Cangtao
Yin
* and
Gábor
Czakó
*
MTA-SZTE Lendület Computational Reaction Dynamics Research Group, Interdisciplinary Excellence Centre and Department of Physical Chemistry and Materials Science, Institute of Chemistry, University of Szeged, Rerrich Béla tér 1, Szeged H-6720, Hungary. E-mail: cangtaoyin@foxmail.com; gczako@chem.u-szeged.hu
First published on 16th December 2022
A quasi-classical trajectory (QCT) study is performed for the HBr + C2H5 multi-channel reaction using a recently-developed high-level ab initio full-dimensional spin–orbit-corrected potential energy surface (PES) by exciting five different vibrational modes of reactants at five collision energies. The effect of the normal-mode excitations on the reactivity, the mechanism, and the post-reaction energy flow is followed. A significant decrease of the reactivity caused by the longer initial distances of the reactants for the vHBr = 1 reaction at low collision energy (Ecoll) is observed due to the intramolecular vibrational-energy redistribution and the classical nature of the QCT method. All of the three reaction pathways (H-abstraction, Br-abstraction, and H-exchange) are intensely promoted when the HBr-stretching mode is excited. No clear promotion is observed when excitation is imposed to C2H5 except that asymmetric CH-stretching helps the H-exchange process. The enhancement effect of the excitation in the HBr vibrational mode is found to be much more effective than increasing the translational energy, in contrast to the HBr + CH3 reaction. The forward scattering mechanism can be clearly promoted by the excitation of the HBr-stretching mode, or by the high collision energy, indicating the dominance of the direct stripping mechanism in these cases. At low collision energy with no excitation or excitation of any vibrational mode of C2H5, the forward scattering feature is less obvious. At Ecoll = 1 kcal mol−1, when HBr-stretching is excited, the product clearly gains more relative translational energy. However, it is interesting to see that when the excitation is in C2H5, the effect is the opposite, i.e., the product gains less relative translational energy compared to the ground-state reaction.
From the theoretical side, the prototype of this class of reaction, HBr + CH3 → Br + CH4, has been extensively studied in detail. Chen et al.10 located the minimum and transition state of the reaction and further investigated the rate constants by RRKM and G1 theory.11 The thermal rate coefficients calculated by Yu and Nyman12 show a strong nonlinear Arrhenius behavior. Below 550 K they have a negative temperature dependence, whereas a positive activation energy was obtained at higher temperatures. They also found that placing one quantum of energy in the vibrational mode of the H–Br bond stretch enhances the reactivity, whereas one quantum in the umbrella mode of CH3 has the opposite effect. Espinosa-Garcia13 calculated the forward and reverse thermal rate constants and the kinetic isotope effects using variational transition state theory with semiclassical transmission coefficients over a wide temperature range. The theoretical rate constants provided by Sheng et al.14 using improved canonical variational transition state theory incorporating small-curvature tunneling correction are in excellent agreement with the experimental values. Krasnoperov15 developed a modified transition state theory for gas-phase reactions with negative barriers and applied it to the reaction HBr + CH3. Wang et al.16 showed that the individual excitation of the CH3 symmetric stretching mode, the umbrella mode and the HBr stretching mode visibly enhances the reaction while they are all less efficient than the translational energy in promoting the reaction, as expected for an early-barrier reaction. In 2013, one of us17 developed a high-quality full-dimensional PES for the backward Br + CH4 reaction based on CCSD(T)/aug-cc-pwCVTZ-PP-quality ab initio energy points. Later a new version was developed18 by calculating the potential energy at the same ab initio level at 5000 additional geometries in the region of CH3 + HBr van der Waals potential well, and the rate coefficients were determined by QCT calculations. Using the same PES, the integral cross sections were calculated by both a six-degree-of-freedom reduced-dimensional quantum dynamics and the QCT method and very good agreement was found between the two approaches.19 The cross sections were found to diverge when the collision energy decreases, indicating that the reactant attraction is responsible for the dynamics at low collision energy. The quantum mechanical and the quasi-classical rate constants also agree very well and almost exactly reproduce the experimental results at low temperatures up to 540 K.
For the HBr + C2H5 reaction, however, only a small amount of theoretical work has been done, including the evaluation of absolute rate constants and kinetic isotope effects by transition state theory and RRKM theory,20 the calculation of the enthalpy of formation,21 the determination of the temperature dependence over the temperature range from 200 to 1400 K,22 and the analysis of the kinetics by employing RRKM theory.23 The computed rate constants agree well with most experimental data in the literature, and indicate that at temperatures above 850 K, the activation energy may switch from negative to positive.
