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		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=732266</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=732266"/>
		<updated>2018-05-25T14:47:25Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* F-H-H System */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). While the simulations in this case allow for any arbitrary initial positions and translational / vibrational momenta to be set, such experiments can be actually done (to some extent, of course) by manipulating the atoms with ultrafast lasers &amp;lt;ref&amp;gt;Gruebele M., Zewail A. H. Physics Today. May 1990, pp. 24-33.&amp;lt;/ref&amp;gt;. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores external factors (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
A more accurate and faster way to find the TS would be by simply computing the determinants of the Hessians throughout the PES. However, after a quick inspection of the LepsPy source code, the modification of the code appeared to be more time consuming than finding it by hand, given the fact only two TS needed to be determined in this work. Nevertheless, it would be a useful feature. &lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the speed of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length (0.74) and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) produces similar results as the transition state dissociates into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows the process down significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process (an integral of the 1/r potential), in the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=&amp;quot;220px&amp;quot; widths=&amp;quot;250px&amp;quot;&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | The path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | The path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and unreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as defined in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple times and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The Transition State Theory (TST) is used to explain the kinetics of elementary reactions and to determine the thermodynamic parameters of activation. This theory works with an assumed quasi-equilibrium between the reactants and the activated complex in the transition state corresponding to a saddle point &amp;lt;ref&amp;gt;Wikipedia: Transition State Theory. Accessed on 24/05/2018. Available online at https://en.wikipedia.org/wiki/Transition_state_theory&amp;lt;/ref&amp;gt;. Then, kinetic theory can be used to determine the reaction rate. It also assumes that the nuclei behave according to classical mechanics and the transition state collapses directly into the products (no barrier recrossing). Therefore, due to the last assumption the real reaction rates would be lower than predicted by the TST. It also deviates at higher temperature due to higher vibrational states not passing the saddle point and possibly due to quantum-mechanical effects like tunneling.&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Exchanging one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Making a reference to Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others (neglected in this simulation) &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and unreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-crosses the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png|350x350px]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png|frameless|350x350px]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
The energy for the activation can be supplied as both vibrational and translational momenta. Polanyi&#039;s rules state&amp;lt;ref&amp;gt;Steinfeld I.J., Francisco J. S., Hase, W. L. Chemical Kinetic and Dynamics. Prentice-Hall (1998).&amp;lt;/ref&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For an early barrier (forward reaction in this case) the most effective passage is with translational rather than vibrational energy. Conversely, for a late barrier (the reverse reaction), it&#039;s easier passed with vibrational rather than translational energy.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
From the results of the forward reaction, it appears that the vibrational energy had a significant effect on enhancing the forward reaction, while a high translational energy has helped with the reverse reaction - exactly the opposite as Polanyi&#039;s rules state. The results here are inconclusive and more calculations would be useful - the few calculations ran in this report might not provide a representative data set. In all cases the success of the reaction was sensitive to the initial energy values in a more complex way than simply &#039;high enough&#039; - in the high energy cases barrier recrossing has often occured.&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=732220</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=732220"/>
		<updated>2018-05-25T14:41:04Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Introduction */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). While the simulations in this case allow for any arbitrary initial positions and translational / vibrational momenta to be set, such experiments can be actually done (to some extent, of course) by manipulating the atoms with ultrafast lasers &amp;lt;ref&amp;gt;Gruebele M., Zewail A. H. Physics Today. May 1990, pp. 24-33.&amp;lt;/ref&amp;gt;. &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores external factors (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
A more accurate and faster way to find the TS would be by simply computing the determinants of the Hessians throughout the PES. However, after a quick inspection of the LepsPy source code, the modification of the code appeared to be more time consuming than finding it by hand, given the fact only two TS needed to be determined in this work. Nevertheless, it would be a useful feature. &lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the speed of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length (0.74) and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) produces similar results as the transition state dissociates into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows the process down significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process (an integral of the 1/r potential), in the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=&amp;quot;220px&amp;quot; widths=&amp;quot;250px&amp;quot;&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | The path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | The path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and unreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as defined in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple times and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The Transition State Theory (TST) is used to explain the kinetics of elementary reactions and to determine the thermodynamic parameters of activation. This theory works with an assumed quasi-equilibrium between the reactants and the activated complex in the transition state corresponding to a saddle point &amp;lt;ref&amp;gt;Wikipedia: Transition State Theory. Accessed on 24/05/2018. Available online at https://en.wikipedia.org/wiki/Transition_state_theory&amp;lt;/ref&amp;gt;. Then, kinetic theory can be used to determine the reaction rate. It also assumes that the nuclei behave according to classical mechanics and the transition state collapses directly into the products (no barrier recrossing). Therefore, due to the last assumption the real reaction rates would be lower than predicted by the TST. It also deviates at higher temperature due to higher vibrational states not passing the saddle point and possibly due to quantum-mechanical effects like tunneling.&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Exchanging one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Making a reference to Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others (neglected in this simulation) &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and unreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-crosses the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
