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MRD:01576020

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Molecular reaction Dynamics Lab Report

Introduction

Modelling the dynamics of molecular reactions has been enabled by the emergence of computers and the field of computational chemistry is an ever-expanding field. Despite most approaches being purely theoretical, ab initio, calculations, the insight given is invaluable for understanding the pathways of chemical reactions. It is often also not necessary to include quantum mechanics, as atoms are of sufficient mass to be reasonably accurately modelled by Newton's equations of motion. Isolated systems in the gas phase only experience interatomic interactions which can be represented by a potential energy surface (PES) which is a function only of atomic positions. The force on a given interatomic coordinate can be calculated as follows:

F=V(r1,r2,...)ri

where F = dpidt

Calculating the forces and adjusting the system in consecutive steps results in a trajectory which shows how a system evolves in time. Such calculations have almost endless application from chemical biology and medicine[1] to materials science[2].


It is worth mentioning some main aspects about the transition state (TS) theory here as it is central to the concepts used here. It is purely classical - it ignores any quantum mechanical effects such as tunnelling, which is incredibly small anyway. It also assumes that the transition state structure is in equilibrium with the reactants, which is called a quasi-equilibrium. TS theory also assumes that the reactants have energies which follow a Boltzmann distribution, which is not a bad assumption as long as the system has had time to equilibrate. This assumption, however is not very applicable to the system studied here. Another crucial assumption of the TS theory, developed in the 1930s, is that once the TS is surpassed, the products will necessarily be formed, which was not the case in some simulations performed here. This latter assumption is also the reason why theoretically derived reaction rates using the TS state theory overestimate experimentally obtained reaction rates. This can be improved by adding a correcting factor, but to do that one must already have extensive knowledge of the system in question. The TS is defined as the maximum on the minimum energy path going from reactants to products. This is called a saddle point and the net force on the system is 0.[3][4]

We will deal here with triatomic linear systems, as depicted in the following Figure 1.

Figure 1. A triatomic system used here. The atoms will either all be Hs or in the last case one H will be replaced with a F. Figure taken from https://wiki.ch.ic.ac.uk/wiki/index.php?title=CP3MD

Terms like reactive and unreactive trajectories will be used often. A reactive trajectory is one which leads the reaction to completeness, i. e. the products are formed. In contrast an unreactive trajectory will not form products. The work here is divided into two exercises. Questions from the script are coloured blue for clarity and the answers follow below.


EXERCISE 1

Dynamics from the TS region

On a potential energy surface diagram, how is the transition state mathematically defined? How can the transition state be identified, and how can it be distinguished from a local minimum of the potential energy surface?

The transition state is defined as the local maximum on the minimum energy path the reactants take when forming products. Mathematically, an extremum of a function is identified by its divergence being the zero vector at that point. To further characterise a point, one needs to evaluate the second derivatives at that point to determine whether it is a maximum or a minimum. The second derivative at the transition state will be negative, corresponding to a local maximum of the potential energy surface (PES). Conversely, if the first derivative is zero and the second is positive, the point in question is a local minimum, which could be the lowest energy structure of the reactants or the products for example.

Good but your mathematical definition for the TS is unclear. Also, the derivatives are partial derivatives Sf3014 (talk) 15:40, 24 May 2020 (BST)


Report your best estimate of the transition state position (rts) and explain your reasoning illustrating it with a “Internuclear Distances vs Time” plot for a relevant trajectory.

A simple system, consisting of a H atom colliding with an H2 molecule was investigated. Firstly, the transition state position was estimated by setting the momenta (p1 and p2) to 0 and, since the system is symmetric, the positions (r1 and r2) equal. By using these initial conditions, we have constrained our system to only move along the path in black in the following figure.


Figure 2. By setting both r1 and r2 equal and momenta = 0, we have constrained our system to only move along the black path shown in this figure. The transition state is the minimum of this line.


