Department of Physics and Astronomy: Publications and Other Research
Date of this Version
November 1983
Abstract
Recent measurements of the 5s-subshell photoelectron angular distribution of xenon have found larger values for the asymmetry parameter β in the region of the 5s-subshell cross-section minimum than predicted by relativistic random-phase-approximation calculations. Final-state ionic configuration interaction is adduced as a possible explanation for this and other discrepancies.
Comments
Published by American Physical Society. Phys. Rev. A 28, 3143 (1983). http://pra.aps.org. Copyright © 1983 American Physical Society. Permission to use.