2017
DOI: 10.1002/jcc.24914
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Instanton rate constant calculations close to and above the crossover temperature

Abstract: Canonical instanton theory is known to overestimate the rate constant close to a system-dependent crossover temperature and is inapplicable above that temperature. We compare the accuracy of the reaction rate constants calculated using recent semi-classical rate expressions to those from canonical instanton theory. We show that rate constants calculated purely from solving the stability matrix for the action in degrees of freedom orthogonal to the instanton path is not applicable at arbitrarily low temperature… Show more

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Cited by 33 publications
(35 citation statements)
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“…Yet, close to the crossover temperature, the instanton calculations overestimate the TRC as can be expected owing to the well‐known problems of instanton theory in this regime. Please note that a recently proposed approach can partially alleviate this problem . The results obtained with RPMD are also in good agreement at higher temperature, but less good agreement is found at temperatures below 250 K. The ratios between the TRCs at 300 K, 200 K, and 150 K computed with RPMD and reported here are 1.4, 1.8, and 2.9, respectively.…”
Section: Trcs For the Title Reaction On The Nn1 And Se Pesssupporting
confidence: 49%
“…Yet, close to the crossover temperature, the instanton calculations overestimate the TRC as can be expected owing to the well‐known problems of instanton theory in this regime. Please note that a recently proposed approach can partially alleviate this problem . The results obtained with RPMD are also in good agreement at higher temperature, but less good agreement is found at temperatures below 250 K. The ratios between the TRCs at 300 K, 200 K, and 150 K computed with RPMD and reported here are 1.4, 1.8, and 2.9, respectively.…”
Section: Trcs For the Title Reaction On The Nn1 And Se Pesssupporting
confidence: 49%
“…Some suggestions have been given for avoiding the discontinuity at the crossover temperature [12,56,84,103,167], one of which involves computing the microcanonical rate and integrating over energy to get the thermal rate [19,83]. There is a particular need for a reliable microcanonical theory in the atmospheric and astro-chemistry communities where complex reaction networks occur in low pressure environments such that the molecules do not react under a thermal equilibrium conditions.…”
Section: Discussionmentioning
confidence: 99%
“…Few numerical implementations of Eq. (40) have been performed [15,76] because the stability parameters for the unstable instanton orbit have been shown exhibit poor numerical behaviour [83,84]. This problem is related to the problem of obtaining the monodromy matrix needed for other semiclassical dynamics methods, for which further approximations are often necessary to reduce the numerical errors [85].…”
Section: B Fluctuation Factorsmentioning
confidence: 99%
“…This path is located by a Newton-Raphson optimisation scheme. More details on our implementation of instanton theory are given in , McConnell &Kästner (2017). Reactant partition functions in the bimolecular cases were calculated as products of the partition functions of both separated reactants.…”
Section: Reaction Rate Constantsmentioning
confidence: 99%