Predissociations in 0u+ and 1g states of K2

被引:15
|
作者
Bergeman, T [1 ]
Julienne, PS
Williams, CJ
Tiesinga, E
Manaa, MR
Wang, H
Gould, PL
Stwalley, WC
机构
[1] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA
[2] Natl Inst Stand & Technol, Atom Phys Div, Gaithersburg, MD 20899 USA
[3] Lawrence Livermore Natl Lab, Energet Mat Ctr, Livermore, CA 94551 USA
[4] Aerosp Corp, Elect & Photon Lab, Los Angeles, CA 90009 USA
[5] Univ Connecticut, Dept Phys, Storrs, CT 06269 USA
来源
JOURNAL OF CHEMICAL PHYSICS | 2002年 / 117卷 / 16期
关键词
D O I
10.1063/1.1508375
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
Recently Wang, Gould, and Stwalley [Phys. Rev. Lett. 80, 476 (1998)] showed by exciting atomic fragments that predissociation occurs in the 1(g) and 0(u)(+) states of K-2. In this study, we supplement the interpretation given in the original report with a more detailed discussion. The calculations presented here use discrete variable representation, close coupling, and semiclassical methods, and incorporate an ab initio calculation of diagonal and off-diagonal spin-orbit elements. The predicted predissociation widths for the 1(g) state are too narrow to be observed directly, but may be correlated with the strength of the spectral lines observed by exciting atomic fragments. The missing v=90 level of the 1(g) state in the observed fragmentation spectrum, where the predissociation rate is calculated to be nearly maximum, is attributed to a node in the absorption line strength close to this vibrational level. Since the available information on K-2 electronic states (despite recent progress) gives inadequate information on the inner walls of the A state and especially of the b state, calculations of predissociation in the 0(u)(+) state can give only a range of possible widths. We fit widths to 0(u)(+) spectral lines observed by monitoring trap loss. The fitted experimental widths are significantly larger than the maximum calculated predissociation widths, suggesting that there was line broadening associated with the laser power required for the observation. (C) 2002 American Institute of Physics.
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收藏
页码:7491 / 7505
页数:15
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