Electro-Optical, Electronic and Conformational Transitions of Interstellar Alkyl Molecules at Different Temperatures: An Ab-Initio Study

Aditya Tiwari, G. Tiwari, R. V. Prasad, Dipendra Sharma
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引用次数: 1

Abstract

In this paper, electronic structure of iso-propyl cyanide (i-C3H7CN), gauche-normal-propyl cyanide (g-n-C3H7CN) and anti-normal-propyl cyanide (a-n-C3H7CN) have been optimized using DFT-B3LYP/aug-cc-pVDZ method in neutral and anionic states. Electro-optical properties, HOMO, LUMO and MEP surfaces have been computed in order to check the optical behaviour and chemical reactivity of these interstellar molecules. The a-n-C3H7CN molecule exhibits better electro-optical behaviour than g-n-C3H7CN and iso-C3H7CN molecules. Global reactivity descriptors, adiabatic and vertical electron affinities of these straight and branched alkyl molecules have been investigated. They have negative electron affinities, which means they emit energy in the form of an anion. The distribution of the chemical bonding and electron lone pairs inside the molecules has been discussed using ELF map. Further, the formation of g-n-C3H7CN from i-C3H7CN, a-n-C3H7CN from i-C3H7CN and a-n-C3H7CN from g-n-C3H7CN has been studied using transition state study at temperatures 10K, 298.15K and 500K respectively. Mechanism of formation of g-n-C3H7CN and a-n-C3H7CN from i-C3H7CN at 10K, 298.15K and 500K temperatures along with their physico-chemical properties have been elucidated.
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星际烷基分子在不同温度下的光电、电子和构象转变:Ab-Initio研究
本文采用DFT-B3LYP/aug-cc-pVDZ方法对异丙基氰化物(i-C3H7CN)、间扭正丙基氰化物(g-n-C3H7CN)和反正丙基氰化物(a-n-C3H7CN)在中性和阴离子状态下的电子结构进行了优化。为了检查这些星际分子的光学行为和化学反应性,计算了电光性质、HOMO、LUMO和MEP表面。与g-n-C3H7CN和iso-C3H7CN分子相比,a-n-C3H7CN分子表现出更好的电光行为。研究了这些直链和支链烷基分子的整体反应性描述符、绝热和垂直电子亲和。它们具有负电子亲和,这意味着它们以阴离子的形式释放能量。利用极低频图讨论了分子内化学键和电子孤对的分布。利用过渡态研究分别在10K、298.15K和500K温度下,研究了i-C3H7CN、i-C3H7CN和g-n-C3H7CN分别生成g-n-C3H7CN和a-n-C3H7CN。研究了i-C3H7CN在10K、298.15K和500K温度下生成g-n-C3H7CN和a-n-C3H7CN的机理及其理化性质。
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