Effective cross sections and rates coefficients derived from collision-induced rotational excitation of HCl\(^{+}(X^{2}\Pi )\) with He(\(^{1}S\)): isotopic effects

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Joseph Ngueleo Baldagui, Théophile Tchakoua, Jean Jules Fifen, Mama Nsangou
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Abstract

In this work, we studied the helium-induced collisional excitation of the radical ion HCl+. Our work focuses on calculating two-dimensional potential energy surfaces (PES) to study the interaction due to the collision between HCl+ and He, and on analyzing the influence of the isotopic effect on cross sections and collision rates. For Ab initio calculations of PES \(^{2}A^{\prime }\) and \(^{2}A^{\prime \prime }\) of HCl+(X\(^{2}\Pi \))-He complex, we used the RCCSD(T)-F12 method with cc-pVQZ-F12 basis sets. These surfaces have been fitted using the Reproducing Kernel Hilbert Space (RKHS) method and were submitted to the close-coupling approach in order to work out the inelastic integral cross sections. Collision cross sections taking into account the fine structures of HCl+ have been performed for kinetic energies up to 3500 cm−1 and the thermal excitation rates for kinetic temperatures varying from \(4K\) up to 400 K. It appears that the difference in the cross section and collisional rate cofficients for the H35Cl+ and H37Cl+ colliding with He was found to be negligeable. In contrast, a significant difference in effective cross-sections and collision rates between HCl+-He and DCl+-He was observed to the extent that it is impossible to make estimation of collision rates of deuterated species from those of the hydrogenated species.

HCl \(^{+}(X^{2}\Pi )\)与He(\(^{1}S\))碰撞诱导旋转激发的有效截面和速率系数:同位素效应
本文研究了氦诱导的HCl+自由基的碰撞激发。我们的工作重点是通过计算二维势能面(PES)来研究HCl+与He碰撞的相互作用,并分析同位素效应对碰撞截面和碰撞速率的影响。对于HCl+(X \(^{2}\Pi \))-He配合物的PES \(^{2}A^{\prime }\)和\(^{2}A^{\prime \prime }\)的从头计算,我们使用了RCCSD(T)-F12方法,cc-pVQZ-F12基集。利用再现核希尔伯特空间(RKHS)方法对这些曲面进行拟合,并采用紧密耦合方法求解非弹性积分截面。考虑HCl+精细结构的碰撞截面在动能高达3500 cm−1和热激发率从\(4K\)到400 K的动力学温度范围内进行了计算。H35Cl+和H37Cl+与He碰撞的截面和碰撞率系数的差异似乎可以忽略不计。相比之下,HCl+-He和DCl+-He在有效截面和碰撞率上存在显著差异,以至于无法从氢化物质中估计氘化物质的碰撞率。
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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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