Ring-polymer molecular dynamics: Rate coefficient calculations for energetically symmetric (near thermoneutral) insertion reactions (X + H[subscript 2]) HX The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Suleimanov, Yury V., Wendi J. Kong, Hua Guo, and William H. Green. “Ring-Polymer Molecular Dynamics: Rate Coefficient Calculations for Energetically Symmetric (near Thermoneutral) Insertion Reactions (X + H[subscript 2]) HX + H(X = C([superscript 1]D), S([superscript 1]D)).” The Journal of Chemical Physics 141, no. 24 (December 28, 2014): 244103. As Published http://dx.doi.org/10.1063/1.4904080 Publisher American Institute of Physics (AIP) Version Author's final manuscript Accessed Wed May 25 22:14:54 EDT 2016 Citable Link http://hdl.handle.net/1721.1/93151 Terms of Use Creative Commons Attribution-Noncommercial-Share Alike Detailed Terms http://creativecommons.org/licenses/by-nc-sa/4.0/ Ring-Polymer Molecular Dynamics: Rate Coefficient Calculations for Energetically Symmetric (Near Thermoneutral) Insertion Reactions (X+H2) HX + H (X=C(1D), S(1D)) Yury V. Suleimanov1,2, Wendi J. Kong1, Hua Guo3, William H. Green1 1Department of Chemical Engineering, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, Unites States 2Computation-based Science and Technology Research Center, Cyprus Institute, 20 Kavafi Street, Nicosia 2121, Cyprus 3Department of Chemical and Chemical Biology, University of New Mexico, Albuquerque, New Mexico 87131, United States Abstract Following our previous study of prototypical insertion reactions of energetically asymmetric type with the RPMD (Ring-Polymer Molecular Dynamics) method [Y. Li, Y. Suleimanov, and H. Guo, J. Phys. Chem. Lett. 5, 700(2014)], we extend it to two other prototypical insertion reactions with much less exothermicity (near thermoneutral), namely, X + H2 HX + H where X = C(1D), S(1D), in order to assess the accuracy of this method for calculating thermal rate coefficients for this class of reactions. For both chemical reactions, RPMD displays remarkable accuracy and agreement with the previous quantum dynamic results that makes it encouraging for the future application of the RPMD to other barrier-less, complex-forming reactions involving polyatomic reactants with any exothermicity. Introduction Rate coefficients of chemical reactions are a key input in kinetic modeling of various chemical processes that include, but are not limited to combustion, atmospheric chemistry, and chemistry in the interstellar media. Experimental measurements of rate coefficients can sometimes be troublesome, expensive, inaccurate or even impossible under certain conditions, which is why it is indispensible to develop alternative theoretical methods of estimating them.1 Unfortunately, a rigorous computation of rate coefficients using the quantum mechanical formalism via the Schrödinger equation scales exponentially with the system size and is only achievable for systems with just a few atoms.2 Therefore, there is a considerable interest in developing various approximations to quantum dynamics, which would allow rate calculations for much larger systems with reasonable accuracy. Of particular concern is the proper treatment of the quantum mechanical (QM) effects of nuclear motion, such as zero point energy (ZPE) and tunneling. The proper inclusion of these effects is important especially if the reaction involves the transfer of light atoms (such as hydrogen) and takes place at room temperature (or lower) 1 where the QM effects can change the rate coefficient of a chemical reaction by several orders of magnitude.1,3 Numerous transition-state theory (TST) methods for rate calculations were developed in the past,4-7 which are based on various static (short-time) approximations to the classical real-time correlation functions used to describe chemical reactions. Various approximations were developed to include quantum tunneling and ZPE effects which transformed