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关于 1-丙炔基自由基 (CHCC;XA)与乙烯 (HCCH;XA)的反应动力学的实验与计算综合研究以及 1-戊烯-3-炔 (CHCHCCCH;XA')的形成

A combined experimental and computational study on the reaction dynamics of the 1-propynyl radical (CHCC; XA) with ethylene (HCCH; XA) and the formation of 1-penten-3-yne (CHCHCCCH; XA').

机构信息

Department of Chemistry, University of Hawai'i at Manoa, Honolulu, Hawaii 96822, USA.

Department of Chemistry and Biochemistry, Florida International University, Miami, Florida 33199, USA.

出版信息

Phys Chem Chem Phys. 2019 Oct 28;21(40):22308-22319. doi: 10.1039/c9cp04073k. Epub 2019 Oct 2.

Abstract

The crossed molecular beam reactions of the 1-propynyl radical (CHCC; XA) with ethylene (HCCH; XA) and ethylene-d (DCCD; XA) were performed at collision energies of 31 kJ mol under single collision conditions. Combining our laboratory data with ab initio electronic structure and statistical Rice-Ramsperger-Kassel-Marcus (RRKM) calculations, we reveal that the reaction is initiated by the barrierless addition of the 1-propynyl radical to the π-electron density of the unsaturated hydrocarbon of ethylene leading to a doublet CH intermediate(s) with a life time(s) longer than the rotation period(s). The reaction eventually produces 1-penten-3-yne (p1) plus a hydrogen atom with an overall reaction exoergicity of 111 ± 16 kJ mol. About 35% of p1 originates from the initial collision complex followed by C-H bond rupture via a tight exit transition state located 22 kJ mol above the separated products. The collision complex (i1) can also undergo a [1,2] hydrogen atom shift to the CHCHCCCH intermediate (i2) prior to a hydrogen atom release; RRKM calculations suggest that this pathway contributes to about 65% of p1. In higher density environments such as in combustion flames and circumstellar envelopes of carbon stars close to the central star, 1-penten-3-yne (p1) may eventually form the cyclopentadiene (c-CH) isomer via hydrogen atom assisted isomerization followed by hydrogen abstraction to the cyclopentadienyl radical (c-CH) as an important pathway to key precursors to polycyclic aromatic hydrocarbons (PAHs) and to carbonaceous nanoparticles.

摘要

在单分子碰撞条件下,于 31 kJ mol 的碰撞能下,研究了 1-丙炔基自由基(CHCC;XA)与乙烯(HCCH;XA)和乙烯-d(DCCD;XA)的交叉分子束反应。结合我们的实验室数据与从头算电子结构和统计 RRKM(Rice-Ramsperger-Kassel-Marcus)计算,我们揭示了该反应是由 1-丙炔基自由基对不饱和烃的π电子密度的无势垒加成引发的,导致 CH 双自由基中间体(s)具有长于旋转周期(s)的寿命(s)。反应最终生成 1-戊烯-3-炔(p1)和一个氢原子,总反应为 111±16 kJ mol 放热。约 35%的 p1 来自初始碰撞复合物,随后通过位于分离产物上方 22 kJ mol 的紧密出口过渡态发生 C-H 键断裂。碰撞复合物(i1)也可以在氢原子释放之前经历[1,2]氢原子迁移到 CHCHCCCH 中间体(i2);RRKM 计算表明该途径对 p1 的贡献约为 65%。在密度较高的环境中,如燃烧火焰和碳星的星周包层中,靠近恒星中心的位置,1-戊烯-3-炔(p1)可能通过氢原子辅助异构化形成环戊二烯(c-CH)异构体,然后通过氢原子提取到环戊二烯基自由基(c-CH)作为多环芳烃(PAHs)和碳质纳米颗粒的关键前体的重要途径最终形成环戊二烯(c-CH)。

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