in Figure 7, where this excess energy is interplayed between the kinetic and the potential terms periodically. Experimentally, this could be determined using calorimetry to determined the amount of heat energy lost to the environment due to vibrations or through IR spectroscopy, following the intensity of the H-F band over time.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_12.png|thumb|left|Figure 6: F+H-H momentum vs time plot]][[File:RCR16_13.png|thumb|center|Figure 7:F+H-H energy vs time plot]]&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719288</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719288"/>
		<updated>2018-05-17T13:56:42Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* EXERCISE 2: F - H - H system */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions r1 = rts and  r2 = rts+0.01 instead?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|thumb|centre|Figure 4]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 5: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;br /&gt;
&lt;br /&gt;
For the F + H-H reaction, a MEP calculation has been made from r(F-H)=1.9 Å and r(H-H)=0.75 Å, and the final energy after 2500 has been determined to be -104.008 kcal/mol, which would lead to an activation energy in this direction of 0.256 kcal/mol. &lt;br /&gt;
In an analogue manner, a calculation was run from r(F-H)=1.8 Å and r(H-H)=0.8 Å, and the final energy after 25 seconds was -133.727 kcal/mol. The activation energy in this direction is then 29.975 kcal/mol.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. How could this be confirmed experimentally?}}&lt;br /&gt;
&lt;br /&gt;
The reaction is exothermic, so an excess of energy is produced. From the Animation result, it is quite obvious that the system contains more energy after the H-F molecule is formed, since it oscillates much quicker than the H-H molecule. Since this is quite a simple system and energy must be conserved, it is then obvious that the excess reaction energy is present in the system as vibrational energy. The momentum vs time plot in Figure 6 shows the H-H (B-C) and H-F (A-B) being quickly deformed at the transition state, after which the oscillating H-F momentum is large and constant while the H-H momentum is lost. &lt;br /&gt;
This gain of vibrational energy is also evident in the energy vs time plot in Figure 7, where this excess energy is interplayed between the kinetic and the potential terms periodically. Experimentally, this could be determined using calorimetry to determined the amount of heat energy lost to the environment due to vibrations or through IR spectroscopy, following the intensity of the H-F band over time.&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_13.png&amp;diff=719227</id>
		<title>File:RCR16 13.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_13.png&amp;diff=719227"/>
		<updated>2018-05-17T13:49:41Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_12.png&amp;diff=719221</id>
		<title>File:RCR16 12.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_12.png&amp;diff=719221"/>
		<updated>2018-05-17T13:49:18Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719132</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=719132"/>
		<updated>2018-05-17T13:42:46Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* EXERCISE 2: F - H - H system */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions r1 = rts and  r2 = rts+0.01 instead?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|thumb|centre|Figure 4]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 5: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;br /&gt;
&lt;br /&gt;
For the F + H-H reaction, a MEP calculation has been made from r(F-H)=1.9 Å and r(H-H)=0.75 Å, and the final energy after 2500 has been determined to be -104.008 kcal/mol, which would lead to an activation energy in this direction of 0.256 kcal/mol. &lt;br /&gt;
In an analogue manner, a calculation was run from r(F-H)=1.8 Å and r(H-H)=0.8 Å, and the final energy after 25 seconds was -133.727 kcal/mol. The activation energy in this direction is then 29.975 kcal/mol.&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718995</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718995"/>
		<updated>2018-05-17T13:30:18Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* EXERCISE 2: F - H - H system */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions r1 = rts and  r2 = rts+0.01 instead?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|thumb|centre|Figure 4]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 5: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718988</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718988"/>
		<updated>2018-05-17T13:29:43Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* Trajectories from r1 = rts+δ, r2 = rts */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| What would change if we used the initial conditions r1 = rts and  r2 = rts+0.01 instead?}} The reaction would take place in the opposite direction.&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| 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?}} The reaction system reaches very close to the transition state but doesn&#039;t have enough energy to cross barrier, so it returns back to products, as seen in Figure 4.&lt;br /&gt;
[[File:RCR16_11.png|thumb|centre|Figure 4]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 4: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_11.png&amp;diff=718968</id>
		<title>File:RCR16 11.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_11.png&amp;diff=718968"/>
		<updated>2018-05-17T13:27:41Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718879</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718879"/>
		<updated>2018-05-17T13:19:35Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* PES inspection */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 4: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718875</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718875"/>
		<updated>2018-05-17T13:19:15Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* Trajectories from r1 = rts+δ, r2 = rts */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 4: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718871</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718871"/>
		<updated>2018-05-17T13:18:59Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* Trajectories from r1 = r2: locating the transition state */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 4: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718870</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718870"/>
		<updated>2018-05-17T13:18:50Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 4: Internuclear distance vs time plot for F H H transition state]]&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Report the activation energy for both reactions.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718859</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718859"/>
