R. Si
Fudan University
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Publication
Featured researches published by R. Si.
Journal of Physics B | 2015
X. L. Guo; Min Huang; J. Yan; S. Li; R. Si; C Y Li; C.Y. Chen; Y.S. Wang; Yunzeng Zou
Wavelengths and transition probabilities have been computed for forbidden lines within the 3dk(k = 1-9) ground configurations in ions of hafnium, tantalum, tungsten and gold, employing the second-order relativistic many-body perturbation theory (RMBPT). For comparison, the relativistic configuration-interaction (RCI) calculations have also been performed. Comparing to the previously published theoretical wavelengths and the present RCI ones, the present RMBPT results are in much better agreement with the experimental values measured recently by using the electron beam ion trap facility, reproducing these observed wavelengths to within 0.2% for all transitions only with one exception. In addition, it removes dramatically the systematic underestimation/overestimation for shorter/longer wavelengths existing in the present RCI and other calculations.
Astrophysical Journal Supplement Series | 2016
R. Si; S. Li; X. L. Guo; Z. B. Chen; Tomas Brage; Per Jönsson; K. Wang; Jun Yan; ChangYan Chen; Yaming Zou
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 1s22s22p5, 1s22s22p6, 1s22s22p43l, 1s22s2p23l, 1s22p63l, and 1s22s22p44l 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. (Less)
Astrophysical Journal Supplement Series | 2016
K. Wang; Zhan Bin Chen; R. Si; Per Jönsson; Jörgen Ekman; Xue Ling Guo; S. Li; Fei Yun Long; W. Dang; X.H. Zhao; R. Hutton; C. Y. Chen; Jun Yan; Xu Yang
Level energies, wavelengths, electric dipole, magnetic dipole, electric quadrupole, and magnetic quadrupole transition rates, oscillator strengths, and line strengths from combined relativistic configuration interaction and many-body perturbation calculations are reported for the 201 fine-structure states of the
Astrophysical Journal Supplement Series | 2016
K. Wang; R. Si; W. Dang; Per Jönsson; Xue Ling Guo; S. Li; Zhan Bin Chen; Hong Zhang; Fei Yun Long; Hai Tao Liu; R. Hutton; C. Y. Chen; Jun Yan
2s^2 2p^6
Astronomy and Astrophysics | 2016
R. Si; X. L. Guo; K. Wang; S. Li; J. Yan; C. Y. Chen; Tomas Brage; Yaming Zou
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Journal of Physics B | 2015
R. Si; X. L. Guo; J. Yan; C Y Li; S. Li; Min Huang; C.Y. Chen; Yunzeng Zou
2s^2 2p^5 3l
Journal of Physics B | 2016
X. L. Guo; Jon Grumer; Tomas Brage; R. Si; Chong-Yang Chen; Per Jönsson; K. Wang; Jun Yan; R. Hutton; Yaming Zou
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Astrophysical Journal Supplement Series | 2017
K. Wang; Per Jönsson; Jörgen Ekman; Gediminas Gaigalas; Michel Godefroid; R. Si; Z. B. Chen; S. Li; C. Y. Chen; Jun Yan
2s 2p^6 3l
Atomic Data and Nuclear Data Tables | 2018
Z.L. Zhao; K. Wang; S. Li; R. Si; C.Y. Chen; Z.B. Chen; J. Yan; Yu. Ralchenko
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Astronomy and Astrophysics | 2015
S. Li; J. Yan; C. Y. Li; R. Si; X. L. Guo; Min Huang; C.Y. Chen; Yunzeng Zou
2s^2 2p^5 4l