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arXiv · 1805.00073

Photoionization of Xe and Rn from the relativistic random-phase theory

Chen-Kai Qiao·Hsin-Chang Chi·Ming-Chien Hsu·Xu-Gen Zheng·Gang Jiang·Shin-Ted Lin·Chang-jian Tang·Keh-Ning Huang
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Abstract

Photoionization cross section $\sigma_{n\kappa}$, asymmetry parameter $\beta_{n\kappa}$, and polarization parameters $\xi_{n\kappa}$, $\eta_{n\kappa}$, $\zeta_{n\kappa}$ 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.

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Chen-Kai Qiao, Hsin-Chang Chi, Ming-Chien Hsu, Xu-Gen Zheng, Gang Jiang, Shin-Ted Lin, Chang-jian Tang, Keh-Ning Huang. 2018-04-30. Photoionization of Xe and Rn from the relativistic random-phase theory. https://doi.org/10.1088/1361-6455%2Fab06d9

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