In 2019 our group24 determined benchmark geometries and energies for the stationary points of the backward reaction Br + C2H6, considering also the H-substitution and the methyl-substitution reaction pathways, by augmenting the CCSD(T)-F12b/aug-cc-pVQZ energies with core-correlation, post-CCSD(T) and spin–orbit corrections. Taking these correction terms into account turns out to be essential to reach subchemical, i.e. 0.5 kcal mol−1, accuracy. Very recently25 we reported a high-level ab initio full-dimensional spin–orbit-corrected PES built from 11364 geometries and energies at the following composite level of theory: ManyHF-based26 UCCSD(T)-F12a/cc-pVDZ-F12(-PP) + SOcorr(MRCI-F12+Q(5,3)/cc-pVDZ-F12),27 where for the Br atom a small-core relativistic effective core potential (ECP)28 is used. The multi-reference computations utilized a minimal active space of 5 electrons on 3 spatial 4p-like orbitals, and the Q Davidson-correction29 estimates higher-order correlation energy effects. The SO computations made use of the Breit–Pauli operator in the interacting-states approach,30 where the SO eigenstates were determined by diagonalizing the 6 × 6 SO matrix whose diagonal elements were replaced by the Davidson-corrected MRCI energies. For the fitting of the energy points of the PES we utilized the Monomial Symmetrization Approach (MSA).31 The ground-state dynamics for the HBr + C2H5 → Br(2P3/2) + C2H6 reaction were also studied in that work. With the purpose of providing more accurate dynamical and mechanistic descriptions, and aiming to achieve the ultimate goal of explaining the temperature dependence of the rate constant behavior, here we investigate the competition between vibrational and translational excitation in the nine-atomic reaction featuring an early barrier slightly submerged below the reactants. The HBr-stretching mode and four selected vibrational modes of the ethyl radical are excited, one at a time and each with one quantum, at five different collision energies. The effects of the different kinds of excitations on the reactivity, the reaction mechanisms, the alternative product channels, and the post-reaction distribution of energy are monitored.
At the beginning of the trajectories, the initial vibrational excitation energies and the zero-point energies (ZPEs) of HBr and C2H5 are set by standard normal-mode sampling.32 The spatial orientations of the reactants are randomly sampled. The initial distance between the center of mass of HBr and the center of mass of C2H5 is (x2 + b2)1/2, where x = 16 bohr and the impact parameter is varied between 0 and bmax (where the reaction probability vanishes) with a step size of 0.5 bohr. Note that the x-dependence of the reactivity is also studied as described in Section III A. 1000 trajectories are run at each b value. The trajectories are propagated with a 0.0726 fs time step until the largest interatomic distance becomes larger than the largest initial one by 1 bohr.
Integral cross sections (σ) for the HBr + C2H5 reaction are calculated by a b-weighted numerical integration of the P(b) opacity functions at each Ecoll. The product ZPE-constraint, i.e., the classical vibrational energy of C2H6 has to be greater than its ZPE on the present PES, only rules out 8/4/3 trajectories from the 5793/4840/8555 reactive trajectories of no/v9/vHBr excitation. So from now on we can safely ignore the differences between the features with and without ZPE constraints. The scattering angle distributions are obtained by binning the cosine of the angle (θ) of the relative velocity vectors of the center of masses of the products and those of the reactants into 10 equidistant bins from −1 to 1. cos(θ) = 1 (θ = 0°) corresponds to forward scattering and cos(θ) = −1 (θ = 180°) corresponds to backward scattering. The initial attack angle distributions for the reactants are calculated by binning the cosine of the angle (α for HBr and β for C2H5) of the velocity vector of the center of mass of the examined reactant and an interatomic vector that is considered as the Br–H bond for HBr and the C–C bond for C2H5. We also use 10 equidistant bins between −1 to 1 like for the scattering angle distributions. For HBr cos(α) = −1 means that HBr approaches with its Br atom side and in the situation of cos(α) = 1 HBr goes with its H atom towards C2H5. While for C2H5 cos(β) = −1 means that C2H5 approaches HBr with its CH3 side and in the situation of cos(β) = 1 C2H5 goes with its CH2 side towards the HBr. The rotational quantum numbers of the C2H6 product are obtained by rounding the lengths of the classical rotational angular momentum vectors, in atomic units, to the nearest integer values.
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Fig. 2 Schematic potential energy diagram of the HBr + C2H5 reaction comparing the classical relative energies obtained on the PES, ManyHF-UCCSD(T)-F12a/cc-pVDZ-F12 + SOcorr(MRCI-F12+Q(5,3)/cc-pVDZ-F12(-PP)) energies at geometries optimized on the PES, UCCSD(T)-F12b/AVDZ relative energies at geometries optimized at UCCSD(T)-F12b/AVDZ or the relativistic all-electron CCSDT(Q)/complete-basis-set-quality benchmark relative energies24 of the stationary points. Five single-excited vibrational energy levels (in parentheses) of the reactants obtained on the PES are also shown. All the energies are given in kcal mol−1. |
Differential cross sections showing the initial distance dependence of the vibrational and rotational energy distributions of the product ethane from the HBr + C2H5 → Br + C2H6 reaction are plotted in Fig. 4.
From Fig. 4 we see that the longer initial distance between reactants only has a minor influence on the post-reaction energy distribution, both in the ground state and excited cases. Thus, these test computations show that the choice of the initial distance did not have any significant effect on our previous results for the ground-state reaction. In the present mode-specific study we use the shorter initial distance (x = 16 bohr) to decrease the time for IVR prior to collision, which may affect the cross sections at low Ecoll as we have just demonstrated. Finally, we emphasize that IVR in the isolated reactants occurs in every QCT study due to classical mechanics and the anharmonic nature of the PES (see, for example, ref. 33, where mode energies of isolated C2H6 as a function of time are examined). This IVR does not necessarily indicate any problem with the PES. For the title reaction the correct asymptotic behavior of the PES is shown in ref. 25.
