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首页> 外文期刊>The journal of physical chemistry, A. Molecules, spectroscopy, kinetics, environment, & general theory >Rate coefficients for the reactions of C-2(a(3)Pi(u)) and C-2(X-1 Sigma(+)(g)) with various hydrocarbons (CH4, C2H2, C2H4, C2H6, and C3H8): A gas-phase experimental study over the temperature range 24-300 K
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Rate coefficients for the reactions of C-2(a(3)Pi(u)) and C-2(X-1 Sigma(+)(g)) with various hydrocarbons (CH4, C2H2, C2H4, C2H6, and C3H8): A gas-phase experimental study over the temperature range 24-300 K

机译:C-2(a(3)Pi(u))和C-2(X-1 Sigma(+)(g))与各种碳氢化合物(CH4,C2H2,C2H4,C2H6和C3H8)反应的速率系数:在24-300 K的温度范围内进行气相实​​验研究

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摘要

The kinetics of reactions of C-2(a(3)Pi(u)) and C-2(X-1 Sigma(+)(g)) with various hydrocarbons (CH4, C2H2, C2H4, C2H6, and C3H8) have been studied in a uniform supersonic flow expansion over the temperature range 24-300 K. Rate coefficients have been obtained by using the pulsed laser photolysis-laser induced fluorescence technique, where both radicals were produced at the same time but detected separately. The reactivity of the triplet state was found to be significantly lower than that of the singlet ground state for all reactants over the whole temperature range of the study. Whereas C-2(X-1 Sigma(+)(g)) reacts with a rate coefficient close to the gas kinetic limit with all hydrocarbons studied apart from CH4, C-2(a(3)Pi(u)) appears to be more sensitive to the molecular and electronic structure of the reactant partners. The latter reacts at least one order of magnitude faster with unsaturated hydrocarbons than with alkanes, and the rate coefficients increase very significantly with the size of the alkane. Results are briefly discussed in terms of their potential astrophysical impact.
机译:C-2(a(3)Pi(u))和C-2(X-1 Sigma(+)(g))与各种烃(CH4,C2H2,C2H4,C2H6和C3H8)的反应动力学具有我们在24-300 K的温度范围内以均匀的超声速流动进行了研究。通过使用脉冲激光光解-激光诱导荧光技术获得了速率系数,其中两个自由基同时产生,但分别检测。发现在整个研究温度范围内,所有反应物的三重态的反应性均显着低于单重态的反应性。 C-2(X-1 Sigma(+)(g))的反应速率系数接近于气体动力学极限,除CH4外,所有已研究的碳氢化合物似乎都与C-2(a(3)Pi(u))反应。对反应伙伴的分子和电子结构更敏感。后者与不饱和烃的反应比与烷烃的反应至少快一个数量级,并且速率系数随烷烃的大小而显着增加。根据其潜在的天体物理影响简要讨论了结果。

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