The formation of H2O from the radiative association of O and H2

被引：7
作者：
Talbi, Dahbia [1 ,2 ]
Bacchus-Montabonel, Marie-Christine [3 ,4 ]
机构：
[1] Univ Montpellier 2, Grp Rech Astron & Astrophys Languedoc, F-34095 Montpellier, France
[2] CNRS, F-34095 Montpellier, France
[3] Univ Lyon, Spectrometrie Ion & Mol Lab, F-69622 Villeurbanne, France
[4] CNRS, F-69622 Villeurbanne, France
来源：
CHEMICAL PHYSICS LETTERS | 2010年 / 485卷 / 1-3期
关键词：
POTENTIAL-ENERGY SURFACE; AB-INITIO; WATER; SPECTRA; STATES;
D O I：
10.1016/j.cplett.2009.12.045
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 formation of H2O((1)A(1)) from the radiative association of oxygen and H-2 has been investigated by accurate quantum chemistry calculations. The rate constant calculations have been undertaken for the IR radiative stabilisation of the (1)A(1) H2O complex formed at the O(D-1) and H-2 dissociation limit. The formation of H2O((1)A(1)) from the radiative association of O and H-2 is discussed within the astrophysical context. (C) 2009 Elsevier B. V. All rights reserved.
引用
收藏
页码：56 / 58
页数：3
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