		<updated>2018-05-17T13:17:39Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
{{fontcolor|blue|What value do the different components of the gradient of the potential energy surface have at a minimum and at a transition structure? Briefly explain how minima and transition structures can be distinguished using the curvature of the potential energy surface.}}&lt;br /&gt;
&lt;br /&gt;
The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Report your best estimate of the transition state position (&#039;&#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;&#039;&#039;&#039;) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.}}&lt;br /&gt;
&lt;br /&gt;
The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
{{fontcolor1|blue|Comment on how the &#039;&#039;mep&#039;&#039; and the trajectory you just calculated differ.}}&lt;br /&gt;
&lt;br /&gt;
The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
{{fontcolor1|blue|Complete the table by adding a column with the total energy, and another column reporting if the trajectory is reactive or unreactive. For each set of initial conditions, provide a plot of the trajectory and a small description for what happens along the trajectory.}}&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|State what are the main assumptions of Transition State Theory. Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?}}&lt;br /&gt;
&lt;br /&gt;
Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. &lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
{{fontcolor1|blue|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?}}&lt;br /&gt;
&lt;br /&gt;
The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  &lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|Locate the approximate position of the transition state.}}&lt;br /&gt;
&lt;br /&gt;
Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 4: Internuclear distance vs time plot for F H H transition state]]&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718753</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718753"/>
		<updated>2018-05-17T13:06:05Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* Trajectories from r1 = r2: locating the transition state */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.908 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2x.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.}}&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 4: Internuclear distance vs time plot for F H H transition state]]&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_2x.png&amp;diff=718744</id>
		<title>File:RCR16 2x.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_2x.png&amp;diff=718744"/>
		<updated>2018-05-17T13:05:22Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: x&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;x&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718588</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718588"/>
		<updated>2018-05-17T12:46:54Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* EXERCISE 2: F - H - H system */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.907 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.}}&lt;br /&gt;
[[File:RCR16_10.png|thumb|center|Figure 4: Internuclear distance vs time plot for F H H transition state]]&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718585</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718585"/>
		<updated>2018-05-17T12:46:43Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* EXERCISE 2: F - H - H system */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.907 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept approximately at equilibrium, a stable transition state has been found at r(H-H) of 0.745 Å and r(F-H) of 1.8115 Å, and its total energy is -103.752 kcal/mol. Figure 4 indicates the stability of these coordinates.}}&lt;br /&gt;
[[File:RCR16_10.png|thumb|Figure 4: Internuclear distance vs time plot for F H H transition state]]&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_10.png&amp;diff=718554</id>
		<title>File:RCR16 10.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_10.png&amp;diff=718554"/>
		<updated>2018-05-17T12:43:19Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718521</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718521"/>
		<updated>2018-05-17T12:37:57Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.907 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|center|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at r(H-H) of 0.74 Å and r(F-H) of 1.81355 Å, and its total energy is -103.743 kcal/mol.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718512</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718512"/>
		<updated>2018-05-17T12:35:58Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* EXERCISE 1: H + H2 system */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.907 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2.png|thumb|center|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|left|Figure 2: MEP contour plot]][[File:RCR16_4.png|thumb|right|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at r(H-H) of 0.74 Å and r(F-H) of 1.81355 Å, and its total energy is -103.743 kcal/mol.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718491</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718491"/>
		<updated>2018-05-17T12:32:36Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* Reactive and unreactive trajectories */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.907 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2.png|thumb|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|Figure 2: MEP contour plot]]&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_4.png|thumb|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Plot !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || [[File:RCR16_5.png|thumb]] || Reactive - initial trajectory is linear so molecule doesn&#039;t oscillate before collision.   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || [[File:RCR16_6.png|thumb]] || Unreactive - system does not have sufficient energy to reach the activation barrier and oscillates back.&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || [[File:RCR16_7.png|thumb]] || Reactive - oscillating initial trajectory proves the H-H bond starts deforming before the attack of the other atom.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || [[File:RCR16_8.png|thumb]] || Unreactive - the 3 atom complex oscillates around the transition state and crosses the barrier but ultimately turns back to reactants.&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || [[File:RCR16_9.png|thumb]] || Reactive - the small additional momentum gives the complex enough energy now to cross to products.&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory has 3 main assumptions stated slightly differently in different sources: &lt;br /&gt;
