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Photoionization of the outer shells of radon and radium: Relativistic random-phase approximation for high-z atoms. (Reannouncement with new availability information)

Technical Report ·
OSTI ID:177473
Photoionization cross sections, branching ratios, and photoelectron angular distributions have been calculated for Ra (Z = 88) 7s, 6p, 6s, 5d, and 5p, and Rn (Z = 86) 6p, 6s, 5d, and 5p subshells within the framework of the relativistic random-phase approximation, including coupling between all of the relativistic channels arising from these subshells, in an effort to elucidate the interplay between relativistic and interchannel interactions at high Z where no experiments are extant. The results show that, aside from inducing structure in subshell cross sections, relativistic plus interchannel effects dominate the photoelectron angular-distribution asymmetry parameter and the branching ratio between spin-orbit doublets largely through the relativistic splitting of Cooper minima. This qualitatively confirms effects predicted by simple central-field calculations. Detailed explanations of the reasons for each of the structures are presented.
Research Organization:
Georgia State Univ., Atlanta, GA (United States). Dept. of Physics
OSTI ID:
177473
Report Number(s):
AD-A--255458/2/XAB
Country of Publication:
United States
Language:
English

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