EXTENDED CALCULATIONS WITH SPECTROSCOPIC ACCURACY: ENERGY LEVELS AND TRANSITION PROPERTIES FOR THE FLUORINE-LIKE ISOELECTRONIC SEQUENCE WITH Z=24-30

被引：39
|
作者：
Si, R. [1 ,2 ]
Li, S. [3 ]
Guo, X. L. [4 ]
Chen, Z. B. [5 ]
Brage, T. [2 ]
Jonsson, P. [6 ]
Wang, K. [7 ]
Yan, J. [3 ,8 ,9 ]
Chen, C. Y. [1 ]
Zou, Y. M. [1 ]
机构：
[1] Fudan Univ, Dept Nucl Sci & Technol, Inst Modern Phys, Shanghai EBIT Lab, Shanghai 200433, Peoples R China
[2] Lund Univ, Dept Phys, Div Math Phys, Box 118, SE-22100 Lund, Sweden
[3] Inst Appl Phys & Computat Math, Beijing 100088, Peoples R China
[4] Second Mil Med Univ, Shanghai Changhai Hosp, Dept Radiotherapy, Shanghai 200433, Peoples R China
[5] Natl Univ Def Technol, Coll Sci, Changsha 410073, Hunan, Peoples R China
[6] Malmo Univ, Grp Mat Sci & Appl Math, SE-20506 Malmo, Sweden
[7] Hebei Univ, Coll Phys Sci & Technol, Hebei Key Lab Opt Elect Informat & Mat, Baoding 071002, Peoples R China
[8] Peking Univ, Ctr Appl Phys & Technol, Beijing 100871, Peoples R China
[9] Shanghai Jiao Tong Univ, CICIFSA, Shanghai 200240, Peoples R China
来源：
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2016年 / 227卷 / 02期
基金：
中国国家自然科学基金; 瑞典研究理事会;
关键词：
atomic data; atomic processes; PERTURBATION-THEORY APPROACH; COMBINED CONFIGURATION-INTERACTION; X-RAY-SPECTRA; ELECTRON-IMPACT EXCITATION; L-SHELL IONS; F-LIKE IONS; ATOMIC DATA; DIELECTRONIC RECOMBINATION; SYSTEMATIC CALCULATIONS; LABORATORY MEASUREMENTS;
D O I：
10.3847/0067-0049/227/2/16
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We have performed extensive multiconfiguration Dirac-Hartree-Fock calculations and second-order many-body perturbation calculations for F-like ions with Z = 24-30. Energy levels and transition rates for electric dipole (E1), electric-quadrupole (E2), electric-octupole (E3), magnetic dipole (M1), and magnetic-quadrupole (M2) transitions, as well as radiative lifetimes, are provided for the lowest 200 levels belonging to the 1s(2)2s(2)2p(5), 1s(2)2s2p(6), 1s(2)2s(2)2p(4)3l, 1s(2)2s2p(5)3l, 1s(2)2p(6)3l, and1s(2)2s(2)2p(4)4l configurations of each ion. The results from the two sets of calculations are in excellent agreement. Extensive comparisons are also made with other theoretical results and observed data from the CHIANTI and NIST databases. The present energies and wavelengths are believed to be accurate enough to aid line identifications involving the n = 3 and n = 4 configurations, for which observations are largely missing. The calculated wavelengths and transition data will be useful in the modeling and diagnostics of astrophysical and fusion plasmas.
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页数：17
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