DEPOPULATION OF METASTABLE HELIUM BY RADIATIVE ASSOCIATION WITH HYDROGEN AND LITHIUM IONS

被引:6
|
作者
Augustovicova, L. [1 ]
Kraemer, W. P. [2 ]
Soldan, P. [1 ]
机构
[1] Charles Univ Prague, Fac Math & Phys, Dept Chem Phys & Opt, CZ-12116 Prague 2, Czech Republic
[2] Max Planck Inst Astrophys, D-85741 Garching, Germany
来源
ASTROPHYSICAL JOURNAL | 2014年 / 782卷 / 01期
关键词
atomic data; atomic processes; molecular data; molecular processes; LONG-RANGE INTERACTIONS; AB-INITIO; POTENTIAL-ENERGY; EARLY UNIVERSE; MOLECULAR ION; INTERSTELLAR; ABSORPTION; STATE; HEH+; COEFFICIENTS;
D O I
10.1088/0004-637X/782/1/46
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Depopulation of metastable He(2(3)S) by radiative association with hydrogen and lithium ions is investigated using a fully quantal approach. Rate coefficients for spontaneous and stimulated radiative association of the HeH+, HeD+, and LiHe+ molecular ions on the spin-triplet manifold are presented as functions of temperature considering the association to rotational-vibrational states of the lowest triplet electronic states a(3)Sigma(+) and b(3)Sigma(+) from the continuum states of the b(3)Sigma(+) electronic state. Evaluation of the rate coefficients is based on highly accurate quantum calculations, taking into account all possible state-to-state transitions at thermal energies (for spontaneous association) or at higher background energies (stimulated association). As expected, calculations show that the rate coefficients for radiative association to the a state are several orders of magnitude larger than the one for the b state formation. A noticeable effect by blackbody background radiation on the radiative association is only obtained for the b -> b process. Aspects of the formation and abundance of the metastable HeH+(a(3)Sigma(+)) in astrophysical environments are briefly discussed.
引用
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页数:7
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