Photoionization of Xe and Rn from the relativistic random-phase theory
arXiv:1805.00073 · doi:10.1088/1361-6455/ab06d9
Abstract
Photoionization cross section , asymmetry parameter , and polarization parameters , , of Xe and Rn are calculated in the fully relativistic formalism. To deal with the relativistic and correlation effects, we adopt the relativistic random-phase theory with channel couplings among different subshells. Energy ranges for giant \emph{d}-resonance regions are especially considered.
arXiv comment14 pages, 10 figures, 1 table, 2 appendix; V2 Corrections for author information and grants numbers; V3 Majar revision: add 2 figures and an appendix; V4 Minor revision; V5 Minor revision; V6 accepted version: add one more appendix
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