methods based on classical TST to an inexpensive and simple way for determining theoretical rate coefficients, particularly for thermally-activated reactions with significant activation barriers.3 Many TST-based methods require only a small portion of the PES, which greatly reduces the computational effort needed to compute a rate coefficient, and so these practical approximate methods are widely used. However, several persistent issues with the TST assumption limit the accuracy of these rate calculation methods. The main problem is an exponential sensitivity of short-time limits of correlation functions to the choice of the dividing surface that separates reactants from products. Within the TST framework, it is assumed that we can always find a dividing surface that will provide an accurate approximation to the long-time limit of the real-time correlation functions (no recrossings assumption). However, making a proper choice of such a dividing surface is not easy for many complex systems and there is no unambiguous way to treat recrossings within the TST framework as it is inherently a real-time dynamical feature. For some thermally-activated reactions, recrossing plays a crucial role, for instance, in the case of heavy-light-heavy mass combinations10-13. Finding an accurate dividing surface is also challenging for reactions with no or low barriers, and for systems with multiple large-amplitude vibrational modes. Several methods have been developed to try to deal with these problems, e.g. multi-structural methods [ref] and variational transition state theory3, including variable reaction coordinate approaches which allow significant flexibility in constructing improved dividing surfaces.8,9 In these cases, simple methods for approximating ZPE and tunneling effects also tend to become less accurate, the computations become more complex, and larger portions of the PES need to be computed. In the present paper we focus on barrierless insertion-scission reactions, where it is challenging to define the dividing surface and the reaction proceeds through a deep well.14,15 As an alternative to TST, the quasi-classical trajectory (QCT) method was developed in an attempt to treat properly recrossing events.14,16 QCT is a full dimensional approach that treats nuclear motions classically but includes the ZPE effect of the products and reactants. However, QCT does not take into account the change in ZPE along the reaction coordinate and completely ignores the tunneling effect.14,16 The problem with ZPE is particularly significant in the case of the barrier-less reactions: trajectories exiting the potential well may violate the ZPE and lead to substantial errors.14,17,18 2 Recently, another alternative method based on the Ring Polymer Molecular Dynamic (RPMD) theory has been developed19-21 which exhibits several distinctions from both TST and QCT methods. RPMD is a full dimensional approach that uses the classical isomorphism22 between the statistical properties of a quantum particle and a ring polymer consisting of harmonically connected classical copies of the original particle to approximate the real-time quantum dynamics in the system.19-21 Though introduced in an ad hoc manner, this approach turned out to possess several desirable features for calculating chemical reaction rate coefficients. First, at high temperatures where the ring polymer collapses to a single bead, RPMD rate becomes exact. Second, the RPMD method has a well-defined short-time limit related to TST-methods, providing an upper bound on the RPMD rate. Finally, because the RPMD formalism is based on the long-time limit correlation functions, the rate coefficient is independent of the choice of the transition state dividing surface used to compute it. This is an extremely advantageous feature of RPMD, especially when it is challenging to determine the optimal dividing surface of a complex multidimensional reaction. In