Abstract
In this work, we calculated the fluorescence and Coster-Kronig yields for the shell and the and subshells of Ne, Ar, Kr, Xe, Rn, and Uuo , using a Dirac-Fock model which provides a better description of the electron-electron interaction than previous approaches, and is suitable to handle superheavy elements. The results are compared with available data from other authors. In what concerns Ne, Ar, Kr, Xe, and Rn shells, the obtained results are in very good agreement with the adopted values of Krause [25] and with experiment when available. For the subshells, our results are in line with existing ones. For the subshells and for all shells of Uuo there are no previous experimental and theoretical results to compare to our calculations.
- Received 27 March 2015
DOI:https://doi.org/10.1103/PhysRevA.91.052507
©2015 American Physical Society