The energy for the activation can be supplied as both vibrational and translational momenta. Polanyi&#039;s rules state&amp;lt;ref&amp;gt;Steinfeld I.J., Francisco J. S., Hase, W. L. Chemical Kinetic and Dynamics. Prentice-Hall (1998).&amp;lt;/ref&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For an early barrier (forward reaction in this case) the most effective passage is with translational rather than vibrational energy. Conversely, for a late barrier (the reverse reaction), it&#039;s easier passed with vibrational rather than translational energy.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
From the results of the forward reaction, it appears that the vibrational energy had a significant effect on enhancing the forward reaction, while a high translational energy has helped with the reverse reaction - exactly the opposite as Polanyi&#039;s rules state. The results here are inconclusive and more calculations would be useful - the few calculations ran in this report might not provide a representative data set. In all cases the success of the reaction was sensitive to the initial energy values in a more complex way than simply &#039;high enough&#039; - in the high energy cases barrier recrossing has often occured.&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730644</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730644"/>
		<updated>2018-05-24T20:43:37Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Reverse reaction analysis */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores external factors (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
A more accurate and faster way to find the TS would be by simply computing the determinants of the Hessians throughout the PES. However, after a quick inspection of the LepsPy source code, the modification of the code appeared to be more time consuming than finding it by hand, given the fact only two TS needed to be determined in this work. Nevertheless, it would be a useful feature. &lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the speed of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length (0.74) and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) produces similar results as the transition state dissociates into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows the process down significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process (an integral of the 1/r potential), in the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=&amp;quot;220px&amp;quot; widths=&amp;quot;250px&amp;quot;&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | The path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | The path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and unreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as defined in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple times and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The Transition State Theory (TST) is used to explain the kinetics of elementary reactions and to determine the thermodynamic parameters of activation. This theory works with an assumed quasi-equilibrium between the reactants and the activated complex in the transition state corresponding to a saddle point &amp;lt;ref&amp;gt;Wikipedia: Transition State Theory. Accessed on 24/05/2018. Available online at https://en.wikipedia.org/wiki/Transition_state_theory&amp;lt;/ref&amp;gt;. Then, kinetic theory can be used to determine the reaction rate. It also assumes that the nuclei behave according to classical mechanics and the transition state collapses directly into the products (no barrier recrossing). Therefore, due to the last assumption the real reaction rates would be lower than predicted by the TST. It also deviates at higher temperature due to higher vibrational states not passing the saddle point and possibly due to quantum-mechanical effects like tunneling.&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Exchanging one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Making a reference to Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others (neglected in this simulation) &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and unreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-crosses the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
The energy for the activation can be supplied as both vibrational and translational momenta. Polanyi&#039;s rules state&amp;lt;ref&amp;gt;Steinfeld I.J., Francisco J. S., Hase, W. L. Chemical Kinetic and Dynamics. Prentice-Hall (1998).&amp;lt;/ref&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;For an early barrier (forward reaction in this case) the most effective passage is with translational rather than vibrational energy. Conversely, for a late barrier (the reverse reaction), it&#039;s easier passed with vibrational rather than translational energy.&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
From the results of the forward reaction, it appears that the vibrational energy had a significant effect on enhancing the forward reaction, while a high translational energy has helped with the reverse reaction - exactly the opposite as Polanyi&#039;s rules state. The results here are inconclusive and more calculations would be useful - the few calculations ran in this report might not provide a representative data set. In all cases the success of the reaction was sensitive to the initial energy values in a more complex way than simply &#039;high enough&#039; - in the high energy cases barrier recrossing has often occured.&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730575</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730575"/>
		<updated>2018-05-24T20:15:32Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Reverse reaction analysis */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores external factors (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
A more accurate and faster way to find the TS would be by simply computing the determinants of the Hessians throughout the PES. However, after a quick inspection of the LepsPy source code, the modification of the code appeared to be more time consuming than finding it by hand, given the fact only two TS needed to be determined in this work. Nevertheless, it would be a useful feature. &lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the speed of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length (0.74) and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) produces similar results as the transition state dissociates into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows the process down significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process (an integral of the 1/r potential), in the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=&amp;quot;220px&amp;quot; widths=&amp;quot;250px&amp;quot;&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | The path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | The path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and unreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as defined in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple times and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The Transition State Theory (TST) is used to explain the kinetics of elementary reactions and to determine the thermodynamic parameters of activation. This theory works with an assumed quasi-equilibrium between the reactants and the activated complex in the transition state corresponding to a saddle point &amp;lt;ref&amp;gt;Wikipedia: Transition State Theory. Accessed on 24/05/2018. Available online at https://en.wikipedia.org/wiki/Transition_state_theory&amp;lt;/ref&amp;gt;. Then, kinetic theory can be used to determine the reaction rate. It also assumes that the nuclei behave according to classical mechanics and the transition state collapses directly into the products (no barrier recrossing). Therefore, due to the last assumption the real reaction rates would be lower than predicted by the TST. It also deviates at higher temperature due to higher vibrational states not passing the saddle point and possibly due to quantum-mechanical effects like tunneling.&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Exchanging one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Making a reference to Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others (neglected in this simulation) &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and unreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-crosses the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations are in an agreement with Polanyi&#039;s rules &amp;lt;ref&amp;gt;Steinfeld I.J., Francisco J. S., Hase, W. L. Chemical Kinetic and Dynamics. Prentice-Hall (1998).&amp;lt;/ref&amp;gt;:&lt;br /&gt;
