Theoretical investigation of electron capture processes in slow O7+-H collisions

被引:0
|
作者
Lin, Xiaohe [1 ]
Wang, Kun [5 ]
Wang, Yu [2 ,4 ]
Liu, Ling [2 ]
Wu, Yong [2 ,3 ]
Lin, Minjuan [6 ]
Li, Rui [6 ]
Wang, J. G. [2 ]
机构
[1] Space Engn Univ, Fac Fdn, 1 Bayi Rd, Beijing 101416, Peoples R China
[2] Inst Appl Phys & Computat Math, Data Ctr High Energy Dens Phys, POB 8009,6 Huayuan Rd, Beijing 100088, Peoples R China
[3] Peking Univ, Ctr Appl Phys & Technol, HEDPS, 22 Huaqing Jiayuan,Chengfu Rd, Zhongguancun St, Beijing 100084, Peoples R China
[4] Beijing Inst Technol, Sch Phys, 5 Zhongguancun South St, Beijing 100081, Peoples R China
[5] Shanxi Univ, Inst Environm Sci, 92 Wucheng Rd, Taiyuan 030006, Shanxi, Peoples R China
[6] Qiqihar Univ, Coll Sci, Dept Phys, 42 Wenhua St, Qiqihar 161006, Heilongjiang Pr, Peoples R China
基金
中国国家自然科学基金;
关键词
solar wind; atomic data; scattering; MATRIX-ELEMENTS; CHARGE-TRANSFER; CROSS-SECTIONS; IONS; IONIZATION; HE;
D O I
10.1051/0004-6361/202347302
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. The total and n-, l-, and S -resolved single-electron-capture cross sections for the collisions of O7+ with atomic hydrogen are studied in the energy region from 10(-3)eV u(-1)-5keV u(-1).Methods. These state-selective cross sections were calculated by employing the full quantum-mechanical molecular-orbital close-coupling (QMOCC) method. The ab initio multireference single- and double-excitation configuration interaction approach, with optimized atomic basis sets to accurately describe the highly excited states, was used to obtain the adiabatic potentials and the radial and rotational coupling matrix elements that are required in the QMOCC calculation.Results. Our results are compared with other available theoretical and experimental data. The n = 5 manifold is the dominant reaction channel for the chasrge-transfer process for this collision system over the entire energy range, and our results agree better with the experimental data than the other theoretical results in the energy region in which they overlap because we included the necessary highly excited states in the expansion basis set. These charge-exchange cross-section data are useful for understanding and modeling the X-ray emission in astrophysical environments.
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页数:7
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