CS状态的行列表

IF 8.6 1区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Shilin Hou, Zhengxing Wei
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引用次数: 0

摘要

八种单硫化碳同位素物的旋转-振动谱表计算12C32S、12C33S、12C34S、12C36S、13C32S、13C33S、13C34S、13C36S)的基电子态(X1Σ+)。利用12C32S、12C33S、12C34S和13C32S超过4300个观测到的跃迁频率,通过直接电位拟合方法确定了Born-Oppenheimer击穿效应修正后的经验势函数,用于线表计算。再现的跃迁频率在实验数据的观测不确定度范围内。在具有较大电子组态主动空间的多参考组态相互作用方法/cc-pv5z水平上,用从头算方法计算了偶极矩函数。平衡核分离时的偶极矩与实验结果基本一致。计算强度与2573 K时的实验室观测结果吻合良好。预测了相应的爱因斯坦A系数和振子强度。已经计算了温度高达7500 K的配分函数。谱表可用于不同温度天文环境下CS的光谱测量。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Line Lists for the State of CS
Rotation-vibrational line lists for eight isotopologues of carbon monosulphide (CS; 12C32S, 12C33S, 12C34S, 12C36S,13C32S, 13C33S,13C34S, and 13C36S) in their ground electronic state (X1Σ+) are calculated. An empirical potential function with the corrections of Born–Oppenheimer breakdown effects, which are determined by a direct potential fitting approach using over 4300 observed transition frequencies of 12C32S, 12C33S, 12C34S, and 13C32S, is used in line list calculations. The reproduced transition frequencies are within the observation uncertainties for the isotopologues with experimental data. The dipole moment functions are calculated using an ab initio method at a multireference configuration interaction method/cc-pv5z level with a large active space of electronic configuration. The dipole moment at equilibrium nuclear separation is almost identical to the experimental result. The calculated intensities agree excellently with the laboratory observations at 2573 K. The corresponding Einstein A coefficients and oscillator strengths are predicted. Partition functions for temperatures up to 7500 K have been calculated. The line lists can be used for spectroscopic measurements of CS in astronomical environments of various temperatures.
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来源期刊
Astrophysical Journal Supplement Series
Astrophysical Journal Supplement Series 地学天文-天文与天体物理
CiteScore
14.50
自引率
5.70%
发文量
264
审稿时长
2 months
期刊介绍: The Astrophysical Journal Supplement (ApJS) serves as an open-access journal that publishes significant articles featuring extensive data or calculations in the field of astrophysics. It also facilitates Special Issues, presenting thematically related papers simultaneously in a single volume.
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