For an early barrier (forward reaction in this case) the most effective passage is with translational rather than vibrational energy. Conversely, for a late barrier (the reverse reaction), it&#039;s easier passed with vibrational rather than translational energy.&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730562</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730562"/>
		<updated>2018-05-24T20:06:15Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Reaction dynamics */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores external factors (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
A more accurate and faster way to find the TS would be by simply computing the determinants of the Hessians throughout the PES. However, after a quick inspection of the LepsPy source code, the modification of the code appeared to be more time consuming than finding it by hand, given the fact only two TS needed to be determined in this work. Nevertheless, it would be a useful feature. &lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the speed of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length (0.74) and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) produces similar results as the transition state dissociates into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows the process down significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process (an integral of the 1/r potential), in the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=&amp;quot;220px&amp;quot; widths=&amp;quot;250px&amp;quot;&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | The path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | The path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and unreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as defined in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple times and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The Transition State Theory (TST) is used to explain the kinetics of elementary reactions and to determine the thermodynamic parameters of activation. This theory works with an assumed quasi-equilibrium between the reactants and the activated complex in the transition state corresponding to a saddle point &amp;lt;ref&amp;gt;Wikipedia: Transition State Theory. Accessed on 24/05/2018. Available online at https://en.wikipedia.org/wiki/Transition_state_theory&amp;lt;/ref&amp;gt;. Then, kinetic theory can be used to determine the reaction rate. It also assumes that the nuclei behave according to classical mechanics and the transition state collapses directly into the products (no barrier recrossing). Therefore, due to the last assumption the real reaction rates would be lower than predicted by the TST. It also deviates at higher temperature due to higher vibrational states not passing the saddle point and possibly due to quantum-mechanical effects like tunneling.&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Exchanging one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Making a reference to Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others (neglected in this simulation) &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and unreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-crosses the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730561</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730561"/>
		<updated>2018-05-24T20:05:40Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Forward Reaction Reactive and unreactive pathways */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores external factors (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
A more accurate and faster way to find the TS would be by simply computing the determinants of the Hessians throughout the PES. However, after a quick inspection of the LepsPy source code, the modification of the code appeared to be more time consuming than finding it by hand, given the fact only two TS needed to be determined in this work. Nevertheless, it would be a useful feature. &lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the speed of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length (0.74) and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) produces similar results as the transition state dissociates into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows the process down significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process (an integral of the 1/r potential), in the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=&amp;quot;220px&amp;quot; widths=&amp;quot;250px&amp;quot;&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | The path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | The path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and unreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as defined in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple times and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The Transition State Theory (TST) is used to explain the kinetics of elementary reactions and to determine the thermodynamic parameters of activation. This theory works with an assumed quasi-equilibrium between the reactants and the activated complex in the transition state corresponding to a saddle point &amp;lt;ref&amp;gt;Wikipedia: Transition State Theory. Accessed on 24/05/2018. Available online at https://en.wikipedia.org/wiki/Transition_state_theory&amp;lt;/ref&amp;gt;. Then, kinetic theory can be used to determine the reaction rate. It also assumes that the nuclei behave according to classical mechanics and the transition state collapses directly into the products (no barrier recrossing). Therefore, due to the last assumption the real reaction rates would be lower than predicted by the TST. It also deviates at higher temperature due to higher vibrational states not passing the saddle point and possibly due to quantum-mechanical effects like tunneling.&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Exchanging one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Making a reference to Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others (neglected in this simulation) &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and unreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-crosses the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730558</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730558"/>
		<updated>2018-05-24T20:03:30Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Forward Reaction Reactive and unreactive pathways */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores external factors (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
