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解释气相中强氢键二聚体膦酸及其氘代类似物的红外光谱中 OH 伸缩带的结构:计算研究。

Explaining the structure of the OH stretching band in the IR spectra of strongly hydrogen-bonded dimers of phosphinic acid and their deuterated analogs in the gas phase: a computational study.

机构信息

Department of Chemistry, University of Alberta, Edmonton, Alberta, Canada.

出版信息

J Phys Chem A. 2012 May 10;116(18):4495-509. doi: 10.1021/jp3016084. Epub 2012 Apr 26.

DOI:10.1021/jp3016084
PMID:22489963
Abstract

We present a simulation of the OH stretching band in the gas-phase IR spectra of strongly hydrogen-bonded dimers of phosphinic acid and their deuterated analogs [(R(2)POOH(D), with R = CH(2)Cl, CH(3)], which is based on a model for a centrosymmetric hydrogen-bonded dimer that treats the high-frequency OH stretches harmonically and the low-frequency intermonomer (i.e., O···O) stretches anharmonically. This model takes into account the following effects: anharmonic coupling between the OH and O···O stretching modes; Davydov coupling between the two hydrogen bonds in the dimer; promotion of symmetry-forbidden OH stretching transitions; Fermi resonances between the fundamental of the OH stretches and the overtones of the in- and out-of-plane bending modes involving the OH groups; direct relaxation of the OH stretches; and indirect relaxation of the OH stretches via the O···O stretches. Using a set of physically sound parameters as input into this model, we have captured the main features in the experimental OH(D) bands of these dimers. The effects of key parameters on the spectra are also elucidated. By increasing the number and strength of the Fermi resonances and by promoting symmetry-forbidden OH stretching transitions in our simulations, we directly see the emergence of the ABC structure, which is a characteristic feature in the spectra of very strongly hydrogen-bonded dimers. However, in the case of the deuterated dimers, which do not exhibit the ABC structure, the Fermi resonances are found to be much weaker. The results of this model therefore shed light on the origin of the ABC structure in the IR spectra of strongly hydrogen-bonded dimers, which has been a subject of debate for decades.

摘要

我们提出了一个模拟气相中膦酸及其氘代类似物[(R(2)POOH(D),其中 R = CH(2)Cl,CH(3))强烈氢键二聚体的 OH 伸缩带的模型,该模型基于一个处理高频 OH 伸缩的对称氢键二聚体的模型。伸缩谐频,而低频率的单体间(即 O···O)伸缩非谐。该模型考虑了以下效应:OH 和 O···O 伸缩模式之间的非谐耦合;二聚体中两个氢键之间的 Davydov 耦合;对称禁戒的 OH 伸缩跃迁的促进;涉及 OH 基团的 OH 伸缩基频与面内和面外弯曲模式的泛频之间的 Fermi 共振;OH 伸缩的直接弛豫;以及通过 O···O 伸缩的 OH 伸缩的间接弛豫。使用一组物理上合理的参数作为输入到该模型中,我们捕获了这些二聚体实验 OH(D)带的主要特征。还阐明了关键参数对光谱的影响。通过增加 Fermi 共振的数量和强度以及促进我们模拟中对称禁戒的 OH 伸缩跃迁,我们直接看到了 ABC 结构的出现,这是非常强氢键二聚体光谱的一个特征。然而,在不表现出 ABC 结构的氘代二聚体的情况下,发现 Fermi 共振要弱得多。因此,该模型的结果揭示了强氢键二聚体的 IR 光谱中 ABC 结构的起源,这是几十年来争论的主题。

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