A theoretical calculation of the absorption spectrum of CH2+

被引:49
作者
Osmann, G
Bunker, PR
Jensen, P
Kraemer, WP
机构
[1] Berg Univ Gesamthsch Wuppertal, FB Theoret Chem 9, D-42097 Wuppertal, Germany
[2] Max Planck Inst Astrophys, D-85740 Garching, Germany
[3] Natl Res Council Canada, Steacie Inst Mol Sci, Ottawa, ON K1A 0R6, Canada
关键词
D O I
10.1016/S0301-0104(97)00173-0
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
The ground (X) over tilde(2)A(1) electronic state of CH2+ is quasilinear with a small barrier to linearity, and at linearity the state becomes degenerate with the (A) over tilde(2)B(1) electronic state forming a (2) Pi(u) state. Because of the nonzero electronic angular momentum the rovibrational basis states belonging to the two electronic states strongly interact due to both the Renner effect and spin-orbit coupling. Tn a previous paper (P. Jensen, M. Brumm, W. P. Kraemer, and P. R. Bunker, J. Mel. Spectrosc. 172 (1995) 194) we calculated the rovibronic energies of the states using ab initio potential energy surfaces that we generated. In the present paper we use the electronic wavefunctions of the previous nb initio calculation to determine the dipole moment and transition moment surfaces, and we develop the theory that allows us to use these to calculate intensities. As a result we now calculate both the positions and intensities of the lines in the absorption spectrum of CH2+, and its deuterated isotopomers, making full allowance for the effects of the Renner interaction and of spin-orbit coupling. We predict the appearance of the absorption spectrum over the whole wavenumber range from 0 cm(-1) to beyond 15 000 cm(-1); this involves only the (X) over tilde and (A) over tilde electronic states. We hope that these results allow experimentalists to search successfully for the features that we predict, and thereby to achieve a better spectroscopic characterization of this important molecular ion. (C) 1997 Elsevier Science B.V.
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页码:33 / 54
页数:22
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