1. The transition state is in quasi-equilibrium with the reactants but not the products. &lt;br /&gt;
2. The particles involved follow Boltzmann&#039;s distribution and obey classical mechanics.&lt;br /&gt;
3. Once the reactants reach the minimum energy saddle point, the transition state does not collapse back to reactants.&lt;br /&gt;
The simulations that have been made prove that barrier recrossing is possible: the activated complex would have enough energy to turn into products, but not all collisions with good energy will result in a successful reaction since the transition state is not in equilibrium with the reactants. Tunneling in low activation barrier systems is not accounted for either in the transition state theory, but it is difficult to predict its influence on the simulations made. Considering these factors, experimental rates should be usually slower than the ones predicted by theory. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at r(H-H) of 0.74 Å and r(F-H) of 1.81355 Å, and its total energy is -103.743 kcal/mol.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_9.png&amp;diff=718425</id>
		<title>File:RCR16 9.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_9.png&amp;diff=718425"/>
		<updated>2018-05-17T12:10:44Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_8.png&amp;diff=718424</id>
		<title>File:RCR16 8.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_8.png&amp;diff=718424"/>
		<updated>2018-05-17T12:10:21Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: Rcr16 uploaded a new version of File:RCR16 8.png&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_8.png&amp;diff=718420</id>
		<title>File:RCR16 8.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_8.png&amp;diff=718420"/>
		<updated>2018-05-17T12:09:45Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_7.png&amp;diff=718418</id>
		<title>File:RCR16 7.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_7.png&amp;diff=718418"/>
		<updated>2018-05-17T12:09:23Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_6.png&amp;diff=718417</id>
		<title>File:RCR16 6.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_6.png&amp;diff=718417"/>
		<updated>2018-05-17T12:08:37Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_5.png&amp;diff=718416</id>
		<title>File:RCR16 5.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_5.png&amp;diff=718416"/>
		<updated>2018-05-17T12:08:02Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718387</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718387"/>
		<updated>2018-05-17T11:54:42Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* EXERCISE 1: H + H2 system */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.907 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2.png|thumb|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|Figure 2: MEP contour plot]]&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_4.png|thumb|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || Reactive   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || Reactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || Reactive&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory assumes that the rates of reactions can be studied by analyzing the transition state at the saddle point of the potential energy surface for the particular reaction. The transition state is in quasi-equilibrium with the reagents and it can convert into products at a determinable rate using kinetic theory. This theory works well in this simple example as long as the reaction has 1 step, the temperature is not too high and the atoms approximately behave in a classical manner. The simulations that have been carried out ran quite smoothly and it should be assumed that the obtained results will be similar to experimental values, although a systematical error due to the factors that have not been taken into consideration will exist. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at r(H-H) of 0.74 Å and r(F-H) of 1.81355 Å, and its total energy is -103.743 kcal/mol.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718370</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718370"/>
		<updated>2018-05-17T11:52:01Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.907 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in Figure 1.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2.png|thumb|Figure 1:Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in Figure 2 and 3 below.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|Figure 2: MEP contour plot]]&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_4.png|thumb|Figure 3: Dynamics contour plot]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || Reactive   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || Reactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || Reactive&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory assumes that the rates of reactions can be studied by analyzing the transition state at the saddle point of the potential energy surface for the particular reaction. The transition state is in quasi-equilibrium with the reagents and it can convert into products at a determinable rate using kinetic theory. This theory works well in this simple example as long as the reaction has 1 step, the temperature is not too high and the atoms approximately behave in a classical manner. The simulations that have been carried out ran quite smoothly and it should be assumed that the obtained results will be similar to experimental values, although a systematical error due to the factors that have not been taken into consideration will exist. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at r(H-H) of 0.74 Å and r(F-H) of 1.81355 Å, and its total energy is -103.743 kcal/mol.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718366</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718366"/>
		<updated>2018-05-17T11:50:51Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.907 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in the graph.}}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_2.png|thumb|Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in the 2 contour plot below }}&lt;br /&gt;
&lt;br /&gt;
[[File:RCR16_3.png|thumb|MEP plot]]&lt;br /&gt;
&lt;br /&gt;
