Dynamics of the reaction of C2 with C6H2: An implication for the formation of interstellar C8H

被引:8
|
作者
Sun, Yi-Lun [1 ]
Huang, Wen-Jian [1 ]
Chin, Chih-Hao [1 ]
Lee, Shih-Huang [1 ]
机构
[1] NSRRC, Hsinchu 30076, Taiwan
来源
JOURNAL OF CHEMICAL PHYSICS | 2014年 / 141卷 / 19期
关键词
ASTRONOMICAL DETECTION; CHEMISTRY; MOLECULE; TMC-1; ENVELOPES; CRL-618; CLOUDS; STARS; C2H2; CN;
D O I
10.1063/1.4901981
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
The reaction C-2 + C6H2 -> C8H + H was investigated for the first time. Reactant C-2 (C6H2) was synthesized from 1% C3F6/He (5% C2H2/He) by pulsed high-voltage discharge. We measured the translational-energy distribution, the angular distribution, and the photoionization spectrum of product C8H in a crossed molecular-beam apparatus using synchrotron vacuum-ultraviolet ionization. This reaction released average translational energy of 8.5 kcal mol(-1) corresponding to a fraction of 0.37 in translation. (CH)-H-8 was identified as octatetranyl based on the maximal translational-energy release 23 +/- 2 kcal mol(-1) and the ionization threshold 8.9 +/- 0.2 eV. Kinematic constraints can qualitatively account for the nearly isotropic angular distribution. The quantum-chemical calculations indicate that the exothermic reactions C-2 (X (1)Sigma(+)(g)/a (3)Pi(u)) + HC6H -> C8H + H can proceed without entrance and exit barriers, implying the importance in the cold interstellar medium. This work verifies that interstellar C8H can be formed through the C-2 + C6H2 reaction. (c) 2014 AIP Publishing LLC.
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页数:8
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