addition to avoiding the need to define a good dividing surface, RPMD automatically includes effects of large-amplitude motions, anharmonicity, and multidimensional tunneling. However, it is more computationally expensive than TSTbased methods, primarily because it requires more of the PES, and it is more computationally expensive than QCT because it propagates the motion of a ring of many beads to represent each atom. It is therefore important to determine how accurate this new method is, so users can decide whether it is worth the computational cost. In a series of recent studies13,15,17,20,21,23-26,28-32,34 it has been shown that the RPMD method provides accurate rate coefficients when applied to systems with various dimensionalities starting from one-dimensional Eckhart barriers,20,21 atomdiatom13,15,26,32 to more complex polyatomic reactions.17,23-25,28-31 The RPMD rate coefficient captures the ZPE effect almost perfectly, and is within a factor of 2-3 of the exact rate at low temperatures in the so-called deep tunneling regimes, where tunneling dominates. At low temperatures, the RPMD rate theory exhibits systematic behavior: it consistently underestimates rates for energetically symmetric (thermoneutral) reactions, and conversely overestimates rates for significantly asymmetric (endo or exothermic) reactions.26,27 A recent comprehensive test of various quantum transition-state theories and other ratecalculation methods suggested that the RPMD approach is the most accurate and well behaved.32,33 More recently, the RPMD method was applied to insertion chemical reactions.15 Using two prototypical reactions of this type, namely X + H2 HX + H, (where X = N(2D),O(1D)) it has been shown that RPMD can provide very accurate results when compared to the exact quantum mechanical solution. These two very exothermic insertion chemical reactions are highly asymmetric (ΔErxn,0 = -1.25 eV for X =N(2D) and -1.88 eV for X = O(1D), see Fig. 1). In the previous studies of thermally-activated 3 chemical reactions, it has been well established that RPMD provides over- and underestimations of rate coefficients depending on the reaction energy symmetry.26 It is therefore important to assess the accuracy of RPMD for energetically symmetric (or thermoneutral) chemical reactions of the insertion type, which represent the main purpose of this work. To this end, we employ two prototypical complexforming reactions, namely X + H2 HX + H, where the difference in energies between reactants and products is 0.2 and 0.3 eV for X = C(1D) and S(1D), respectively (see Fig. 1). We believe that the results of the present work will provide insights into the performance of the RPMD approach and will be useful in future studies of polyatomic complex-forming chemical reactions. Computational Details All calculations were performed using the RPMDrate code developed by Suleimanov and co-workers.34 The detailed explanation of the RPMD rate theory and computational procedure implemented in this code can be found in Ref. 34. Here we only describe the key steps of the rate calculations. First, we make use of the Bennett-Chandler factorization and express the RPMD rate coefficient in the following form: kRPMD (T ) kQTST (T ; # ) (t ; # ) (1) The first term, kQTST (T ; # ) , designates the static contribution, which depends on the position of the dividing surface and is completely determined by the static equilibrium properties. When the dividing surface is defined in terms of the centroid variables (which is the present case), it coincides with the centroid-density quantum transition-state theory (QTST) rate coefficient.4,5,35 In practice, kQTST (T ; # ) is calculated from the centroid potential of mean force (PMF) along a given reaction coordinate as:34 1 1 2 W ( # )W ( 0) e kQTST (T , # ) 4R2 2 R (2) where μR is the reduced mass between the two reactants, (k BT ) 1 and W ( # ) W (0) represent the free energy difference between the dividing surface and the separated reactants at R , which is usually obtained using umbrella integration along ,36,37 and R is an adjustable parameter chosen to be sufficiently large to make the interaction between the reactants negligible.23,34 The second term in Eq.