Rotationally resolved gas-phase spectrum of the (A)over-tilde 2Σ+-(X)over-tilde 2Π3/2 electronic transition for the cyanogen halide radical cation ICN+

被引:0
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作者
Araki, Mitsunori [1 ,2 ]
Ito, Takumi [1 ]
Hoshino, Shoma [1 ]
Tsukiyama, Koichi [1 ]
机构
[1] Tokyo Univ Sci, Fac Sci, Dept Chem, Division1, 1-3 Kagurazaka,Shinju Ku, Tokyo, 1628601, Japan
[2] Tokyo Univ Sci, Res Inst Sci Technol, 2641 Yamazaki, Noda, Chiba 2788510, Japan
关键词
Absorption; ICN+; Electronic transition; Rotational constant; ClCN+; Diffuse Interstellar Bands; EMISSION-SPECTRA; PHOTOELECTRON-SPECTRA; CLCN+; BRCN+; IONS; NEON;
D O I
10.1016/j.jms.2022.111675
中图分类号
O64 [物理化学(理论化学)、化学物理学]; O56 [分子物理学、原子物理学];
学科分类号
070203 ; 070304 ; 081704 ; 1406 ;
摘要
A rotationally resolved gas-phase absorption spectrum of the (A) over tilde (2)Sigma(+)-(X) over tilde (2)Pi(3/2) electronic transition of the cyanogen iodide radical cation ICN+ was observed by cavity ring-down spectroscopy for the first time. This cation was produced in a supersonic planar discharge jet through a mixture of ICN in helium. By the aid of a program for rotational, vibrational and electronic spectra PGOPHER, the rotational constants were determined to be 0.10700 (12) and 0.11002(12) cm(-1) for the (A) over tilde (2)Sigma(+)-(X) over tilde (2)Pi(3/2) electronic states, respectively, and the band origin to be 18262.083(3) cm(-1). The rotational constant ratio beta {= (B'-B '')/B ''}was determined to be -2.8%. The beta values for FCN+, ClCN+, BrCN+, and ICN+ were also evaluated theoretically by CAM-B3LYP/CEP-121G using Gaussian 09W. The rotational profile of the absorption band and its temperature dependence for ClCN+, one of the important candidates for Diffuse Interstellar Bands, were simulated, aiding us in the identification of this cation as in interstellar space.
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页数:5
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