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

被引:28
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
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
相关论文
共 36 条
[1]   A STABLE LINEAR REFERENCE POTENTIAL ALGORITHM FOR SOLUTION OF THE QUANTUM CLOSE-COUPLED EQUATIONS IN MOLECULAR-SCATTERING THEORY [J].
ALEXANDER, MH ;
MANOLOPOULOS, DE .
JOURNAL OF CHEMICAL PHYSICS, 1987, 86 (04) :2044-2050
[2]   H2 pure rotational lines in the Orion Bar [J].
Allers, KN ;
Jaffe, DT ;
Lacy, JH ;
Draine, BT ;
Richter, MJ .
ASTROPHYSICAL JOURNAL, 2005, 630 (01) :368-380
[3]  
[Anonymous], MOLSCAT VERSION 14
[4]   A far UV study of interstellar gas towards HD 34078:: High excitation H2 and small scale structure [J].
Boissé, P ;
Le Petit, F ;
Rollinde, E ;
Roueff, E ;
des Forêts, GP ;
Andersson, BG ;
Gry, C ;
Felenbok, P .
ASTRONOMY & ASTROPHYSICS, 2005, 429 (02) :509-523
[5]   An accurate analytic H4 potential energy surface [J].
Boothroyd, AI ;
Martin, PG ;
Keogh, WJ ;
Peterson, MJ .
JOURNAL OF CHEMICAL PHYSICS, 2002, 116 (02) :666-689
[6]   Near-IR fluorescent molecular hydrogen emission from NGC 2023 [J].
Burton, MG ;
Howe, JE ;
Geballe, TR ;
Brand, PWJL .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, 1998, 15 (02) :194-201
[7]   ROTATIONALLY INELASTIC-COLLISIONS BETWEEN H-2-MOLECULES IN INTERSTELLAR MAGNETOHYDRODYNAMIC SHOCKS [J].
DANBY, G ;
FLOWER, DR ;
MONTEIRO, TS .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1987, 226 (03) :739-745
[8]   An accurate H2-H2 interaction potential from first principles (vol 112, pg 4465, 2000) [J].
Diep, P ;
Johnson, JK .
JOURNAL OF CHEMICAL PHYSICS, 2000, 113 (08) :3480-3481
[9]   PHOTO-ELECTRIC HEATING OF INTER-STELLAR GAS [J].
DRAINE, BT .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1978, 36 (04) :595-619
[10]   CLOUDY 90: Numerical simulation of plasmas and their spectra [J].
Ferland, GJ ;
Korista, KT ;
Verner, DA ;
Ferguson, JW ;
Kingdon, JB ;
Verner, EM .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1998, 110 (749) :761-778