A more accurate and faster way to find the TS would be by simply computing the determinants of the Hessians throughout the PES. However, after a quick inspection of the LepsPy source code, the modification of the code appeared to be more time consuming than finding it by hand, given the fact only two TS needed to be determined in this work. Nevertheless, it would be a useful feature. &lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the speed of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length (0.74) and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) produces similar results as the transition state dissociates into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows the process down significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process (an integral of the 1/r potential), in the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=&amp;quot;220px&amp;quot; widths=&amp;quot;250px&amp;quot;&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | The path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | The path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and unreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as defined in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple times and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The Transition State Theory (TST) is used to explain the kinetics of elementary reactions and to determine the thermodynamic parameters of activation. This theory works with an assumed quasi-equilibrium between the reactants and the activated complex in the transition state corresponding to a saddle point &amp;lt;ref&amp;gt;Wikipedia: Transition State Theory. Accessed on 24/05/2018. Available online at https://en.wikipedia.org/wiki/Transition_state_theory&amp;lt;/ref&amp;gt;. Then, kinetic theory can be used to determine the reaction rate. It also assumes that the nuclei behave according to classical mechanics and the transition state collapses directly into the products (no barrier recrossing). Therefore, due to the last assumption the real reaction rates would be lower than predicted by the TST. It also deviates at higher temperature due to higher vibrational states not passing the saddle point and possibly due to quantum-mechanical effects like tunneling.&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Exchanging one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Making a reference to Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others (neglected in this simulation) &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and unreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730556</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730556"/>
		<updated>2018-05-24T20:01:31Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* F-H-H System */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores external factors (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
A more accurate and faster way to find the TS would be by simply computing the determinants of the Hessians throughout the PES. However, after a quick inspection of the LepsPy source code, the modification of the code appeared to be more time consuming than finding it by hand, given the fact only two TS needed to be determined in this work. Nevertheless, it would be a useful feature. &lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the speed of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length (0.74) and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) produces similar results as the transition state dissociates into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows the process down significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process (an integral of the 1/r potential), in the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=&amp;quot;220px&amp;quot; widths=&amp;quot;250px&amp;quot;&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | The path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | The path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and unreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as defined in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple times and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The Transition State Theory (TST) is used to explain the kinetics of elementary reactions and to determine the thermodynamic parameters of activation. This theory works with an assumed quasi-equilibrium between the reactants and the activated complex in the transition state corresponding to a saddle point &amp;lt;ref&amp;gt;Wikipedia: Transition State Theory. Accessed on 24/05/2018. Available online at https://en.wikipedia.org/wiki/Transition_state_theory&amp;lt;/ref&amp;gt;. Then, kinetic theory can be used to determine the reaction rate. It also assumes that the nuclei behave according to classical mechanics and the transition state collapses directly into the products (no barrier recrossing). Therefore, due to the last assumption the real reaction rates would be lower than predicted by the TST. It also deviates at higher temperature due to higher vibrational states not passing the saddle point and possibly due to quantum-mechanical effects like tunneling.&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Exchanging one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Making a reference to Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others (neglected in this simulation) &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and unreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730555</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730555"/>
		<updated>2018-05-24T19:58:04Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* H-H-H system */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores external factors (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
A more accurate and faster way to find the TS would be by simply computing the determinants of the Hessians throughout the PES. However, after a quick inspection of the LepsPy source code, the modification of the code appeared to be more time consuming than finding it by hand, given the fact only two TS needed to be determined in this work. Nevertheless, it would be a useful feature. &lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the speed of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length (0.74) and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) produces similar results as the transition state dissociates into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows the process down significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process (an integral of the 1/r potential), in the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=&amp;quot;220px&amp;quot; widths=&amp;quot;250px&amp;quot;&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | The path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | The path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and unreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as defined in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple times and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
The Transition State Theory (TST) is used to explain the kinetics of elementary reactions and to determine the thermodynamic parameters of activation. This theory works with an assumed quasi-equilibrium between the reactants and the activated complex in the transition state corresponding to a saddle point &amp;lt;ref&amp;gt;Wikipedia: Transition State Theory. Accessed on 24/05/2018. Available online at https://en.wikipedia.org/wiki/Transition_state_theory&amp;lt;/ref&amp;gt;. Then, kinetic theory can be used to determine the reaction rate. It also assumes that the nuclei behave according to classical mechanics and the transition state collapses directly into the products (no barrier recrossing). Therefore, due to the last assumption the real reaction rates would be lower than predicted by the TST. It also deviates at higher temperature due to higher vibrational states not passing the saddle point and possibly due to quantum-mechanical effects like tunneling.&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Exchanging one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730518</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730518"/>