(1), (t ; # ) , is the dynamic factor (transmission coefficient) which accounts for recrossings at # , counterbalancing kQTST (T ; # ) and 4 securing the independence of the RPMD rate coefficient from the choice of the dividing surface. Usually, the position of # is chosen to correspond with the maximum value of W ( ) to try to minimize the recrossings and accelerate the calculations. The reaction coordinate for the reactions X + H2 (X = C(1D), S(1D)) is determined using two standard dividing surfaces used in all our previous atom-diatom studies (see Eqs.(27),(70), and (77-79) in Ref.13.). Although these dividing surfaces may not be an optimal choice for these particular reactions, they will have no effect on the final result due to the “long-time dynamics” nature of RPMD. For this particular work, the thermal rate coefficients for the C(1D) + H2 and S(1D) + H2 reactions were calculated for three temperatures: 200, 300, and 400 K. The input parameters are outlined in the Table 1 and are similar to previous ones used in the recent RPMDrate study of exothermic insertion chemical reactions15 as well as several previous studies of thermally-activated chemical reactions. RPMDrate provides a convenient parallel computing option that speeds up the recrossing factor calculations.15,34 These calculations require more effort to converge in the case of complex-forming chemical reactions, due to much longer times of the propagation of the recrossings. The RPMD calculations were carried out using 128 ring polymer beads. For the PMF calculations, we divided the interval of the reaction coordinate , between -0.05 and 1.05 in windows of .01. The end of umbrella integration corresponded to the intermediate configuration along the reaction path between reactants and products (see Table 1). In each window 200 constrained RPMD trajectories of 100 ps were run, in which the first 20 ps were used for thermalization in the presence of an Andersen thermostat.38 The time step was set to 0.0001 ps. For each window i, a bias is applied to its center by adding a harmonic potential of the type k( - i)2 to the Hamilton function of the system. In doing so, the trajectory is biased to explore in the vicinity of ξi.. Therefore, the force constant must be large enough to constrain the sampling to a region about the vicinity of ξi, but small enough to allow overlapping between adjacent ξ distributions.36,37 To obtain the transmission coefficient, (t ; # ) , a long “parent” trajectory of 2 ns is run after a thermalization period of 20 ps in the presence of an Andersen thermostat with the constraint of having its centroid pinned at # , which corresponds to the maximum value of the PMF. Once every 2 ps, configurations are taken from the parent trajectory as initial conditions for 100 unconstrained “daughter” trajectories. All daughters’ trajectories are run for 2 ps (C + H2) or 3 ps (S + H2) with different initial momenta and without either the constraint or the thermostat to accumulate the transmission coefficient. The parameters used in our calculations are summarized in Table 1 and they were checked to be sufficient to converge RPMD rate coefficients to within a statistical error of ∼10%. 