ROTATIONAL QUENCHING RATE COEFFICIENTS FOR H2 IN COLLISIONS WITH H2 FROM 2 TO 10,000 K

被引:27
|
作者
Lee, T. -G. [1 ,2 ]
Balakrishnan, N. [3 ]
Forrey, R. C. [4 ]
Stancil, P. C. [5 ,6 ]
Shaw, G. [7 ]
Schultz, D. R. [2 ]
Ferland, G. J. [1 ]
机构
[1] Univ Kentucky, Dept Phys & Astron, Lexington, KY 40506 USA
[2] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA
[3] Univ Nevada, Dept Chem, Las Vegas, NV 89154 USA
[4] Penn State Univ, Dept Phys, Reading, PA 19610 USA
[5] Univ Georgia, Dept Phys & Astron, Athens, GA 30602 USA
[6] Univ Georgia, Ctr Simulat Phys, Athens, GA 30602 USA
[7] Tata Inst Fundamental Res, Dept Astron & Astrophys, Bombay 400005, Maharashtra, India
来源
ASTROPHYSICAL JOURNAL | 2008年 / 689卷 / 02期
关键词
ISM: molecules; molecular data; molecular processes;
D O I
10.1086/592560
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Rate coefficients for rotational transitions in H(2) induced by H(2) impact are presented. Extensive quantum mechanical coupled-channel calculations based on a recently published (H(2))(2) potential energy surface were performed. The potential energy surface used here has been demonstrated to be more reliable than surfaces used in previous work. Rotational transition cross sections with initial levels of J <= 8 were computed for collision energies ranging between 10(-4) and 2.5 eV, and the corresponding rate coefficients were calculated for the temperature range 2 <= T <= 10, 000 K. In general, agreement with earlier calculations, which were limited to 100-6000 K, is good, although discrepancies are found at the lowest and highest temperatures. Low-density-limit cooling functions due to para-and ortho-H(2) collisions are obtained from the collisional rate coefficients. Implications of the new results for nonthermal H(2) rotational distributions in molecular regions are also investigated.
引用
收藏
页码:1105 / 1111
页数:7
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