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.

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页码：56 / 58

页数：3

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