Excitation and charge transfer in low-energy hydrogen atom collisions with neutral manganese and titanium

被引:8
作者
Grumer, J. [1 ]
Barklem, P. S. [1 ]
机构
[1] Uppsala Univ, Dept Phys & Astron, Theoret Astrophys, Box 516, S-75120 Uppsala, Sweden
基金
瑞典研究理事会;
关键词
atomic data; atomic processes; line: formation; Sun: abundances; stars: abundances; IONIZATION; RECOMBINATION; COEFFICIENTS; LTE;
D O I
10.1051/0004-6361/201937434
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Data for inelastic processes due to hydrogen atom collisions with manganese and titanium are needed for accurate modeling of the corresponding spectra in late-type stars. In this work excitation and charge transfer in low-energy Mn+H and Ti+H collisions have been studied theoretically using a method based on an asymptotic two-electron linear combination of an atomic orbitals model of ionic-covalent interactions in the neutral atom-hydrogen-atom system, together with the multichannel Landau-Zener model to treat the dynamics. Extensive calculations of charge transfer (mutual neutralization, ion-pair production), excitation and de-excitation processes in the two collisional systems are carried out for all transitions between covalent states dissociating to energies below the first ionic limit and the dominating ionic states. Rate coefficients are determined for temperatures in the range 1000-20 000 K in steps of 1000 K. Like for earlier studies of other atomic species, charge transfer processes are found to lead to much larger rate coefficients than excitation processes.
引用
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页数:9
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