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氦原子碰撞诱导 NCCN 转动跃迁的量子动力学研究。

Quantum dynamics study of rotational transitions of NCCN induced by He collision.

机构信息

Department of Chemistry, Indian Institute of Technology Ropar, Rupnagar 140001, India.

出版信息

J Chem Phys. 2018 Nov 7;149(17):174312. doi: 10.1063/1.5058126.

Abstract

Quantum dynamics of the molecule cyanogen (NCCN) and its collision with helium taking place in the interstellar medium has been studied. An potential energy surface of NCCN-He, a van der Waals complex, is generated using the high-level single reference coupled-cluster with single and double and perturbative triple excitation method and aug-cc-pVQZ basis sets. Using the multipole expansion, Legendre coefficients have been calculated and utilized in determining collisional cross sections. Close-coupling calculations have been performed to study rotational excitations for He collision with NCCN. Due to nuclear spin statistics, collision induced transitions have even Δ, while odd Δ transitions are forbidden. The presence of resonances arising from rapid oscillation of cross sections in the low energy region is the result of quasi-bound states in the NCCN-He van der Waals complex. Among all the transitions, Δ = 2 are found to be predominant for excitation. Thereafter, for each transition, the rate coefficients have been calculated which decrease with increasing values of and Δ. The result of this work will be helpful to accurately model the abundance of cyanogen in stellar atmospheres and interstellar gas.

摘要

已研究了星际介质中氰基(NCCN)分子的量子动力学及其与氦的碰撞。使用高水准单参考耦合簇方法与单双和微扰三激发方法以及 aug-cc-pVQZ 基组生成了 NCCN-He 的势能面,范德华复合物。通过极坐标展开,计算了勒让德系数,并将其用于确定碰撞截面。进行了密耦计算以研究氦与 NCCN 的碰撞引起的转动激发。由于核自旋统计,碰撞诱导跃迁具有偶数Δ,而奇数Δ跃迁是禁止的。在低能区截面快速振荡引起的共振的存在是由于 NCCN-He 范德华复合物中的准束缚态。在所有跃迁中,发现Δ=2 对于激发占主导地位。此后,对于每个跃迁,都计算了速率系数,其随和Δ值的增加而减小。这项工作的结果将有助于准确模拟星际气体和恒星大气中氰基的丰度。

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