Theoretical Study on Formamide (NH2CHO) and Methylidene (CH2) Reactions for the Formation of Interstellar N-Methylformamide

Shivani, Aftab Ahamad, Manish K. Singh, K. Singh, Alka Misra, P. Tandon
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Abstract

N-methylformamide (NMF), E & Z containing an amide bond, a vital component of peptides, is one of the simplest derivatives of formamides. It is detected towards the hot molecular core of the Sgr B2(N2) molecular cloud with the Atacama Large Millimeter/submillimeter Array (ALMA). It is proposed that the radical-molecule mechanism can be used as a strong contrivance to investigate the formation of NMF in the interstellar medium (ISM) via some interstellar molecules like methylidene CH2(1Σ1 & 3Σ1) and formamide (NH2CHO). The density functional theory (DFT) at B3LYP/6-311G (d,p) has been applied to study the mechanisms. All the possible cases of E- & Z-NMF formation with singlet and triplet CH2 have been investigated. It is found that the formation of E-NMF with CH2(1Σ1) and Z-NMF with CH2(3Σ1) is more feasible and favorable in comparison to E-NMF formation from CH2(3Σ1) and Z-NMF with CH2(1Σ1).
甲酰胺(NH2CHO)与亚甲基(CH2)反应生成星际n -甲基甲酰胺的理论研究
n -甲基甲酰胺(NMF)是甲酰胺类化合物中最简单的衍生物之一,含有一个酰胺键,是肽的重要组成部分。它是用阿塔卡马大型毫米/亚毫米阵列(ALMA)探测到的Sgr B2(N2)分子云的热分子核心。提出了自由基分子机制可以作为研究星际介质(ISM)中通过亚甲基CH2(1Σ1 & 3Σ1)和甲酰胺(NH2CHO)等星际分子形成NMF的有力手段。利用B3LYP/6-311G (d,p)的密度泛函理论(DFT)研究了其机理。研究了所有可能的由CH2单线态和三重态形成E-和Z-NMF的情况。与CH2(3Σ1)和Z-NMF与CH2(1Σ1)形成E-NMF相比,E-NMF与CH2(1Σ1)和Z-NMF与CH2(3Σ1)形成更为可行和有利。
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