		<updated>2018-05-24T19:40:09Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* H-H-H system */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores external factors (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
A more accurate and faster way to find the TS would be by simply computing the determinants of the Hessians throughout the PES. However, after a quick inspection of the LepsPy source code, the modification of the code appeared to be more time consuming than finding it by hand, given the fact only two TS needed to be determined in this work. Nevertheless, it would be a useful feature. &lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the speed of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730461</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730461"/>
		<updated>2018-05-24T19:07:20Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Introduction */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730458</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730458"/>
		<updated>2018-05-24T19:06:50Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Introduction */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative, the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730456</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730456"/>
		<updated>2018-05-24T19:05:58Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Introduction */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;\bold H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=  \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2} -\left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If the determinant is negative, the point is a saddle point. If the determinant is positive and &amp;lt;math&amp;gt;\dfrac{\partial^2 V}{\partial x^2}&amp;lt;/math&amp;gt; is also positive, then the point is a local minimum.&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730449</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730449"/>
		<updated>2018-05-24T19:01:30Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Introduction */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;\bold H(x,y) = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Then, the determinant of the Hessian has to be calculated&lt;br /&gt;
:&amp;lt;math&amp;gt;D(x,y)=\det(H(x,y)) = \dfrac{\partial^2 V}{\partial x^2}\dfrac{\partial^2 V}{\partial y^2) - \left( \dfrac{\partial^2 V}{\partial x\,\partial y} \right)^2 &amp;lt;/math&amp;gt;,&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
If both eigenvalues are positive the point is a maximum, if both are negative the point is a minimum and if one is positive and one negative the point is a saddle point (and corresponds to the transition state).&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated using the LepsPy software, developed by T. Mackenzie and published under the GPL License. In all cases, a 180-degree collision trajectory was assumed.&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730353</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730353"/>
		<updated>2018-05-24T18:27:13Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Introduction */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To distinguish between these three cases, the second derivatives have to be calculated &amp;lt;ref&amp;gt;Quirke, N. Maths 2 Lecture Notes. Imperial College (2017).&amp;lt;/ref&amp;gt;, providing a Hessian matrix.&lt;br /&gt;
:&amp;lt;math&amp;gt;\bold H = \begin{bmatrix}&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial x^2} &amp;amp; \dfrac{\partial^2 V}{\partial x\,\partial y} \\[2.2ex]&lt;br /&gt;
  \dfrac{\partial^2 V}{\partial y\,\partial x} &amp;amp; \dfrac{\partial^2 V}{\partial y^2} \\[2.2ex]&lt;br /&gt;
\end{bmatrix}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730341</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=730341"/>
		<updated>2018-05-24T18:21:13Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Introduction */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
Simulating reactions as paths on a potential energy surface (PES) can provide interesting insights into the elementary reaction rates and mechanisms. From the minima it is possible to calculate the energy difference between the reactants and the products and by finding the saddle point of the PES it is possible to both determine the activation energies and the structure of the transition state (TS). The minima, maxima and saddle point all satisfy the requirement for zero gradient of the PES:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla V(x,y) = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The collisions between three atoms were simulated&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728420</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728420"/>
		<updated>2018-05-24T12:47:15Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Reverse reaction analysis */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==References==&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728418</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728418"/>
		<updated>2018-05-24T12:46:49Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Reaction dynamics */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during the reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. Also, the excess vibrational energy can be emitted in the form of IR photons, as observed by Polanyi and others &amp;lt;ref&amp;gt;J. C. Polanyi, Science 236, 680 (1987).&amp;lt;/ref&amp;gt;. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the contour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728334</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728334"/>
		<updated>2018-05-24T12:22:00Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* F-H-H System */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.811&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the countour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728332</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728332"/>
		<updated>2018-05-24T12:21:23Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Energy considerations */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.919&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.745&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the countour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728294</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728294"/>
		<updated>2018-05-24T12:10:42Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Reverse reaction analysis */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the countour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -10&#039;&#039; produced a reactive pathway as shown in the Figure below.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-016-revreact.png]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
Starting from the transition state determined earlier (with a small deviation due to rounding errors), after 2500 steps the final parameters were found to be &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.89736&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 9.97011&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -5.16018&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.06519&#039;. When these values were fed into the software (inverting the momenta), the reactants did not even reach the transition state, even when the inputs were matched to 6 significant figures with the final position from the TS simulation.&lt;br /&gt;
&lt;br /&gt;
