Absolute measurements of state-to-state rotational energy transfer between CO and H2 at interstellar temperatures

被引:5
|
作者
Labiad, Hamza [1 ]
Fournier, Martin [1 ]
Mertens, Laura A. [1 ,2 ]
Faure, Alexandre [3 ]
Carty, David [4 ,5 ]
Stoecklin, Thierry [6 ]
Jankowski, Piotr [7 ]
Szalewicz, Krzysztof [8 ]
Le Picard, Sebastien D. [1 ]
Sims, Ian R. [1 ]
机构
[1] Univ Rennes, CNRS, IPR Inst Phys Rennes, UMR 6251, F-35000 Rennes, France
[2] CALTECH, Div Chem & Chem Engn, Pasadena, CA 91125 USA
[3] Univ Grenoble Alpes, IPAG Inst Planetol & Astrophys Grenoble, CNRS, F-38000 Grenoble, France
[4] Univ Durham, Joint Quantum Ctr Durham Newcastle, Dept Phys, South Rd, Durham DH1 3LE, England
[5] Univ Durham, Joint Quantum Ctr Durham Newcastle, Dept Chem, South Rd, Durham DH1 3LE, England
[6] Univ Bordeaux, Inst Sci Mol, F-33405 Talence, France
[7] Nicolaus Copernicus Univ Torun, Fac Chem, Gagarina 7, PL-87100 Torun, Poland
[8] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA
基金
美国国家科学基金会;
关键词
COLLISIONS; HE; EXCITATION; AR;
D O I
10.1103/PhysRevA.105.L020802
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Experimental measurements and theoretical calculations of state-to-state rate coefficients for rotational energy transfer of CO in collision with H-2 are reported at the very low temperatures prevailing in dense interstellar clouds (5-20 K). Detailed agreement between quantum state-selected experiments performed in cold supersonic flows using time-resolved infrared-vacuum-ultraviolet double-resonance spectroscopy and close-coupling quantum scattering calculations confirms the validity of the calculations for collisions between the two most abundant molecules in the interstellar medium.
引用
收藏
页数:6
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