中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Energy levels and transition rates for helium-like ions with Z=10-36

文献类型:期刊论文

作者Si, R.1,2,3; Guo, X. L.2,3; Wang, K.4; Li, S.5; Yan, J.5,6,7; Chen, C. Y.2,3; Brage, T.1; Zou, Y. M.2,3
刊名ASTRONOMY & ASTROPHYSICS
出版日期2016-08-01
卷号592页码:10
关键词atomic data atomic processes
ISSN号1432-0746
DOI10.1051/0004-6361/201628656
英文摘要Aims. Helium-like ions provide an important X-ray spectral diagnostics in astrophysical and high-temperature fusion plasmas. An interpretation of the observed spectra provides information on temperature, density, and chemical compositions of the plasma. Such an analysis requires information for a wide range of atomic parameters, including energy levels and transition rates. Our aim is to provide a set of accurate energy levels and transition rates for helium-like ions with Z = 10-36. Methods. The second-order many-body perturbation theory (MBPT) was adopted in this paper. To support our MBPT results, we performed an independent calculation using the multiconfiguration Dirac-Hartree-Fock (MCDHF) method. Results. We provide accurate energies for the lowest singly excited 70 levels among 1snl (n <= 6; l <= (n 1)) configurations and the lowest doubly excited 250 levels arising from the K-vacancy 2ln' l' (n' <= 6; l' <= (n' 1)) configurations of helium-like ions with Z = 10 36. Wavelengths, transition rates, oscillator strengths, and line strengths are calculated for the E1, M1, E2, and M2 transitions among these levels. The radiative lifetimes are reported for all the calculated levels. Conclusions. Our MBPT results for singly excited n <= 2 levels show excellent agreement with other elaborate calculations, while those for singly excited n >= 3 and doubly excited levels show significant improvements over previous theoretical results. Our results will be very helpful for astrophysical line identification and plasma diagnostics.
WOS关键词X-RAY-EMISSION ; DIELECTRONIC SATELLITE SPECTRA ; PERTURBATION-THEORY APPROACH ; ELECTRON-IMPACT EXCITATION ; CONFIGURATION-INTERACTION CALCULATIONS ; LYING RESONANCE STATES ; MANY-BODY CALCULATIONS ; SOLAR-FLARE SPECTRA ; HYDROGEN-LIKE IRON ; L-SHELL IONS
资助项目NSAF[11076009] ; National Natural Science Foundation of China[11374062] ; Chinese Association of Atomic and Molecular Data ; Swedish Research Council[2015-04842] ; Chinese National Fusion Project for ITER[2015GB117000] ; Shanghai Leading Academic Discipline Project[B107] ; International Exchange Program Fund for Doctorate Students of Fudan University Graduate School
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000384722600145
出版者EDP SCIENCES S A
资助机构NSAF ; National Natural Science Foundation of China ; Chinese Association of Atomic and Molecular Data ; Swedish Research Council ; Chinese National Fusion Project for ITER ; Shanghai Leading Academic Discipline Project ; International Exchange Program Fund for Doctorate Students of Fudan University Graduate School
源URL[http://119.78.100.186/handle/113462/43528]  
专题中国科学院近代物理研究所
通讯作者Brage, T.
作者单位1.Lund Univ, Dept Phys, Div Math Phys, Box 118, S-22100 Lund, Sweden
2.Fudan Univ, Inst Modern Phys, Dept Nucl Sci & Technol, Shanghai EBIT Lab, Shanghai 200433, Peoples R China
3.Fudan Univ, Appl Ion Beam Phys Lab, Key Lab Minist Educ, Shanghai 200433, Peoples R China
4.Hebei Univ, Coll Phys Sci & Technol, Hebei Key Lab Opt Elect Informat & Mat, Baoding 071002, Peoples R China
5.Inst Appl Phys & Computat Math, Beijing 100088, Peoples R China
6.Peking Univ, Ctr Appl Phys & Technol, Beijing 100871, Peoples R China
7.Shanghai Jiao Tong Univ, Collaborat Innovat Ctr IFSA CICIFSA, Shanghai 200240, Peoples R China
推荐引用方式
GB/T 7714
Si, R.,Guo, X. L.,Wang, K.,et al. Energy levels and transition rates for helium-like ions with Z=10-36[J]. ASTRONOMY & ASTROPHYSICS,2016,592:10.
APA Si, R..,Guo, X. L..,Wang, K..,Li, S..,Yan, J..,...&Zou, Y. M..(2016).Energy levels and transition rates for helium-like ions with Z=10-36.ASTRONOMY & ASTROPHYSICS,592,10.
MLA Si, R.,et al."Energy levels and transition rates for helium-like ions with Z=10-36".ASTRONOMY & ASTROPHYSICS 592(2016):10.

入库方式: OAI收割

来源:近代物理研究所

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