Calculations with spectroscopic accuracy: Energies and transition parameters for lines of fusion interest in Mo XXXIX

Chen, Zhan-Bin; Wang, Kai

doi:10.1016/j.jqsrt.2018.09.025

Cited by 24 publications

(1 citation statement)

References 47 publications

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“…Using at least one of the three methods (RMBPT, MCDHF, and FAC-RCI), we carried out many theoretical studies of excitation energies and E1, M1, E2, M2 transition rates for Kand L-shell ions with Z ≤ 42, such as the ions in the sequences of H-like, [37,38] He-like, [39,40] Be-like, [41][42][43][44][45] B-like, [46][47][48] C-like, [49,50] N-like, [51][52][53][54][55] Olike, [56][57][58][59][60] F-like, [61][62][63] and Ne-like. [64] It is important to provide atomic data for more than just the levels of the lowest configurations in plasma modeling and diagnostics.…”

Section: Resultsmentioning

confidence: 99%

Benchmarking calculations of excitation energies and transition properties with spectroscopic accuracy of highly charged ions used for the fusion plasma and astrophysical plasma

Zhang

Wang

et al. 2023

Chinese Phys. B

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Atomic radiative data such as excitation energies, transition wavelengths, radiative rates, and level lifetimes with high precision are the essential parameters for the abundance analysis, simulation, and diagnostics in fusion and astrophysical plasmas. In this work, we mainly focus on reviewing our two projects performed in the past decade. One is about the ions with Z ≲ 30 that are generally of astrophysical interest, and the other one is about the highly charged krypton (Z = 36) and tungsten (Z = 74) ions that are relevant in research of magnetic confinement fusion. Two different and independent methods, namely, multiconfiguration Dirac–Hartree–Fock (MCDHF) and the relativistic many-body perturbation theory (RMBPT) are usually used in our studies. As a complement/extension to our previous works for highly charged tungsten ions with open M-shell and open N-shell, we also mainly focus on presenting and discussing our complete RMBPT and MCDHF calculations for the excitation energies, wavelengths, electric dipole (E1), magnetic dipole (M1), electric quadrupole (E2), and magnetic quadrupole (M2) transition properties, and level lifetimes for the lowest 148 levels belonging to the 3l 3 configurations in Al-like W61+. We also summarize the uncertainties of our systematical theoretical calculations, by cross-checking/validating our datasets from our RMBPT and MCDHF calculations, and by detailed comparisons with available accurate observations and other theoretical calculations. The data are openly available in Science Data Bank at https://doi.org/10.57760/sciencedb.10569.

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