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用于天体化学研究的苯甲腈阳离子的电子光谱和振动光谱

Electronic and vibrational spectroscopy of benzonitrile cation for astrochemical consideration.

作者信息

Daly F C, Douglas-Walker T E, Palotás J, Anstöter C S, Zheng A, Campbell E K

机构信息

School of Chemistry, University of Edinburgh, Joseph Black Building, King's Buildings, David Brewster Road, Edinburgh EH9 3FJ, United Kingdom.

出版信息

J Chem Phys. 2024 Aug 21;161(7). doi: 10.1063/5.0223270.

DOI:10.1063/5.0223270
PMID:39145559
Abstract

The electronic and vibrational spectra of benzonitrile cation, C6H5CN+ (BZN+), in the gas phase at low temperatures are reported. Measurements were carried out using a cryogenic ion trapping apparatus. The mid-infrared spectrum shows a strong CN stretch at 2130 ± 1 cm-1 (4.694 ± 0.002 µm). The electronic spectrum is reported in the range 5040-5750 Å. This covers the forbidden B2B2 ← X2B1 and allowed C2B1 ← X2B1 transitions. The spectrum is dominated by a broad absorption feature at wavelengths shorter than 5250 Å, with the strongest absorption located at 5140 Å. Experimental data are complemented with quantum chemical calculations carried out at the density functional theory and extended multi-configurational quasi-degenerate perturbation theory level. The spectroscopic results are discussed in the context of astronomical observations in the infrared and visible.

摘要

报道了低温气相中苯甲腈阳离子(C6H5CN+,BZN+)的电子光谱和振动光谱。使用低温离子捕获装置进行了测量。中红外光谱显示在2130±1 cm-1(4.694±0.002 µm)处有强烈的CN伸缩振动。电子光谱报道范围为5040 - 5750 Å。这涵盖了禁戒的B2B2←X2B1跃迁和允许的C2B1←X2B1跃迁。光谱主要由波长小于5250 Å处的宽吸收特征主导,最强吸收位于5140 Å。实验数据辅以在密度泛函理论和扩展多组态准简并微扰理论水平上进行的量子化学计算。在红外和可见光天文观测的背景下讨论了光谱结果。

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