Abstract
The random-phase approximation (RPA) is applied to study nondipole corrections to the angular distribution of photoelectrons from the shell of Ne. Calculations of the parameters and arising from interference effects are carried out for the and subshells of Ne in the photon energy range 100–2000 eV. For the shell, the RPA calculations show small effects of correlation near the threshold energy, but are otherwise in agreement with independent-particle approximation (IPA) calculations. The RPA and IPA values of are also in agreement with experiment. For the shell, a small difference between RPA and IPA calculations of the nondipole parameters is found for energies near the threshold; however, both RPA and IPA calculations of the parameter disagree significantly with experimental measurements for photon energies above 1000 eV.
- Received 21 December 1998
DOI:https://doi.org/10.1103/PhysRevA.59.3609
©1999 American Physical Society