碘化碲阳离子光谱特性的理论研究

IF 1.4 4区 物理与天体物理 Q4 PHYSICS, ATOMIC, MOLECULAR & CHEMICAL Journal of Molecular Spectroscopy Pub Date : 2024-10-01 DOI:10.1016/j.jms.2024.111951
Nan Fang , Chuan-Yu Zhang , Ming-Jie Wan , Xiao-Peng Huang
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引用次数: 0

摘要

分子势能函数在许多领域发挥着重要作用。本文利用icMRCI + Q方法计算了TeI+体系22个Λ-S态和51个Ω态的势能和偶极矩。计算 TeI+ 系统时采用了两种基集(AVQZ-PP 和 AWCVQZ-PP),结果表明 AVQZ-PP 基集得到的结果更为精确。因此,本文中的所有计算均基于该基础集。此外,为了确保结果的准确性,还对同一主族内分子离子的基态和两个激发态的光谱参数进行了比较。考虑到自旋轨道耦合的重大影响(如计算的 SO 矩阵元素所示),我们的讨论将主要集中在避免 Ω 态的交叉上。最后,我们根据 TeI+ 分子 X3Σ0+-↔11Σ0++ 之间的转变数据计算了这两种状态之间的弗朗克-康顿因子、爱因斯坦系数和辐射寿命。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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Theoretical study on the spectrum properties of tellurium iodide cation
The molecular potential energy function plays an important role in many fields. In this paper, the icMRCI + Q method was utilized to compute the potential energy and dipole moments for 22 Λ-S states and 51 Ω states of the TeI+ system. Two basis sets (AVQZ-PP and AWCVQZ-PP) were employed to compute the TeI+ system, with the results indicating that the AVQZ-PP basis set yielded more accurate results. Therefore, all calculations in this paper are based on this basis set. Furthermore, to ensure the accuracy of the results, a comparison was conducted on the spectral parameters of the ground state and two excited states of the molecular ion within the same main group. Given the significant impact of spin–orbit coupling, as indicated by the calculated SO matrix elements, our discussion will predominantly center on the avoidance of crossovers in the Ω states. Finally, the Franck-Condon factors, Einstein coefficients and radiative lifetime between these two states were calculated from the data of the transition between the X3Σ0+-11Σ0++ of the TeI+ molecule.
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来源期刊
CiteScore
2.70
自引率
21.40%
发文量
94
审稿时长
29 days
期刊介绍: The Journal of Molecular Spectroscopy presents experimental and theoretical articles on all subjects relevant to molecular spectroscopy and its modern applications. An international medium for the publication of some of the most significant research in the field, the Journal of Molecular Spectroscopy is an invaluable resource for astrophysicists, chemists, physicists, engineers, and others involved in molecular spectroscopy research and practice.
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