The minimum of this curve is the maximum of the lowest energy path. Since the gradient is zero at that point, there should be no movement of our system if the initial structure corresponds to the TS structure. By changing the initial internuclear distances, we can indentify the TS as the distance where the internuclear distances are constant throughout the simulation.


Figure 3. Internuclear distance vs. time plots are shown in this figure. Due to the symmetry of the system, A-B and B-C distances overlay at all times. In graph (a), the initial distances between atoms were 90 pm. In graph (b), atoms were separated by 90.8 pm and in graph (c) the distances were 92 pm.
Figure 4. Contour plot with the initial geometry being the transition state geometry and initial momenta = 0 g.mol-1.pm.fs-1.


We can see that in cases (a) and (c) there were oscillations of the atoms present so the net force on the system was not 0, which means that these are not transition state structures. But looking at these two graphs more thoroughly, we can see that the oscillations began in opposite directions. In case (a) the initial distance was elongated at first, meaning that there was a repulsive force between the atoms and that in the TS the atoms are separated by more than 90 pm. Conversely, in case (c), the distance between atoms was shortened at first, denoting attraction between atoms. We know that the transition state structure will be between these two. There are no noticeable oscillations in case (b), suggesting that the distance between the atoms in the transition state structure will be in close proximity to 90.8 pm.


But we can get a more accurate value now that we know where to look for the transition state. With some interval bisection, our best estimate for the transition state is rTS = 90.775 pm. And most importantly, the forces on this initial geometry are -0.000 kJ/mol.pm along AB and -0.000 kJ/mol.pm along BC so this is the actual saddle point. Of course this is only true for our accuracy, there may be additional decimal points which are not 0. But force fields are not without errors either and such a system would be experimentally almost impossible to construct and study anyway so it makes no sense to improve the precision any further.


The plot on the right confirms that the chosen rTS is correct, since the system did not roll into either of the valleys even in a long simulation.

Very good. For more clarity, you should refer to "(a) and (c)" as fig. 3(a) and (c) Sf3014 (talk) 15:46, 24 May 2020 (BST)


Dynamics vs. MEP

Comment on how the mep and the trajectory you just calculated differ.


In a minimum energy path (MEP) calculation, the momentum of all particles is set to 0 in each step. Therefore there are no vibrations of the molecule at any point of the simulation. Of course this is unphysical as energy is lost, but it can be useful for some applications. In a dynamics simulation, on the other hand, vibrations of the molecule are observed as total energy of the system is constant.


Figure 5. Internuclear distance vs. time plot for r1 = 91.8 pm and r2 = 90.8 pm. As the simulation progresses, atom A moves away from the molecule BC. Molecule BC vibrates, as can be seen from the oscillating distance between atoms B and C. AB and AC distances are rising linearly as the system moves towards the products.
Figure 6. Momenta vs. time plot for r1 = 91.8 pm and r2 = 90.8 pm. As the simulation progresses, atom A moves away from the molecule BC. The AB momentum increases and ultimately moves with constant momentum away from the molecule BC. Molecule BC vibrates, so the momentum BC oscillates.


Using the initial conditions r1=rts and r2=rts+1, the system would roll into the other valley on the PES with similar behaviour to what is described in the figures on the left and right.


If we start another simulation, where the initial positions are the same as the final positions of the previous calculation, and we set the initial momenta to be the inverse of the final momenta, the new simulation will almost reach the transition state and then roll back through the valley. The reason that it does not reach the transition state is that we started slightly off the transition state structure in the previous calculation since otherwise our system would just stay at the transition state. Our first simulation started off with 0 momentum, and only had potential energy as it was very close to the saddle point. During the simulation the potential energy was transformed into kinetic energy (translational and vibrational). We then took this kinetic energy and started transforming it into potential energy again. Since no energy was lost or gained, we reached the exact same point as we started off and then, depending on the length of simulation, the system may roll down the valley again. It will not turn back however, unless we manually revert momenta again.


If we use these initial conditions and run a MEP simulation, the first step will go back uphill, but then as the momenta are set to 0 and new momenta are calculated from the PES, the system will roll back downhill so the initial point of the previous simulation will not be reached.