5 Similar to the previous theoretical studies, we assume that the reaction occurs in a low pressure gas and we do not consider pressure dependence (thermal bath effects). For the C + H2 reaction, the potential energy surface (PES) of Banares et al.39 was used. For the S + H2 reaction, the PES of Ho et al.40 was used. These PESs were the same used in the earlier quantum dynamics calculations of rate coefficients. The final rate coefficients were corrected by electronic partition functions: Qel = 5 was used for both reactions. Discussion The PMFs for the C + H2 and S + H2 reactions are plotted in Figures 2a and 2b, respectively. These PMF profiles demonstrate several important features. First, they show that these reactions do indeed proceed through complex formation, which corresponds to deep wells of the free energy along the reaction coordinate. Second, they also confirm that the free energy does not change much until the reaction gets in the complex formation zone. This is because there is no significant bottleneck in the PESs. Finally, the shapes of the free-energy profiles do not change much with the temperature and do not exhibit any significant activation free-energy barrier. This situation is very similar to the O(1D) + H2 reaction discussed in our previous work.15 A small increase of the free energy (below 0.04 eV for C(1D) + H2 and below 0.02 eV for S(1D) + H2) occurs prior to the complex (deep well); this is due to the entropic factor and is weakly temperature dependent as expected. For the second step in the RPMDrate calculations, the recrossings calculations, we selected the positions of the free-energy barriers for both systems as the initial conditions. The recrossings factor profiles are plotted for both reactions in Figures 3a (C(1D) + H2) and 3b (S(1D) + H2). Comparing the two reaction profiles, one can first notice that both reach the plateau regime only after several picoseconds. This extremely long time for the convergence of the transmission coefficients is a characteristic of the complex-forming reaction mechanism.14,15 For reactions over barriers, the plateau region is typically reached about an order of magnitude faster. Although the recrossing factors reach practically the same plateau values for all temperatures, the profiles for various temperatures are quite different. They exhibit short-time oscillations apparently due to entering and re-entering in the complex formation zone at short times, which are more active at higher temperature thus taking less time to reach the plateau. Note that these short-time oscillations are due to our particular choice of a transition-state dividing surface which has no effect on the final rates. In all cases the recrossing factors are significantly below 1 (in the range of 0.30-0.34 for S + H2 and ~0.47 for C + H2), confirming the importance of the inclusion of this factor in the total rate coefficient calculation. Table 2 compares the RPMD rate coefficients with theoretical and experimental results from the previous works.41-45 The title reactions are barrierless, thus, reflecting very weak temperature dependence of the present RPMD results. Indeed, 6 such weak temperature dependence has been observed for the S(1D) + H2 reaction.45 Table 2 also shows that it is very important to take into account the recrossing effect since the kQTST values are too high compared to the Quantum Dynamics (QD) ones. In the case of the S + H2 reaction, the centroid-density QTST rates exhibit nonsystematic temperature dependence. This might be due to the fact that the freeenergy barrier just before the entrance into the H2S well becomes so tiny at 200 K that the free-energy maximum in the entrance channel is attained in the asymptote region (see Fig. 2). Correcting kQTST with gives us the RPMD value, which turns out to be in a very good agreement with the QD results with an error of ~ 5-10%. This deviation is the right order of magnitude to be due to the statistical sampling uncertainties in the RPMD calculations, but this deviation may also be due in part to approximations made in the QD calculations: a quantum statistical model46-48 was used and high rotational states were cut off in the quantum calculation. While the RPMD and QD calculations agree very closely with each other, and they are within the error bar of the experimental measurement for C(1D)+H2, they are both about 25% less