Apparent change of the 3C/3D line intensity ratio in neonlike ions

被引:4
作者
Yang, Zhihao [1 ]
He, Zhencen [1 ,2 ]
Xiong, Gang [2 ,3 ]
Yao, Ke [2 ]
Yang, Yang [2 ]
Wei, Baoren [2 ]
Zou, Yaming [2 ]
Wu, Zhongwen [4 ,5 ]
Tian, Ziqiang [4 ]
Ma, Yulong [4 ]
Wu, Chensheng [6 ]
Gao, Xiang [6 ,7 ]
Hu, Zhimin [1 ]
机构
[1] Sichuan Univ, Inst Nucl Sci & Technol, Minist Educ, Key Lab Radiat Phys & Technol, Chengdu 610064, Peoples R China
[2] Fudan Univ, Key Lab Nucl Phys & Ion Beam Applicat MOE, Shanghai 200433, Peoples R China
[3] China Acad Engn Phys, Laser Fus Res Ctr, Mianyang 6219, Sichuan, Peoples R China
[4] Northwest Normal Univ, Coll Phys & Elect Engn, Key Lab Atom & Mol Phys & Funct Mat Gansu Prov, Lanzhou 730070, Peoples R China
[5] Helmholtz Inst Jena, D-07743 Jena, Germany
[6] Inst Appl Phys & Computat Math, Beijing 100088, Peoples R China
[7] Beijing Computat Sci Res Ctr, Beijing 100193, Peoples R China
基金
中国国家自然科学基金;
关键词
LABORATORY MEASUREMENTS; FE-XVII; CONFIGURATION-INTERACTION; CROSS-SECTIONS; TRANSITIONS; EXCITATION; CHANDRA; SPECTRA; DENSITY; CAPELLA;
D O I
10.1364/OE.458597
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The resonance 3C ([(2p(5))(1/2)3d(3/2)](J=1)->[2p(6)](J=0)) to intercombination 3D ([(2p(5))(3/2) 3d(5/2)](J=1)->[2p(6)](J=0)) line intensity ratio of neonlike ions has been studied. The measured line intensity ratio for neonlike Xe44+ ions shows an apparent change, which is reproduced by the calculations using the relativistic configuration interaction plus many-body perturbation theory. It is clearly elucidated that the change in the 3C/3D line intensity ratio is caused by strong configuration mixing between the upper levels of the 3D and 3F ([(2p(5))(1/2)3s](J=1)->[2p(6)](J=0)) lines. The present measurement allows us to discuss the 3C/3D line intensity ratio for the highest-Z ions hitherto, which suggests that the experiment-theory discrepancy in the 3C/3D line intensity ratio of neonlike ions diminishes with increasing atomic number Z and further trends to vanish at higher-Z ions. Furthermore, the present study provides benefits to better understand configuration mixing effect in the radiative opacity of hot plasmas. (C) 2022 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement
引用
收藏
页码:25326 / 25338
页数:13
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