Good but show that the momenta is set to zero using the mep calculation. Your evidence doesn't support your discussion because you don't show any plots for the mep calculation.Also, fig. 5 is to small to see the BC vibrations mentioned in the caption. Sf3014 (talk) 15:55, 24 May 2020 (BST)


Reactive and Unreactive Trajectories

Complete the table above by adding the total energy, whether the trajectory is reactive or unreactive, and provide a plot of the trajectory and a small description for what happens along the trajectory. What can you conclude from the table?


p1/ g.mol-1.pm.fs-1 p2/ g.mol-1.pm.fs-1 Etot /kJ.mol-1 Reactive? Description of the dynamics Illustration of the trajectory
-2.56 -5.1 -414.280 Yes In this simulation the molecule did not vibrate noticeably at first. The system reached the transition state and then crossed it. As it started rolling into the valley of the reactants the it accumulated some energy in the form of vibration.
-3.1 -4.1 -420.077 No Here, the molecule was vibrating at first and the system did not reach the saddle point but rather turned around and rolled back into the valley of reactants.
-3.1 -5.1 -413.977 Yes This trajectory is also reactive and is quite similar to the first one.
-5.1 -10.1 -357.277 No In this case, the system did cross the saddle point, fluorine and hydrogen collided a few times, but then returned back and reformed reactants. There was a considerable amount of vibration present.
-5.1 -10.6 -349.477 Yes This trajectory is very interesting. The system crossed the transition state and had a structure similar to products but then returned back to the valley of reactants. It eventually crossed the saddle point again and ended up in the valley leading to the products with significant vibration of the product molecule.

In contrast to one of the assumptions of the transition state theory, it is obvious from the table that even if the system has sufficient energy to surpass the kinetic barrier, this is not a guarantee that the reaction will proceed as expected. There is also no general way to determine a reactive trajectory. This is influenced by many factors. There were significant vibrations present in the product molecule, which is a result of conservation of energy and the fact that the reaction is exothermic.

Good layout in table but descriptions on the trajectories are very confusing (note the trajectories show the approach of an atom towards a molecule) and your lack of mention on the approach of the atom to the molecule shows some misunderstanding by you. Clarity needed, there is some mention of fluorine but from the look of the potential energy line spacing on your trajectory plots it looks like the H-H-H system which is the system you should be referring to based on your lab script. Sf3014 (talk) 16:15, 24 May 2020 (BST)


Given the results you have obtained, how will Transition State Theory predictions for reaction rate values compare with experimental values?

As mentioned in the introduction, one of the assumptions of transition state theory is that, once the transition state is surpassed, the system will in all cases end up in the products state. This assumption may cause some discrepancies between theoretical and experimental findings. As we have seen in some cases, even if the saddle point is reached and the system finds itself in the valley of the products, it can end up in the valley of the reactants again, which means that not in all cases does the system reach the products even if it had sufficient energy to overcome the activation energy. The transition state theory therefore overestimates the reaction rate.

Very good description and link to your introduction. Sf3014 (talk) 16:15, 24 May 2020 (BST)


EXERCISE 2

PES inspection

By inspecting the potential energy surfaces, classify the F + H2 and H + HF reactions according to their energetics (endothermic or exothermic). How does this relate to the bond strength of the chemical species involved?Locate the approximate position of the transition state.

Figure 7. Surface plot for the MEP calculation to determine the energy of the HF + H system. A similar calculation was performed to find the energy of the H2 + F system.

The F + H2 --> HF + H reaction is exothermic and H + HF --> H2 + F is endothermic. This means that the HF molecule is more stable than the H2 molecule. This also means that the H-F bond is stronger than the H-H bond. This makes sense as the former has a significant ionic contribution, whereas the H-H bond is purely covalent. This nature is also reflected in the activation energies of the two reactions and the bond dissociation energies. The transition state structure is approximately: AB = 74.478 pm and BC = 181.455 pm, where C is a fluorine atom. For these initial conditions, the forces were: along AB: 0.000 kJ.mol-1.pm-1 and along BC: 0.001 kJ.mol-1.pm-1. Due to these minimum forces, this structure is very close to the TS structure. One can notice that the distance between the H atoms in the TS structure is very close to their bond distance. This phenomenon is expressed in Hammond's postulate which says that the TS structure will resemble that of the species close to it in energy. Since this reaction is very exothermic, the TS structure is close to the structure of reactants which are a H2 molecule and a F atom.