 [[File:RCR16_4.png|thumb|Dynamics plot]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || Reactive   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || Reactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || Reactive&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory assumes that the rates of reactions can be studied by analyzing the transition state at the saddle point of the potential energy surface for the particular reaction. The transition state is in quasi-equilibrium with the reagents and it can convert into products at a determinable rate using kinetic theory. This theory works well in this simple example as long as the reaction has 1 step, the temperature is not too high and the atoms approximately behave in a classical manner. The simulations that have been carried out ran quite smoothly and it should be assumed that the obtained results will be similar to experimental values, although a systematical error due to the factors that have not been taken into consideration will exist. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at r(H-H) of 0.74 Å and r(F-H) of 1.81355 Å, and its total energy is -103.743 kcal/mol.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718364</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718364"/>
		<updated>2018-05-17T11:49:45Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.907 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in the graph.}}&lt;br /&gt;
[[File:RCR16_2.png|thumb|Internuclear distance vs time plot for transition state]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in the 2 contour plot below }}&lt;br /&gt;
[[File:RCR16_3.png|thumb|MEP plot]] [[File:RCR16_4.png|thumb|Dynamics plot]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || Reactive   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || Reactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || Reactive&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory assumes that the rates of reactions can be studied by analyzing the transition state at the saddle point of the potential energy surface for the particular reaction. The transition state is in quasi-equilibrium with the reagents and it can convert into products at a determinable rate using kinetic theory. This theory works well in this simple example as long as the reaction has 1 step, the temperature is not too high and the atoms approximately behave in a classical manner. The simulations that have been carried out ran quite smoothly and it should be assumed that the obtained results will be similar to experimental values, although a systematical error due to the factors that have not been taken into consideration will exist. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at r(H-H) of 0.74 Å and r(F-H) of 1.81355 Å, and its total energy is -103.743 kcal/mol.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718363</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718363"/>
		<updated>2018-05-17T11:49:05Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: /* Trajectories from r1 = rts+δ, r2 = rts */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.907 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in the graph.}}&lt;br /&gt;
[[File:RCR16_2.png]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. This can be seen in the 2 contour plot below }}&lt;br /&gt;
[[File:RCR16_3.png|thumb|MEP plot]] [[File:RCR16_4.png|thumb|Dynamics plot]]&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || Reactive   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || Reactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || Reactive&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory assumes that the rates of reactions can be studied by analyzing the transition state at the saddle point of the potential energy surface for the particular reaction. The transition state is in quasi-equilibrium with the reagents and it can convert into products at a determinable rate using kinetic theory. This theory works well in this simple example as long as the reaction has 1 step, the temperature is not too high and the atoms approximately behave in a classical manner. The simulations that have been carried out ran quite smoothly and it should be assumed that the obtained results will be similar to experimental values, although a systematical error due to the factors that have not been taken into consideration will exist. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at r(H-H) of 0.74 Å and r(F-H) of 1.81355 Å, and its total energy is -103.743 kcal/mol.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_4.png&amp;diff=718344</id>
		<title>File:RCR16 4.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_4.png&amp;diff=718344"/>
		<updated>2018-05-17T11:45:57Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_3.png&amp;diff=718340</id>
		<title>File:RCR16 3.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_3.png&amp;diff=718340"/>
		<updated>2018-05-17T11:45:16Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718335</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=718335"/>
		<updated>2018-05-17T11:44:39Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.907 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a very slight oscillation, as can be seen in the graph.}}&lt;br /&gt;
[[File:RCR16_2.png]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. }}&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || Reactive   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || Reactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || Reactive&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory assumes that the rates of reactions can be studied by analyzing the transition state at the saddle point of the potential energy surface for the particular reaction. The transition state is in quasi-equilibrium with the reagents and it can convert into products at a determinable rate using kinetic theory. This theory works well in this simple example as long as the reaction has 1 step, the temperature is not too high and the atoms approximately behave in a classical manner. The simulations that have been carried out ran quite smoothly and it should be assumed that the obtained results will be similar to experimental values, although a systematical error due to the factors that have not been taken into consideration will exist. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at r(H-H) of 0.74 Å and r(F-H) of 1.81355 Å, and its total energy is -103.743 kcal/mol.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_2.png&amp;diff=718295</id>
		<title>File:RCR16 2.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:RCR16_2.png&amp;diff=718295"/>
		<updated>2018-05-17T11:35:10Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=715514</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=715514"/>
		<updated>2018-05-15T14:40:07Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.95 Å for both A-B and B-C distances. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a uniform oscillation, as can be seen in the graph.}}&lt;br /&gt;
