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半经典传输系数的修正

Corrections to Semiclassical Transmission Coefficients.

作者信息

Upadhyayula Sameernandan, Pollak Eli

机构信息

Chemical and Biological Physics Department, Weizmann Institute of Science, Rehovot 76100, Israel.

出版信息

J Phys Chem A. 2024 May 2;128(17):3434-3448. doi: 10.1021/acs.jpca.4c00452. Epub 2024 Apr 17.

DOI:10.1021/acs.jpca.4c00452
PMID:38630022
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11077496/
Abstract

The uniform semiclassical expression for the energy-dependent transmission probability through a barrier has been a staple of reaction rate theory for almost 90 years. Yet, when using the classical Euclidean action, the transmission probability is identical to 1/2 when the energy equals the barrier height since the Euclidean action vanishes at this energy. This result is generally incorrect. It also leads to an inaccurate estimate of the leading order term in an expansion of the thermal transmission coefficient. The central result of this paper is that adding an dependent correction to the uniform semiclassical expression, whether as a constant action or as a shift in the energy scale, not only corrects this inaccuracy but also leads to a theory that is more accurate than the previous one for almost any energy. Shifting the energy scale is a generalization of the vibrational perturbation theory 2 (VPT2) and is much more accurate than the "standard" VPT2 theory, especially when the potential is asymmetric. Shifting the action by a constant is a generalization of a result obtained by Yasumori and Fueki (YF) only for the Eckart barrier. The resulting modified VPT2 and YF semiclassical theories are applied to the symmetric and asymmetric Eckart barrier, a Gaussian barrier, and a tanh barrier. The one-dimensional theories are also generalized to many-dimensional systems. Their effect on the thermal instanton theory is discussed.

摘要

近90年来,穿过势垒的能量相关透射概率的统一半经典表达式一直是反应速率理论的核心内容。然而,当使用经典欧几里得作用量时,能量等于势垒高度时透射概率等于1/2,因为欧几里得作用量在此能量下为零。这个结果通常是不正确的。它还会导致对热透射系数展开式中首项的估计不准确。本文的核心结果是,对统一半经典表达式添加一个与能量相关的修正项,无论是作为常数作用量还是作为能量尺度的偏移,不仅能纠正这种不准确,而且对于几乎任何能量而言,都能得到一个比之前理论更精确的理论。能量尺度的偏移是振动微扰理论2(VPT2)的推广,并且比“标准”VPT2理论精确得多,特别是当势不对称时。通过一个常数来移动作用量是Yasumori和Fueki(YF)仅针对埃卡特势垒得到的一个结果的推广。由此得到的修正VPT2和YF半经典理论被应用于对称和不对称的埃卡特势垒、高斯势垒以及双曲正切势垒。一维理论也被推广到多维系统。讨论了它们对热瞬子理论的影响。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/11206c86019f/jp4c00452_0006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/99ba91b372a8/jp4c00452_0001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/24e960311ea0/jp4c00452_0002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/8b32e8316af6/jp4c00452_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/0a09bb513995/jp4c00452_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/b3777be30544/jp4c00452_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/11206c86019f/jp4c00452_0006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/99ba91b372a8/jp4c00452_0001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/24e960311ea0/jp4c00452_0002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/8b32e8316af6/jp4c00452_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/0a09bb513995/jp4c00452_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/b3777be30544/jp4c00452_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d37/11077496/11206c86019f/jp4c00452_0006.jpg

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J Phys Chem Lett. 2023 Nov 9;14(44):9892-9899. doi: 10.1021/acs.jpclett.3c02779. Epub 2023 Oct 31.
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ℏ expansion of the transmission probability through a barrier.通过势垒的传输概率的 ℏ 展开。
J Chem Phys. 2022 Aug 21;157(7):074109. doi: 10.1063/5.0106649.
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Faraday Discuss. 2022 Oct 21;238(0):204-235. doi: 10.1039/d2fd00063f.
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Semiclassical transition state theory based on fourth order vibrational perturbation theory: Model system studies beyond symmetric Eckart barrier.基于四阶振动微扰理论的半经典过渡态理论:超越对称 Eckart 势垒的模型体系研究。
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Perspective: Ring-polymer instanton theory.观点:环聚合物瞬时理论。
J Chem Phys. 2018 May 28;148(20):200901. doi: 10.1063/1.5028352.
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Quantum tunneling during interstellar surface-catalyzed formation of water: the reaction H + HO → HO + OH.星际表面催化形成水过程中的量子隧穿:反应H + HO → HO + OH
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