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Fig. 5 Reaction probabilities as a function of the b impact parameter for the HBr(vHBr = 0, 1) + C2H5(vx = 0, 1) → Br + C2H6 [x = 9, 5, 1, 10] reactions at different collision energies. |
As inspecting the opacity functions shown in Fig. 5, we can observe a significant enhancement for the HBr + C2H5 → Br + C2H6 reaction when vHBr = 1, especially at low collision energy, while the bmax values do not change considerably, and the shape of the opacity functions remain, i.e., the reaction probabilities decrease monotonically with increasing b. Only a minor mode-specificity is seen for the four selected vibrational mode excitations of the ethyl radical.
We also plot the ICS values as a function of the total initial energy in the lower panels of Fig. 6. It gives us better vision that the vibrational excitation of HBr-stretching wins over the effect of increasing translational energy. However, it is not like the case for the HBr + CH3 reaction, where the vibrational excitation is less efficient than the translational energy.16
From Fig. 6 we can also make a reasonable prediction that the H-exchange reaction barrier is not high, probably less than 5 kcal mol−1. However, the hydrogen exchange pathway contribution is still very small. The largest contribution studied in this work belongs to v10 = 1 at Ecoll = 40 kcal mol−1, which is 0.88%, i.e. less than 1/100 compared to the dominant hydrogen-abstraction pathway. This is partly because it is a multi-step reaction, and partly because during the reaction process, in most cases the bromine takes the same hydrogen that it originally carries, and in these cases it does not count as a reaction.
Cross sections for the bromine-abstraction reaction pathway are not plotted here. As can be seen from Fig. 2, the reaction barrier is 21 kcal mol−1. So in the current simulations we only find these reaction trajectories when Ecoll = 40 kcal mol−1, and their contribution to the total reaction is also small, with values of only 0.4% in the ground-state case and 3% in the vHBr = 1 case, and less than 1% for all the other mode-specific cases.
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Fig. 7 Normalized scattering angle distributions for the HBr(vHBr = 0, 1) + C2H5(vx = 0, 1) → Br + C2H6 [x = 9, 5, 1, 10] reactions. |
As can be seen in Fig. 7 the excitation of the HBr-stretching mode can clearly promote the forward scattering mechanism, so can the high collision energy, indicating the dominance of the direct stripping mechanism in these cases. At low collision energy with no excitation or excitation of any vibrational mode of C2H5, the forward scattering feature is less obvious. However, it is quite surprising that the DCS at Ecoll = 1 kcal mol−1 shows more clearly a forward preference than Ecoll = 5 kcal mol−1, which may indicate a different mechanism at low Ecoll. Nevertheless, this forward scattering is consistent with the significantly larger bmax value at low Ecoll (see Fig. 5), because at large b stripping usually occurs resulting in forward scattering.
Normalized initial attack angle distributions for the HBr(vHBr = 0, 1) + C2H5(vx = 0, 1) → Br + C2H6 [x = 9, 5, 1, 10] reactions are plotted in Fig. 8. The reaction favors H-side attack over side-on HBr and the least-preferred Br-side approach, along with increasing collision energy, as expected, because an H–C bond forms in the abstraction process, but no clear mode-specificity is observed. The reaction favors side-on CH3CH2 attack over CH2-side attack and the least-preferred CH3-side approach, without significant mode-specificity. However, with increasing the collision energy, the pattern in the CH3CH2 attack angle is the opposite compared to HBr.
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Fig. 9 Normalized product relative translational energy distributions for the HBr(vHBr = 0, 1) + C2H5(vx = 0, 1) → Br + C2H6 [x = 9, 5, 1, 10] reactions. |
As shown in Fig. 9, no clear mode-specificity is observed at high collision energy. At Ecoll = 1 kcal mol−1, however, when the HBr-stretching mode is excited, the product clearly gains more relative translational energy. This is because the vibrational HBr-stretching energy transfers to translational energy after the H–Br bond is broken. When the excitation is in C2H5, the effect is opposite at Ecoll = 1 kcal mol−1.
The internal energy distributions of the product ethane, plotted in the upper panels of Fig. 10, feature clear mode-specificity with maxima shifting towards higher energies with nearly the value of the excess vibrational energy at low Ecoll. At high Ecoll, however, more collision energy is transferred into the vibrational and rotational degrees of freedom of ethane. Nevertheless, the internal energy excitations of the product ethane mainly come from the reaction energy. Vibrational energy distributions in the upper-middle panels of Fig. 10 confirm the above conclusion, but show a red shift compared to internal energy distribution, due to the fact that some of the vibrational energy is transferred into rotational energy, especially at high Ecoll (lower-middle panels). No significant mode-specificity is observed for the rotational energy or the rotational quantum number distributions, as shown in the lower-middle and lower panels of Fig. 10.
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