than the experimental measurement for S(1D)+H2 at 300 K. It is most likely that the discrepancy between experiment and theory is due to deficiencies in the PES used in the present and previous41,43 dynamical calculations, but other effects (e.g. the calculations completely ignore the low-lying triplet electronic surface; the experiments assume there are no significant side channels) may also contribute. The present results suggest less sensitivity of RPMD to the energetics of insertion-type chemical reactions compared to the previously studied thermallyactivated ones.26 The two title reactions feature relatively small energy differences between reactants and products - 0.17 eV and 0.30 eV for C(1D) + H2 and S(1D) + H2, respectively (see Fig. 1).14 According to the reaction symmetry assignment used for thermally-activated chemical reactions to predict whether RPMD over- or underestimates the rates at low temperatures26,27 they would technically be classified as “effectively symmetric” (or, alternatively, “weakly asymmetric”). For symmetric reactions with barriers RPMD has been found to systematically underestimate the low-temperature rates. However, our results demonstrate that RPMD slightly overestimates them for insertion reactions with low exothermicity and therefore this prediction doesn’t work in the present case. This is not surprising as this prediction was developed for reactions dominated by a significant barrier, where tunneling was significant.26,27 The present (and previous15) RPMD calculations for prototypical insertion-type reactions suggest that RPMD slightly overestimates the rates for this class of reactions. However, such conclusion is rather speculative and more extensive accuracy assessment of RPMD for barrierless reactions is required, similar to numerous recent studies of thermally-activated chemical reactions.13,15,17,23-26,28-32,34 Nevertheless, the level of accuracy that RPMD provides for the insertion reactions is indeed remarkable and suggests that it has the potential to be used for polyatomic reactions involving reaction intermediates, when high accuracy is desired. 7 Conclusions To summarize, in this work, the RPMD method is extended to two prototype energetically symmetric (near thermoneutral) insertion reactions, namely, X + H2 HX + H, where X = C(1D), S(1D). Calculating rate coefficients for this type of reactions is challenging. A significant amount of recrossing occurs along the reaction coordinate because there is no identifiable reaction barrier, and there is a deep well. Fortunately, the computational strategy developed for calculating RPMD rate coefficients can effectively handle recrossing calculations for many types of chemical reactions. In this work, we observed very similar results as to those obtained previously for two energetically asymmetric (with more significant exothermicity) insertion reactions (X = N(2D), O(1D)). The results are in a very good agreement with the previous quantum dynamics calculations for these reactions and thus encouraging for future applications to complex-forming polyatomic chemical reactions with various energetics of reactants and products channels. The present results also suggest that RPMD is less sensitive to the energetics of insertion chemical reactions compared to the previously studied thermally-activated ones, perhaps because tunneling is less important for barrierless reactions. More studies of chemical reactions from this class of reaction with RPMD are required in order to assess accuracy of this novel method. Acknowledgements: Y.V.S. and W.H.G. acknowledge the support of the Combustion Energy Frontier Research Center, an Energy Frontier Research Center funded by the U.S. Department of Energy, Office of Basic Energy Sciences under Award Number DE-SC0001198. WJK thanks the MIT Energy Initiative for support. HG thanks DOE (DE-FG02-05ER15694) for support. References: 1 S. C. Althorpe and D. C. Clary, Annu. Rev. Phys. Chem. 54, 493 (2003). 