Energy levels and transition data of 3p^(6)3d^(8)and 3p^(5)3d^(9)configurations in Fe-like ions(Z=57,60,62,64,65)  

作　　者：Bao-Ling Shi Yi Qin Xiang-Fu Li Bang-Lin Deng Gang Jiang Xi-Long Dou 施宝玲;秦毅;李向富;邓邦林;蒋刚;豆喜龙(Institute of Atomic and Molecular Physics,Sichuan University,Chengdu 610065,China;College of Electrical Engineering,Longdong University,Qingyang 745000,China;College of Geophysics,Chengdu University of Technology,Chengdu 610059,China)

机构地区：[1]Institute of Atomic and Molecular Physics,Sichuan University,Chengdu 610065,China [2]College of Electrical Engineering,Longdong University,Qingyang 745000,China [3]College of Geophysics,Chengdu University of Technology,Chengdu 610059,China

出　　处：《Chinese Physics B》2022年第5期238-244,共7页中国物理B（英文版）

基　　金：The authors express sincere appreciation to professor J?nsson P for providing the GRASP2018 program for free.

摘　　要：Atomic data of highly charged ions(HCIs)offer an attractive means for plasma diagnostic and stars identification,and the investigations on atomic data are highly desirable.Herein,based on the fully relativistic multi-configuration Dirac–Hartree–Fock(MCDHF)method,we have performed calculations of the fine-structure energy levels,wavelengths,transition rates,oscillator strengths,and line strengths for the lowest 21 states of 3p^(6)3d^(8)–3p^(5)3d^(9)electric dipole(E1)transitions configurations in Fe-like ions(Z=57,60,62,64,65).The correlation effects of valence–valence(VV)and core–valence(CV)electrons were systematically considered.In addition,we have taken into account transverse-photon(Breit)interaction and quantum electrodynamics(QED)corrections to treat accurately the atomic state wave functions in the final relativistic configuration interaction(RCI)calculations.Our calculated energy levels and transition wavelengths are in excellent agreement with the available experimental and theoretical results.Most importantly,we predicted some new transition parameters that have not yet been reported.These data would further provide critical insights into better analyzing the physical processes of various astrophysical plasmas.

关 键 词：Fe-like ions energy levels WAVELENGTHS transition rates 

分 类 号：O641.1[理学—物理化学]