These observations outline two requirements:&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Forward reaction:&#039;&#039;&#039; &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Reverse reaction:&#039;&#039;&#039; High collision momentum (translational) energy required with the vibrational energy being relatively unimportant. It was observed that it was very hard to set up the conditions for the reaction to happen with a high vibrational energy but low translational, but very easy the other way round.&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
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		<updated>2018-05-24T12:00:25Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
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		<updated>2018-05-24T10:41:20Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
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	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728075</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728075"/>
		<updated>2018-05-24T10:39:42Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Forward Reaction Reactive and uncreactive pathways */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the countour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;br /&gt;
&lt;br /&gt;
=== Reverse reaction analysis ===&lt;br /&gt;
&lt;br /&gt;
Running with the following initial values: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.91&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;.&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728066</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=728066"/>
		<updated>2018-05-24T10:33:43Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Forward Reaction Reactive and uncreactive pathways */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction. The sign of the HH-momentum affects if the first vibration goes &#039;together&#039; or &#039;away&#039; and on the countour plots are visible as &#039;down&#039; and &#039;up&#039; vibrations, respectively. As it can be seen from the data below, this initial setting can affect the outcome of the reaction. Notice the different vibrational amplitudes for +0.5 and -0.5 setting - this is a result of the anharmonicity of the potential.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || The reaction proceeds. || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
The simulation was also performed with the following parameters: &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039;, &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.5&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.8&#039;&#039;&#039;. Initially, the dihydrogen reactant has a relatively small vibrational energy but the product a much higher - this is due to the energy released in the reaction.&lt;br /&gt;
[[File:Mh-015-react-lowvib.png]]&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-015-react-lowvib.png&amp;diff=728065</id>
		<title>File:Mh-015-react-lowvib.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-015-react-lowvib.png&amp;diff=728065"/>
		<updated>2018-05-24T10:33:33Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727947</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727947"/>
		<updated>2018-05-23T20:32:43Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Reaction dynamics */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
====Forward Reaction Reactive and uncreactive pathways====&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial parameters of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt;&#039;&#039;&#039;, &#039;&#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.74&#039;&#039;&#039; and &#039;&#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -0.5&#039;&#039;&#039; and a variable initial momentum were used to investigate the reactive pathways for this reaction.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -3 ||  Reaction proceeds, the product has a significant vibrational energy. || yes || [[File:Mh-014-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || Reaction proceeds, but the product has a lower vibrational energy than in the first case || yes || [[File:Mh-014-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2  || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +0.5   || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-014-react-E.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2   || The reaction proceeds, crossing the barrier once. || yes || [[File:Mh-014-react-F.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +2.5   || || yes || [[File:Mh-014-react-G.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| +3   || The products re-cross the barrier and revert to reactants. || no || [[File:Mh-014-react-H.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-B.png&amp;diff=727946</id>
		<title>File:Mh-014-react-B.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-B.png&amp;diff=727946"/>
		<updated>2018-05-23T20:32:36Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
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		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-A.png&amp;diff=727945</id>
		<title>File:Mh-014-react-A.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-A.png&amp;diff=727945"/>
		<updated>2018-05-23T20:32:24Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
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		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-C.png&amp;diff=727944</id>
		<title>File:Mh-014-react-C.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-C.png&amp;diff=727944"/>
		<updated>2018-05-23T20:32:13Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
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		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-D.png&amp;diff=727943</id>
		<title>File:Mh-014-react-D.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-D.png&amp;diff=727943"/>
		<updated>2018-05-23T20:32:00Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
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&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-F.png&amp;diff=727942</id>
		<title>File:Mh-014-react-F.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-F.png&amp;diff=727942"/>
		<updated>2018-05-23T20:31:46Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
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		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-E.png&amp;diff=727941</id>
		<title>File:Mh-014-react-E.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-E.png&amp;diff=727941"/>
		<updated>2018-05-23T20:31:32Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
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		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-G.png&amp;diff=727940</id>
		<title>File:Mh-014-react-G.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-G.png&amp;diff=727940"/>
		<updated>2018-05-23T20:31:20Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
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		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-H.png&amp;diff=727939</id>
		<title>File:Mh-014-react-H.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-014-react-H.png&amp;diff=727939"/>
		<updated>2018-05-23T20:31:09Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
&lt;hr /&gt;
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		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727918</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727918"/>
		<updated>2018-05-23T20:09:44Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Reaction dynamics */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. This relates a microscopic simulation to a macroscopic phenomenon, which can be easily measured using, for example, a calorimeter. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727903</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727903"/>
		<updated>2018-05-23T20:04:16Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Reaction dynamics */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels (potential energy maxima where they have no kinetic energy) before and after the reaction. However, the vibrational energy increased significantly during reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727902</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727902"/>
