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乙腈(CHCN)与捕获的、平动冷却的四氯化碳(CCl₄)的同位素特异性反应

Isotope-specific reactions of acetonitrile (CHCN) with trapped, translationally cold CCl.

作者信息

Krohn O A, Catani K J, Greenberg J, Sundar S P, da Silva G, Lewandowski H J

机构信息

Department of Physics, University of Colorado, Boulder, Colorado 80309, USA.

Department of Chemical Engineering, The University of Melbourne, Parkville 3010, Victoria, Australia.

出版信息

J Chem Phys. 2021 Feb 21;154(7):074305. doi: 10.1063/5.0038113.

Abstract

The gas-phase reaction of CCl with acetonitrile (CHCN) is studied using a linear Paul ion trap coupled to a time-of-flight mass spectrometer. This work builds on a previous study of the reaction of CCl with acetylene [K. J. Catani et al., J. Chem. Phys. 152, 234310 (2020)] and further explores the reactivity of CCl with organic neutral molecules. Both of the reactant species are relevant in observations and models of chemistry in the interstellar medium. Nitriles, in particular, are noted for their relevance in prebiotic chemistry and are found in the atmosphere of Titan, one of Saturn's moons. This work represents one of the first studied reactions of a halogenated carbocation with a nitrile and the first exploration of CCl with a nitrile. Reactant isotopologues are used to unambiguously assign ionic primary products from this reaction: HNCCl and CH . Branching ratios are measured, and both primary products are determined to be equally probable. Quantum chemical and statistical reaction rate theory calculations illuminate pertinent information for interpreting the reaction data, including reaction thermodynamics and a potential energy surface for the reaction, as well as rate constants and branching ratios for the observed products. In particular, the reaction products and potential energy surface stimulate questions regarding the strength and role of the nitrile functional group, which can be further explored with more reactions of this class.

摘要

使用与飞行时间质谱仪耦合的线性保罗离子阱研究了CCl与乙腈(CHCN)的气相反应。这项工作建立在先前对CCl与乙炔反应的研究基础上[K. J. 卡塔尼等人,《化学物理杂志》152, 234310 (2020)],并进一步探索了CCl与有机中性分子的反应活性。这两种反应物在星际介质化学的观测和模型中都具有相关性。特别是腈类化合物,因其在生命起源前化学中的相关性而受到关注,并且在土星的卫星之一土卫六的大气中被发现。这项工作代表了卤代碳正离子与腈类化合物的首批研究反应之一,也是对CCl与腈类化合物的首次探索。使用反应物同位素异构体来明确确定该反应的离子初级产物:HNCCl和CH 。测量了分支比,并且确定两种初级产物的可能性相同。量子化学和统计反应速率理论计算为解释反应数据提供了相关信息,包括反应热力学和反应的势能面,以及观测产物的速率常数和分支比。特别是,反应产物和势能面引发了关于腈官能团的强度和作用的问题,这可以通过这类更多的反应进一步探索。

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