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关于辐射电子附着于CN、C2H和C4H自由基的理论研究。

Theoretical study of radiative electron attachment to CN, C2H, and C4H radicals.

作者信息

Douguet Nicolas, Fonseca dos Santos S, Raoult Maurice, Dulieu Olivier, Orel Ann E, Kokoouline Viatcheslav

机构信息

Department of Chemical Engineering and Materials Science, University of California at Davis, Davis, California 95616, USA.

Laboratoire Aimé Cotton, CNRS/Université Paris-Sud/ENS Cachan, bât. 505, Campus d'Orsay, 91405 Orsay Cedex, France.

出版信息

J Chem Phys. 2015 Jun 21;142(23):234309. doi: 10.1063/1.4922691.

Abstract

A first-principle theoretical approach to study the process of radiative electron attachment is developed and applied to the negative molecular ions CN(-), C4H(-), and C2H(-). Among these anions, the first two have already been observed in the interstellar space. Cross sections and rate coefficients for formation of these ions by direct radiative electron attachment to the corresponding neutral radicals are calculated. For the CN molecule, we also considered the indirect pathway, in which the electron is initially captured through non-Born-Oppenheimer coupling into a vibrationally resonant excited state of the anion, which then stabilizes by radiative decay. We have shown that the contribution of the indirect pathway to the formation of CN(-) is negligible in comparison to the direct mechanism. The obtained rate coefficients for the direct mechanism at 30 K are 7 × 10(-16) cm(3)/s for CN(-), 7 × 10(-17) cm(3)/s for C2H(-), and 2 × 10(-16) cm(3)/s for C4H(-). These rates weakly depend on temperature between 10 K and 100 K. The validity of our calculations is verified by comparing the present theoretical results with data from recent photodetachment experiments.

摘要

一种用于研究辐射电子附着过程的第一性原理理论方法被开发出来,并应用于负离子 CN(-)、C4H(-) 和 C2H(-)。在这些阴离子中,前两种已经在星际空间中被观测到。通过直接辐射电子附着到相应中性自由基形成这些离子的截面和速率系数被计算出来。对于 CN 分子,我们还考虑了间接途径,即电子最初通过非玻恩-奥本海默耦合被捕获到阴离子的振动共振激发态,然后通过辐射衰变稳定下来。我们已经表明,与直接机制相比,间接途径对 CN(-) 形成的贡献可以忽略不计。在 30 K 时,直接机制获得的速率系数对于 CN(-) 为 7×10(-16) cm(3)/s,对于 C2H(-) 为 7×10(-17) cm(3)/s,对于 C4H(-) 为 2×10(-16) cm(3)/s。这些速率在 10 K 到 100 K 之间对温度的依赖性较弱。通过将当前理论结果与近期光剥离实验数据进行比较,验证了我们计算的有效性。

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