2 U. Manthe, Mol. Phys. 109, 1415 (2011). 3 A. Fernández-Ramos, J. A. Miller, S. J. Klippenstein, and D. G. Truhlar, Chem. Rev. 106, 4518 (2006). 4 M. J. Gillan, Phys. Rev. Lett. 58, 563 (1987). 5 G. A. Voth, D. Chandler, and W. H. Miller, J. Chem. Phys. 91, 7749 (1989). 6 W. H. Miller, Y. Zhao, M. Ceotto, and S. Yang, J. Chem. Phys.119, 1329 (2003). 7 W. H. Miller, J. Chem. Phys. 62, 1899 (1975). 8 S. J. Klippenstein, J. Phys. Chem. 98, 11459(1994). 9 S. H. Robertson, D. M. Wardlaw, and A. F. Wagner, J. Chem. Phys. 117, 593 (2002). 10 D. G. Truhlar, A.D. Issacson, B.C. Garrett, and M. Bear Ed., CRC: Boca Raton (1985). 11 W. T Duncan and T. N. Truong, J. Chem. Phys. 103, 9642 (1995). 12 J. Espinosa-García and J. C. Corchado, J. Chem. Phys. 105, 3517 (1996). 13 R. Collepardo-Guevara, Y. V. Suleimanov, and D. E. Manolopoulos, J. Chem. Phys. 130, 174713 (2009); Ibid. 133, 049902 (2010). 14 H. Guo, Int. Rev. Phys. Chem. 31, 1 (2012). 15 Y. Li, Y. V. Suleimanov, and H. Guo, J. Phys. Chem. Lett. 5, 700 (2014). 16 J. M. Bowman and G. C. Schatz, Annu. Rev. Phys. Chem. 46, 169(1995). 8 17 R. Pérez de Tudela, Y. V. Suleimanov, M. Menendez, F. Castillo, and F. J. Aoiz, Phys. Chem. Chem. Phys. 16, 2920 (2014). 18 A. J. C. Varandas, Chem. Phys. Lett. 225, 18 (1994). 19 I. R Craig and D.E. Manolopoulos, J. Chem. Phys. 121, 3368 (2004). 20 I. R Craig and D.E. Manolopoulos, J. Chem. Phys. 122, 084106 (2005). 21 I. R Craig and D.E. Manolopoulos, J. Chem. Phys. 123, 034102 (2005). 22 D. Chandler and P.G. Wolynes, J. Chem. Phys. 74, 4078 (1981). 23 Y. V. Suleimanov, R. Collepardo-Guevara, and D. E. Manolopoulos, J. Chem. Phys. 134, 044131 (2011). 24 Y. Li, Y. V. Suleimanov, M. Yang, W. H. Green, and H. Guo, J. Phys. Chem. Lett. 4, 48 (2013). 25 Y. Li, Y. V. Suleimanov, J. Li, W. H. Green, and H. Guo, J. Chem. Phys. 138, 094307 (2013). 26 Y. V. Suleimanov, R. Pérez de Tudela, P. G. Jambrina, J. F. Castillo, V. Sáez-Rábanos, and D. E. Manolopoulos, F. J. Aoiz, Phys. Chem. Chem. Phys. 15, 3655 (2013). 27 J. O. Richardson and S. C. Althorpe, J. Chem. Phys. 131, 214106 (2009). 28 J. W. Allen, W. H. Green, Y. Li, H. Guo, and Y. V. Suleimanov, J. Chem. Phys. 138, 221103 (2013). 29 J. Espinosa-Garcia, A. Fernandez-Ramos, Y. V. Suleimanov, and J. C. Corchado, J. Phys. Chem. A 118, 554 (2014). 30 Y. Li, Y. V. Suleimanov, W. H. Green, and H. Guo, J. Phys. Chem. A 118, 1989 (2014). 31 E. Gonzalez-Lavado, J. Carlos Corchado, Y. V. Suleimanov, W. H. Green, and J. Espinosa-Garcia, J. Phys. Chem. A 118, 3243 (2014). 32 R. P. de Tudela,Y. V. Suleimanov, J. O. Richardson, V. Sáez-Rábanos, W. H. Green, and F. J. Aoiz, in preparation (2014). 33 Y. Zhang, T. Stecher, M. T. Cvitaš and S. C. Althorpe, J. Phys. Chem. Lett. 5, 3976 (2014). 34 Y. V. Suleimanov, J. W. Allen, and W. H. Green, Comput. Phys. Commun. 184, 833(2013). 35 M. J. Gillan, J. Phys. C 20, 3621(1987). 36 J. Kästner and W. Thiel, J. Chem. Phys. 123, 144104(2005). 37 J. Kästner and W. Thiel, J. Chem. Phys.124, 234106 (2006). 38 N. F. Hansen and H. C. Andersen, J. Chem. Phys. 101, 6032 (1994); J. Phys. Chem. 100, 1137 (1996). 39 L. Banares, F. J. Aoiz, S. A. Vazquez, T.-S. Ho, and H. Rabitz, Chem. Phys. Lett. 374, 243 (2003). 40 T.-S. Ho, T. Hollebeek, H. Rabitz, S. D. Chao, R. T. Skodje, A. S. Zyubin, and A. M. Mebel, J. Chem. Phys. 116, 4124 (2002). 41 S. Y. Lin and H. Guo, J. Phys. Chem. A. 108, 10066 (2004). 42 K. Sato, N. Ishisa, T. Kurakata, A. Iwasaki, and S. Tsuneyuki, Chem. Phys. 237, 195 (1998). 43 S. Y. Lin and H. Guo, J. Chem. Phys. 122, 074304 (2005). 44 G. Black and L. E. Jusinki, J. Chem. Phys. 82, 789 (1985). 45 C. Berteloite, M. Lara, A. Bergeat, S. Le Picard, F. Dayou, K. M. Hickson, A. Canosa, C. Naulin, J.-M. Launay, I. R. Sims and M. Costes, Phys. Rev. Lett. 105, 203201 (2010). 9 E. J. Rackham, F. Huarte-Larrañaga and D. E. Manolopoulos, Chem. Phys. Lett. 343, 356 (2001). 