Good but refer to your image. Your description on bond energies can be backed up further using published bond energies for HH and HF. Good description on locating the transition state. More clarity can be gain from relevant simulated plots and by stating the experimental HH bond distance Sf3014 (talk) 16:27, 24 May 2020 (BST)


Report the activation energy for both reactions.

The activation energy for F+H2-->HF+H is approximately 1.05 kJ/mol, whereas the activation energy for the reverse reaction is 126.681 kJ/mol. These were calculated by first finding the energy of the TS structure, which was -433.981 kJ/mol. Energies of the reactants and products were then obtained by performing a MEP simulation starting slightly off the TS structure in both directions (towards the reactants and towards the products, the one for the products is shown in the figure on the right). The calculated energy of the HF + H complex was -360.662 kJ/mol and that of the H2 + F complex was -435.031 kJ/mol. These values were used to calculate the activation energies given above. The obtained values are only approximate as we cannot move the atom infinitely far from the molecule but are nevertheless in good agreement with experimental findings.

Very good. This can be shown clearly using an energy vs time graph Sf3014 (talk) 16:30, 24 May 2020 (BST)


Reaction Dynamics

A reactive set of initial conditions for the F + H2 --> HF + H reaction is the following: AB distance = 230 pm, BC distance = 74 pm, AB momentum = -5.1 g.mol-1.pm.fs-1.

In light of the fact that energy is conserved, discuss the mechanism of release of the reaction energy. Explain how this could be confirmed experimentally.

Since the reaction is exothermic and the system is isolated, there must be a way of release of the excess energy. This energy is released as strong vibrations of the HF molecule. Since the vibration of a H-F bond, in contrast to a H-H bond, results in a change of dipole, electromagnetic radiation from the IR part of the spectrum is emitted as the molecule vibrates. This emitted IR radiation can be experimentally observed by emission vibrational spectroscopy and the production of products can be confirmed.
Figure 8. A GIF showing the animation of the reaction. The system passes the saddle point a few times but eventually forms the products.
Figure 9. A momenta vs. time plot of the above calculation. The momenta vary a lot around the transition state structure so there is not much useful information we can gather from the first 80 fs of the simulation. The system was also going up and down the PES, so we cannot prove that energy was conserved. But once the system is far into the valley and the potential energy is basically constant, we can see that the maximum momenta in the vibrating A-B molecule is constant and so is the momentum of the BC pair which is moving apart, meaning that the total energy of the system is conserved.

Good. Refer to graphs and don't leave all your description in your image caption, the images are meant to support your text not stand alone. This confuses the overall layout Sf3014 (talk) 16:36, 24 May 2020 (BST)


Let's now setup a calculation starting on the side of the reactants of F + H2, at the bottom of the well rHH = 74 pm, an rFH = 238 pm with a momentum pFH = -1.0 g.mol-1.pm.fs-1, and explore several values of pHH in the range -6.1 to 6.1 g.mol-1.pm.fs-1. Note that we are putting more energy into the system than the activation energy. The table below shows some observations and contour plots.

