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Featured researches published by R. Si.


Journal of Physics B | 2015

Relativistic many-body calculations on wavelengths and transition probabilities for forbidden transitions within the

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

3{{{\rm d}}^{k}}

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

ground configurations in Co- through K-like ions of hafnium, tantalum, tungsten and gold

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

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

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

EXTENDED RELATIVISTIC CONFIGURATION INTERACTION AND MANY-BODY PERTURBATION CALCULATIONS OF SPECTROSCOPIC DATA FOR THE N 6 CONFIGURATIONS IN Ne-LIKE IONS BETWEEN Cr XV AND Kr XXVII

R. Si; X. L. Guo; K. Wang; S. Li; J. Yan; C. Y. Chen; Tomas Brage; Yaming Zou

,


Journal of Physics B | 2015

CALCULATIONS WITH SPECTROSCOPIC ACCURACY: ENERGIES AND TRANSITION RATES IN THE NITROGEN ISOELECTRONIC SEQUENCE FROM Ar XII TO Zn XXIV

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

Energy levels and transition rates for helium-like ions with Z = 10–36

X. L. Guo; Jon Grumer; Tomas Brage; R. Si; Chong-Yang Chen; Per Jönsson; K. Wang; Jun Yan; R. Hutton; Yaming Zou

,


Astrophysical Journal Supplement Series | 2017

Energy levels and transition rates for Mg-like Kr XXV

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

Energy levels and radiative data for Kr-like W38+ from MCDHF and RMBPT calculations

Z.L. Zhao; K. Wang; S. Li; R. Si; C.Y. Chen; Z.B. Chen; J. Yan; Yu. Ralchenko

,


Astronomy and Astrophysics | 2015

Extended Calculations of Spectroscopic Data : Energy Levels, Lifetimes, and Transition Rates for O-like Ions from Cr XVII to ZnXXIII

S. Li; J. Yan; C. Y. Li; R. Si; X. L. Guo; Min Huang; C.Y. Chen; Yunzeng Zou

2s^2 2p^5 4l

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X. L. Guo

Second Military Medical University

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