		<updated>2018-05-23T20:03:02Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* F-H-H System */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels before and after the reaction. However, the vibrational energy increased significantly during reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727901</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727901"/>
		<updated>2018-05-23T20:02:41Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Reaction dynamics */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;&#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels before and after the reaction. However, the vibrational energy increased significantly during reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heigths=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727899</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727899"/>
		<updated>2018-05-23T20:02:08Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Reaction dynamics */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below. Looking at the surface plot below, it is clear that the energy is conserved since the &#039;vibrational peaks&#039; reach the same levels before and after the reaction. However, the vibrational energy increased significantly during reaction, corresponding to the &#039;release of heat&#039; since the reaction is exothermic. The amplitudes of the vibrations (stretches) are especially visible on the Momenta in time plot.&lt;br /&gt;
&amp;lt;gallery widths=250px heigths=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-013-FHH-rxn-surface.png|Reaction potential energy surface&lt;br /&gt;
File:Mh-013-FHH-rxn-momenta.png|Internuclear momenta over the course of the reaction.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727895</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727895"/>
		<updated>2018-05-23T19:57:33Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Energy considerations */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&amp;lt;gallery widths=250px heights=250px&amp;gt;&lt;br /&gt;
[[&lt;br /&gt;
File:Mh-012-HH-bond.png|MEP determination of the H-H bond length.&lt;br /&gt;
File:Mh-012-FH-bond.png|MEP determination of the F-H bond length.&lt;br /&gt;
]]&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below.&lt;br /&gt;
[[File:Mh-013-FHH-rxn-surface.png|thumb|Reaction potential energy surface.|none]]&lt;br /&gt;
[[File:Mh-013-FHH-rxn-momenta.png|thumb|Internuclear moment over the course of the reaction.|none]]&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727894</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727894"/>
		<updated>2018-05-23T19:55:36Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Energy considerations */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}[[File:Mh-012-HH-bond.png|thumb|MEP determination of the H-H bond length.|none]][[File:Mh-012-FH-bond.png|thumb|MEP determination of the F-H bond length.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reaction dynamics===&lt;br /&gt;
&lt;br /&gt;
Simulating the reaction with the following parameters &#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 2.4&#039;&#039;, &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;, &#039;p&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = -1&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = -2&#039;&#039; provides the data and plots below.&lt;br /&gt;
[[File:Mh-013-FHH-rxn-surface.png|thumb|Reaction potential energy surface.|none]]&lt;br /&gt;
[[File:Mh-013-FHH-rxn-momenta.png|thumb|Internuclear moment over the course of the reaction.|none]]&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-013-FHH-rxn-momenta.png&amp;diff=727893</id>
		<title>File:Mh-013-FHH-rxn-momenta.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-013-FHH-rxn-momenta.png&amp;diff=727893"/>
		<updated>2018-05-23T19:54:43Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-013-FHH-rxn-surface.png&amp;diff=727891</id>
		<title>File:Mh-013-FHH-rxn-surface.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-013-FHH-rxn-surface.png&amp;diff=727891"/>
		<updated>2018-05-23T19:53:24Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727815</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727815"/>
		<updated>2018-05-23T18:38:26Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* Energetic consideration */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|The position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energy considerations===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}[[File:Mh-012-HH-bond.png|thumb|MEP determination of the H-H bond length.|none]][[File:Mh-012-FH-bond.png|thumb|MEP determination of the F-H bond length.|none]]Reaction dynamics&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-012-FH-bond.png&amp;diff=727812</id>
		<title>File:Mh-012-FH-bond.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-012-FH-bond.png&amp;diff=727812"/>
		<updated>2018-05-23T18:35:12Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: Mh5015 uploaded a new version of File:Mh-012-FH-bond.png&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-012-HH-bond.png&amp;diff=727811</id>
		<title>File:Mh-012-HH-bond.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-012-HH-bond.png&amp;diff=727811"/>
		<updated>2018-05-23T18:34:53Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727810</id>
		<title>MRD:MH5015</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=MRD:MH5015&amp;diff=727810"/>
		<updated>2018-05-23T18:34:00Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: /* F-H-H System */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;This is a report from the Molecular reaction dynamics computational lab by Martin Holicky.&lt;br /&gt;
&lt;br /&gt;
==Introduction==&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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.&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
SW ANGLE&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==H-H-H system==&lt;br /&gt;
[[File:Mh-001-ts-hhh.png|thumb|Nuclear separation in time when the atoms are in the transition state.]]&lt;br /&gt;
The following reaction between three hydrogen atoms was considered:&lt;br /&gt;
&lt;br /&gt;
H-H + H ⇄ H + H-H&lt;br /&gt;
&lt;br /&gt;
It is clear that since all three atoms are identical the bond lengths are equal and also the potential energy surface symmetrical. As stated in the Introduction, the transition state is located at the maximum of the minimum energy path where the potential energy gradient is zero. This implies an unstable equilibrium, however, since the simulation ignores any external factor (such as other atoms) it will be stable forever. By gradually adjusting the internuclear separations while keeping the momenta at zero the transition state position was found at &#039;&#039;r&amp;lt;sub&amp;gt;ts&amp;lt;/sub&amp;gt; = 0.907&#039;&#039;. The internuclear distance did not change in time which is indeed expected from a transition state. Minor oscillations - stretches of the H-H-H bonds are visible but since these are symmetrical the do not shift shift the equlibrium.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Minimum energy paths===&lt;br /&gt;
[[File:Mh-003-mep_not_ts-hhh.png|thumb|Interatomic distances during the process as simulated in the MEP mode.]]By setting the velocity of the atoms to zero in each step, it is possible to calculate the &#039;&#039;minimum energy path&#039;&#039; (MEP). In this simulation, the H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt; distances were set to 0.917 and 0.907 respectively, the former corresponding to a slight displacement from the transition state. This displacement resulted in the transition state collapsing into H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. The H-H distance &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; simply converged to the dihydrogen bond length and &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; increased steadily (reaching a minimum at infinity). &lt;br /&gt;