Very good, clear definitions of variables! Makes your descriptions very easy to follow. Sf3014 (talk) 16:43, 24 May 2020 (BST)


pFH/ g.mol-1.pm.fs-1 pHH/ g.mol-1.pm.fs-1 Einitial /kJ.mol-1 Reactive? Observations Illustration of the trajectory
-1.0 -6.1 -402.504 No Here the system passed through the transition state structure, the hydrogen atom collided with the fluorine and then reformed reactants.
-1.0 -6.0 -404.098 No This is very similar to the case above.
-1.0 -5.0 -414.098 No This trajectory is also not reactive and is quite similar to the two above, again there was one collision with the fluorine atom.
-1.0 -4.1 -421.388 No Here, the fluorine atom did not collide with any atoms and the transition state was not surpassed.
-1.0 0.0 -434.098 No Since even less energy was given the picture was very similar to the one above, but the hydrogen atom approached the fluorine even less.
-1.0 2.1 -427.588 No Slightly more energy than above so the atoms were closer but the transition state was still not reached.
-1.0 4.1 -413.188 No This trajectory was more interesting, the fluorine collided twice with one of the hydrogen atoms, but the reactants were reformed afterwards.
-1.0 4.5 -409.348 Yes Interestingly, this trajectory was reactive despite the fact that the system has smaller energy than in some other cases. The total energy is therefore far from being the only parameter that influences the success of a given chemical reaction.
-1.0 6.0 -392.098 No The system was very close to forming products here, fluorine and hydrogen collided 7 times, but the system rolled into the valley of reactants again.
-1.0 6.1 -390.788 No The fluorine and hydrogen only collided once in this simulation. There is a pattern emerging in this table ...
-1.0 7.0 -378.098 No This was very similar to the one above, there was one collision and then the reactants were reformed.

From the table above it is obvious that whether the reaction will result in the formation of products is clearly not dependent only on the energy of vibration of the H2 molecule. We have also seen that these conditions where the molecule and the fluorine atom approach each other rather slowly rarely result in producing products. Maybe increasing the momentum pFH will help ...

For the same initial position, increase slightly the momentum AB, and considerably reduce the overall energy of the system by reducing the momentum BC. What do you observe now?

There is very little vibration in the H2 molecule now and the F atom and the H2 molecule are approaching each other faster than before. The trajectory is reactive and the reaction proceeds with a considerable amount of vibrational energy in the HF molecule.

Good but show the reaction trajectories for the higher translational energy Sf3014 (talk) 17:05, 24 May 2020 (BST)


Let's now focus on the reverse reaction, H + HF. When there is very little vibrational energy in the HF molecule, the trajectories are non reactive, as we increase the vibration strength more and more trajectories become reactive. Why this is so is discussed below (Polanyi's empirical rules).

An example of a reactive trajectory for this reaction would be produced by the following initial conditions: AB distance = 230 pm, BC distance = 74.2 pm, AB momentum = -1 g.mol-1.pm.fs-1 and BC momentum = 14.5 g.mol-1.pm.fs-1. The animation of this rather interesting trajectory is below.

Figure 10. A GIF showing the animation of the reactive trajectory of the HF + H reaction. The system passes the saddle point a few times but eventually forms the products.
Figure 11. A skew plot of the same reactive trajectory as animated on the left.


Discuss how the distribution of energy between different modes (translation and vibration) affect the efficiency of the reaction, and how this is influenced by the position of the transition state.


Polanyi's empirical rules are very useful when we are trying to find suitable initial conditions for a reactive trajectory. These rules tell us what modes need to have sufficient energy for certain types of TSs for a reaction to proceed. For early TSs, translational energy is more efficient than vibrational energy. For late TSs, on the other hand, vibrational energy will be more efficient. Why this is so is discussed in the figure below.

Figure 12. A figure representing the main idea of Polanyi's empirical rules. Translational energy is more important for reactions with an early TS, and vibrational energy is more efficient for reactions with a late TS.

Very good. More examples (trajectory plots) for the H + HF reaction will solidify your point Sf3014 (talk) 17:05, 24 May 2020 (BST)


Conclusions

Two linear triatomic systems, HHH and HHF, were studied here. Their reaction trajectories were of particular interest. Transition state theory was used and the Polanyi's empirical rules were applied in finding suitable initial conditions for reactions. It was shown that even with a relatively simplistic model, without even invoking quantum mechanics, a remarkable amount of information can be gathered about a system and the insight into the dynamics of molecular reactions is eye-opening.

References