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在泰坦的大气中形成腈和亚胺:激发态氮原子 N(2D)与乙烷的反应动力学的组合交叉束和理论研究。

Formation of nitriles and imines in the atmosphere of Titan: combined crossed-beam and theoretical studies on the reaction dynamics of excited nitrogen atoms N(2D) with ethane.

机构信息

Dipartimento di Chimica, Università degli Studi di Perugia, 06123, Perugia, Italy.

出版信息

Faraday Discuss. 2010;147:189-216; discussion 251-82. doi: 10.1039/c004748a.

Abstract

The dynamics of the H-displacement channels in the reaction N(2D) + C2H6 have been investigated by the crossed molecular beam technique with mass spectrometric detection and time-of-flight analysis at two different collision energies (18.0 and 31.4 kJ mol(-1)). From the derived center-of-mass product angular and translational energy distributions the reaction micromechanisms and the product energy partitioning have been obtained. The interpretation of the scattering results is assisted by new ab initio electronic structure calculations of stationary points and product energetics for the C2H6N ground state doublet potential energy surface. C-C bond breaking and NH production channels have been theoretically characterized and the statistical branching ratio derived at the temperatures relevant for the atmosphere of Titan. Methanimine plus CH3 and ethanimine plus H are the main reaction channels. Implications for the atmospheric chemistry of Titan are discussed.

摘要

利用交叉分子束技术,结合质谱检测和飞行时间分析,在两种不同的碰撞能量(18.0 和 31.4 kJ mol(-1))下,研究了反应 N(2D) + C2H6 中 H 位移通道的动力学。从得出的质心产物角向和平动能分布中,获得了反应微观机制和产物能量分配。通过对 C2H6N 基态双重态位能面的新从头算电子结构计算,对散射结果的解释得到了辅助,该计算包括了对定态点和产物能量的计算。C-C 键断裂和 NH 生成通道已在理论上进行了表征,并在与泰坦大气相关的温度下推导出了统计分支比。甲亚胺加 CH3 和乙亚胺加 H 是主要的反应通道。讨论了对泰坦大气化学的影响。

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