&lt;br /&gt;
Running the simulation in the Dynamics mode (preserving velocities between steps) similar results are obtained as the transition state dissociates into  H&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; and H&amp;lt;sub&amp;gt;B&amp;lt;/sub&amp;gt;-H&amp;lt;sub&amp;gt;C&amp;lt;/sub&amp;gt;. However, the reaction is much faster (no surprise here, resetting the speeds in the MEP mode obviously slows down the process significantly). One interesting feature is perhaps the shape of the &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; curve. With the MEP the curve resembles a logarithmic process, but with the Dynamics simulation it is approximately linear.&lt;br /&gt;
[[File:Mh-004-dynamicsaftermep-hhh.png|thumb|Interatomic distances during the process as simulated in the &#039;&#039;Dynamics&#039;&#039; mode.]]&lt;br /&gt;
&lt;br /&gt;
Exchanging the initial distances shifts the reaction towards the other side of the equilibrium (transition state saddle point), resulting in the other set of products.&lt;br /&gt;
&amp;lt;gallery heights=220px widths=250px&amp;gt;&lt;br /&gt;
Mh-005-dynamicsaftermep-hhh.png | Path towards H + H-H (&#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
Mh-005-dynamicsaftermep2-hhh.png | Path towards H-H + H (&#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt;&#039;&#039; longer)&lt;br /&gt;
&amp;lt;/gallery&amp;gt;&lt;br /&gt;
&lt;br /&gt;
By plotting the momenta of the atoms in time, it was found that at the end of the simulation they were &#039;&#039;p&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 1.230&#039;&#039; and &#039;&#039;p&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 2.481&#039;&#039; (the transition state potential energy roughly divided in 2:1 ratio and converted into kinetic energy). Running the simulation backwards with these momenta (opposite signs to reverse the process) and the final positions &#039;&#039;r&amp;lt;sub&amp;gt;AB&amp;lt;/sub&amp;gt; = 0.746&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;BC&amp;lt;/sub&amp;gt; = 9.006&#039;&#039;  resulted in the molecule going into the transition state. This demonstrates the conservation of energy in the simulation.&lt;br /&gt;
[[File:Mh-005-reversedynamics-hhh.png|thumb|The path for the reverse process (molecule coming back towards the TS) - compare with the figures above demonstrating the dissociation of the TS.|none]]&lt;br /&gt;
&lt;br /&gt;
===Reactive and uncreactive pathways===&lt;br /&gt;
&lt;br /&gt;
The dynamics simulations with the initial momenta as in the Table below with initial distances of &#039;&#039;&#039;r&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;&#039;&#039;&#039; = 0.74 and &#039;&#039;&#039;r&amp;lt;sub&amp;gt;2&amp;lt;/sub&amp;gt;&#039;&#039;&#039; were used to investigate if simply having a high enough momentum is necessary for a succesful collision to occur.&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 !! Comment !! Reactive? !! Contour plot&lt;br /&gt;
|-&lt;br /&gt;
| -1.25 || -2.5  || -99.018 || A successful collision, reaction proceeds. || yes || [[File:Mh-006-react-A.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.0  || -100.456 || The reactants don&#039;t have a sufficient momentum to overcome the activation barrier and no reaction occurs. || no || [[File:Mh-006-react-B.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -1.5  || -2.5  || -98.956 ||Similar to the first case. The higher initial momentum reflects in a higher vibrational energy of the product.|| yes || [[File:Mh-006-react-C.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.0  || -84.956 ||The reactants cross the TS, form the products then revert back to reactants (barrier recrossing). || no || [[File:Mh-006-react-D.png|300px]]&lt;br /&gt;
|-&lt;br /&gt;
| -2.5  || -5.2  || -83.416 || The reactants cross the barrier multiple time and then continue to form the products. || yes  || [[File:Mh-006-react-E.png|300px]]&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;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?&#039;&#039;&#039;&lt;br /&gt;
&lt;br /&gt;
a&lt;br /&gt;
&lt;br /&gt;
== F-H-H System ==&lt;br /&gt;
[[File:Mh-011-FHH-ts.png|thumb|Position of the F-H-H transition state.]]Changing one of the hydrogen atoms for a fluorine atom, the following reaction was investigated:&lt;br /&gt;
&lt;br /&gt;
F + H-H ⇄ HF + H&lt;br /&gt;
&lt;br /&gt;
The transition state was found by carefully adjusting the internuclear distances while keeping the momenta to zero. The process was complicated by the fact the potential energy surface is no longer symmetric and also the forward reaction having a too small activation energy. The distances for which the TS complex remained stationary (at the TS saddle point) were &#039;&#039;r&amp;lt;sub&amp;gt;FHa&amp;lt;/sub&amp;gt; = 1.814&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HaHb&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;. This is an early transition state (with respect to the above reaction) - the H-H bond is almost intact, while the fluorine is at a large distance. Referencing Hammond&#039;s postulate, the structure strongly resembles the reactants.&lt;br /&gt;
&lt;br /&gt;
===Energetic consideration===&lt;br /&gt;
&lt;br /&gt;
As shown in the table below, the energy for each stage of the reaction was found by computing the potential energy (&#039;Initial Geometry Information&#039;) either while in the transition state (with the distances as determined above) or before/after the reaction (large separation between the species, equilibrium bond lengths set to &#039;&#039;r&amp;lt;sub&amp;gt;FH&amp;lt;/sub&amp;gt; = 0.920&#039;&#039; and &#039;&#039;r&amp;lt;sub&amp;gt;HH&amp;lt;/sub&amp;gt; = 0.740&#039;&#039;). The equilibrium bond lengths were determined by an MEP simulation where the interatomic separation converged to the bond length value. The reaction in the forward direction required only a very small activation energy and was found to be overall exothermic.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot; border=1&lt;br /&gt;
! Stage !! Energy&lt;br /&gt;
|-&lt;br /&gt;
| F + HH ||  -104.020&lt;br /&gt;
|-&lt;br /&gt;
| F-H-H (TS) || -103.743&lt;br /&gt;
|-&lt;br /&gt;
| HF + H || -134.025&lt;br /&gt;
|-&lt;br /&gt;
| Forward E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 0.277&lt;br /&gt;
|-&lt;br /&gt;
| Reverse E&amp;lt;sub&amp;gt;A&amp;lt;/sub&amp;gt; || 30.282&lt;br /&gt;
|-&lt;br /&gt;
| Forward ΔE || -30.005 (an exothermic process)&lt;br /&gt;
|}&lt;br /&gt;
&lt;br /&gt;
[[File:Mh-012-FH-bond.png|thumb|MEP determination of the F-H bond length.]]&lt;br /&gt;
[[File:Mh-012-HH-bond.png|thumb|MEP determination of the H-H bond length.]]&lt;/div&gt;</summary>
		<author><name>Mh5015</name></author>
	</entry>
	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-012-FH-bond.png&amp;diff=727809</id>
		<title>File:Mh-012-FH-bond.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-012-FH-bond.png&amp;diff=727809"/>
		<updated>2018-05-23T18:33:53Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: Mh5015 uploaded a new version of File:Mh-012-FH-bond.png&lt;/p&gt;
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		<author><name>Mh5015</name></author>
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	<entry>
		<id>https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-012-FH-bond.png&amp;diff=727808</id>
		<title>File:Mh-012-FH-bond.png</title>
		<link rel="alternate" type="text/html" href="https://chemwiki.ch.ic.ac.uk/index.php?title=File:Mh-012-FH-bond.png&amp;diff=727808"/>
		<updated>2018-05-23T18:33:39Z</updated>

		<summary type="html">&lt;p&gt;Mh5015: &lt;/p&gt;
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