[[File:Rcr16_q1.png]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. }}&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy(kcal/mol) !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || Reactive   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || Reactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || Reactive&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory assumes that the rates of reactions can be studied by analyzing the transition state at the saddle point of the potential energy surface for the particular reaction. The transition state is in quasi-equilibrium with the reagents and it can convert into products at a determinable rate using kinetic theory. This theory works well in this simple example as long as the reaction has 1 step, the temperature is not too high and the atoms approximately behave in a classical manner. The simulations that have been carried out ran quite smoothly and it should be assumed that the obtained results will be similar to experimental values, although a systematical error due to the factors that have not been taken into consideration will exist. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at r(H-H) of 0.74 Å and r(F-H) of 1.81355 Å, and its total energy is -103.743 kcal/mol.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=715450</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=715450"/>
		<updated>2018-05-15T14:34:20Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.95 distance units. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a uniform oscillation, as can be seen in the graph.}}&lt;br /&gt;
[[File:Rcr16_q1.png]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. }}&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || Reactive   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || Reactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || Reactive&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory assumes that the rates of reactions can be studied by analyzing the transition state at the saddle point of the potential energy surface for the particular reaction. The transition state is in quasi-equilibrium with the reagents and it can convert into products at a determinable rate using kinetic theory. This theory works well in this simple example as long as the reaction has 1 step, the temperature is not too high and the atoms approximately behave in a classical manner. The simulations that have been carried out ran quite smoothly and it should be assumed that the obtained results will be similar to experimental values, although a systematical error due to the factors that have not been taken into consideration will exist. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at}} r=0.74 and r(F-H)=1.81355, and its total energy is -103.743 units.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=715431</id>
		<title>MRD:RCR16</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:RCR16&amp;diff=715431"/>
		<updated>2018-05-15T14:33:17Z</updated>

		<summary type="html">&lt;p&gt;Rcr16: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== EXERCISE 1: H + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; system  ==&lt;br /&gt;
&lt;br /&gt;
=== Dynamics from the transition state region ===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The partial derivative of V with respect to r1 and r2 must be 0 at local extremum point. To determine whether this point is a minimum, maximum or a saddle point(transition state), the second partial derivatives test can be used. The second derivative test discriminant D is calculated from the second order derivatives of the potential energy surface with respect to r1, r2 and both r1 and r2. If D is higher than 0 and the second order derivative with respect to r1 is higher than 0, the point is a minimum. If D is smaller than 0, then it is a saddle point.}}&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;: locating the transition state ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The transition state distance has been estimated to be around 0.95 distance units. This is easily seen in the internuclear distance vs time plot, where the A-B and B-C distance lines overlap completely and show a uniform oscillation, as can be seen in the graph.}}&lt;br /&gt;
[[File:Rcr16_q1.png]]&lt;br /&gt;
&lt;br /&gt;
==== Trajectories from r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt;+δ, r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; = r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; ====&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|The mep line towards the products is quite straight, whereas the dynamic trajectory has a sinusoidal aspect. The mep line, in other words, shows the potential energy with the oscillation term completely removed while the dynamic trajectory accounts for bond oscillation. }}&lt;br /&gt;
&lt;br /&gt;
==== Reactive and unreactive trajectories ====&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt; !! p&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; !! Total Energy !! Reactive/Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5 || -99.018 || Reactive   &lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0 || -100.456 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5 || -98.956 || Reactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0 || -84.956 || Unreactive&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2 || -83.416 || Reactive&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor|blue|Transition state theory assumes that the rates of reactions can be studied by analyzing the transition state at the saddle point of the potential energy surface for the particular reaction. The transition state is in quasi-equilibrium with the reagents and it can convert into products at a determinable rate using kinetic theory. This theory works well in this simple example as long as the reaction has 1 step, the temperature is not too high and the atoms approximately behave in a classical manner. The simulations that have been carried out ran quite smoothly and it should be assumed that the obtained results will be similar to experimental values, although a systematical error due to the factors that have not been taken into consideration will exist. }}&lt;br /&gt;
&lt;br /&gt;
== EXERCISE 2: F - H - H system ==&lt;br /&gt;
&lt;br /&gt;
===PES inspection===&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue| The F + H&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt; reaction is exothermic while the H + HF reaction is endothermic, since the H-F bond dissociation energy(565 kJ/mol) is higher compared to the H-H one(432 kJ/mol), meaning that HF has a stronger bond and is more stable.  }}&lt;br /&gt;
&lt;br /&gt;
{{fontcolor1|blue|  Following Hammond&#039;s postulate,  the transition state will be closer in structure to the F+ H-H system rather than F-H + H system since it is higher in energy. Thus, by testing different F-H distances while the H-H distance is kept at equilibrium, a stable transition state has been found at r(HH)=0.74 }} and r(FH)=1.81355, and its total energy is -103.743 units.}}&lt;/div&gt;</summary>
		<author><name>Rcr16</name></author>
	</entry>
</feed>