Structure of the Se4 Isomers─An Ab Initio Study.

IF 2.8 2区 化学 Q3 CHEMISTRY, PHYSICAL The Journal of Physical Chemistry A Pub Date : 2025-01-09 Epub Date: 2024-12-30 DOI:10.1021/acs.jpca.4c07650
Lidan Xiao, Yahong Liu, Yi Lian, Boris F Minaev, Hans Ågren, Bing Yan
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Abstract

This study investigates the equilibrium geometries of four different Se4 isomers using the coupled cluster single and double perturbative (CCSD(T)) method, extrapolating to the complete basis sets. The ground-state geometry of the Se4 isomer with the C2v structure (2.8715 Å, 2.1750 Å, and 88.4°) is found to be very close to other theoretical values (2.910 Å, 2.224 Å, and 90.0°) for the Se═Se and Se-Se bond lengths and valence angle. Additionally, the adiabatic electron affinity, vertical electron affinity, and vertical ionization energy are calculated. The multireference configuration interaction method was used to calculate transitions from the singlet ground state to some excited counterparts, including the vertical excitation energy, oscillator strength, and main electronic configuration. The predicted wavelengths of electronic transitions to 11Bu, 11Au with C2h symmetry, and 11B1 state with the C2V symmetry could match the experimental NIR absorption band at 710-850 nm. These transitions and electronic properties may provide insights into the role of selenium in astrophysical environments, where 74Se in the solar system has been confirmed to originate from the supernova explosion process. The theoretical results offer a deeper understanding of Se4 electronic and geometric structures while also providing crucial spectroscopic data that could aid in the identification of selenium-containing molecules in extraterrestrial environments.

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Se4异构体的结构─从头算研究。
本研究使用耦合簇单、双摄动(CCSD(T))方法研究了四种不同Se4异构体的平衡几何形状,外推到完整的基集。具有C2v结构的Se4异构体的基态几何(2.8715 Å、2.1750 Å和88.4°)与Se = Se和Se-Se键长和价角的其他理论值(2.910 Å、2.224 Å和90.0°)非常接近。此外,还计算了电子的绝热亲和、垂直电子亲和和垂直电离能。采用多参考组态相互作用方法计算了从单重态基态到激发态的跃迁,包括垂直激发能、振子强度和主电子组态。电子跃迁到具有C2h对称性的11Bu、11Au态和具有C2V对称性的11B1态的预测波长与实验近红外吸收带在710 ~ 850 nm处相匹配。这些转变和电子性质可能为硒在天体物理环境中的作用提供见解,其中太阳系中的74Se已被证实起源于超新星爆炸过程。理论结果提供了对Se4电子和几何结构的更深入理解,同时也提供了关键的光谱数据,可以帮助识别地外环境中的含硒分子。
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来源期刊
The Journal of Physical Chemistry A
The Journal of Physical Chemistry A 化学-物理:原子、分子和化学物理
CiteScore
5.20
自引率
10.30%
发文量
922
审稿时长
1.3 months
期刊介绍: The Journal of Physical Chemistry A is devoted to reporting new and original experimental and theoretical basic research of interest to physical chemists, biophysical chemists, and chemical physicists.
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