47 E. J. Rackham, T. Gonzalez-Lezana and D. E. Manolopoulos, J. Chem. Phys. 119, 12895 (2003). 48 S. Y. Lin and H. Guo, J. Chem. Phys. 120, 9907 (2004). 46 10 Table 1 Input parameters for the RPMDrate calculations on the C +H2 and S + H2 reactions. The explanation of the format of the input file can be found in the RPMDrate code manual (see Ref. 34 and http://www.mit.edu/~ysuleyma/rpmdrate). Parameter Reaction C(1D) + H2 S(1D) + H2 400 300 200 128 400 300 200 128 Temperature (K) 20 20 Nbond 1 1 Nchannel 2 2 Dividing surface s1 parameter (a ) Number of forming and breaking bonds Number of equivalent product channels X(1D) H H (1.635 a , 1.302 a , 0.000 a ) (0.000 a , 0.000 a , 0.000 a ) (3.270 a , 0.000 a , 0.000 a ) (0.376 Å, 2.110 Å, 0.000 Å) (0.000 Å, 0.000 Å, 0.000 Å) (0.751 Å, 0.000 Å, 0.000 Å) Cartesian coordinates (x, y, z) of the intermediate geometry Thermostat Biased sampling parameters Nwindows ξ1 dξ ξN dt ki ‘Andersen’ ‘Andersen’ Thermostat option 111 -0.05 0.01 1.05 0.0001 2.72 111 -0.05 0.01 1.05 0.0001 2.72 Ntrajectory tequilibration tsampling 200 20 100 200 20 100 Ni 2 × 108 2 × 108 Number of Windows Center of the first window Window spacing step Center of the last window Time step (ps) Umbrella force constant ((T/K) eV) Number of trajectories Equilibration period (ps) Sampling period in each trajectory (ps) Total number of sampling points 0.00 0.604 (400 K)* 0.599 (300 K)* 0.492 (200 K)* 5000 0.00 0.886 (400 K)* 0.875 (300 K)* 0.403(200 K)*,^ 5000 Start of umbrella integration End of umbrella integration 0.0001 20 0.0001 20 Ntotalchild 200000 200000 tchildsampling 3 3 Nchild 100 100 tchild 2 3 Time step (ps) Equilibration period (ps) in the constrained (parent) trajectory Total number of unconstrained (child) trajectories Sampling increment along the parent trajectory(ps) Number of child trajectories per one initially constrained configuration Length of child trajectories (ps) Command line parameters Temp Nbeads Dividing surface parameters R∞ Explanation Number of Beads 0 Potential of mean force calculation ξ0 ξ‡ Nbins Recrossing factor calculation dt tequilibration 0 0 0 0 0 0 0 0 0 Number of bins *Detected automatically by RPMDrate; ^ In the case of the chemical reaction S+H2, the maximum of the free energy at 200 K occurs before entering the complex-formation region. 11 Table 2 Comparison between RPMD Rate Coefficients (cm3s-1) of the C(1D) + H2 and S(1D) + H2 chemical reactions with the previous theoretical and experimental results. C(1D) + H2 T/K kQTST κ kRPMD QD41 Expt.42 200 3.09×10-10 0.48 1.47×10-11 --- T/K kQTST κ kRPMD QD43 Expt.44 Expt.45 200 4.64×10-10 0.34 1.60×10-10 ---- 300 3.35×10-10 0.47 1.57×10-10 1.50×10-10 (2.0±0.6)×10-10 400 3.56×10-10 0.47 1.66×10-10 --- 300 5.32×10-10 0.30 1.62×10-10 1.49×10-10 2.1×10-10 2.07×10-10 400 4.95×10-10 0.33 1.63×10-10 ---- S(1D) + H2 12 1 O( D) + H2 N(1D) + H2 C(1D) + H2 S(1D) + H2 CH + H SH + H 0.17 eV 0.30 eV NH + H 1.25 eV OH + H 1.88 eV SH2 CH2 3.90 eV 4.33 eV NH2 5.48 eV OH2 7.29 eV Figure 1. Energetics of four prototypical insertion reactions X + H2 XH + H (X = S(1D), C(1D), N(2D), O(1D)) on the lowest electronic state of the specified multiplicity. 13 0.05 W() / eV 0.00 C + H2 -0.05 T = 200 K T = 300 K T = 400 K -0.10 -0.15 -0.20 (a) -0.25 -0.30 0.0 0.1 0.2 0.3 0.4 W() / eV 0.05 0.5 0.6 0.7 0.8 0.00 S + H2 -0.05 -0.10 -0.15 (b) -0.20 -0.25 0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 Figure 2. Ring polymer potentials of mean force (W()) along the reaction coordinate for the C(1D) + H2(top panel) and S(1D) + H2 (bottom panel) chemical reactions at 200, 300 and 400 K. 14 1.0 0.9 C + H2 0.8 (t) T = 400 K T = 300 K T = 200 K 0.7 0.6 (a) 0.5 0.4 1.0 0 500 1000 1500 2000 t / fs (t) 0.8 S + H2 0.6 (b) 0.4 0.2 0 500 1000 1500 2000 2500 3000 t / fs Figure 3. Ring polymer recrossing factors ((t)) along the reaction coordinate for the C(1D) + H2(top panel) and S(1D) + H2 (bottom panel) chemical reactions at 200, 300 and 400 K. 15