Influence of the Energy of the Incident Photon on Satellite Intensities in Photoelectron Spectra of the Rare Gases
- 11 June 1984
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 52 (24) , 2138-2140
- https://doi.org/10.1103/physrevlett.52.2138
Abstract
The influence of the energy of the incident photon on the statellite structure associated with ionization in the outer shell of the heavier rare gases is calculated. When the photon energy decreases from 200 to 50 eV, an increase in satellite intensity of about 30% is predicted for Ar. This prediction agrees, within the experimental accuracy, with recent observations. Similar behavior is predicted for Kr and Xe.
Keywords
This publication has 19 references indexed in Scilit:
- The relativistic time-dependent local-density approximationJournal of Physics B: Atomic and Molecular Physics, 1984
- Ionic-configuration-interaction effects on Xe-subshell photoionization processesPhysical Review A, 1983
- The importance of continuum d states for the interaction nsnp6↔ns4d in the rare gasesJournal of Physics B: Atomic and Molecular Physics, 1983
- Angular distribution of Xe5s→εp photoelectrons: a sensitive test of theoryJournal of Physics B: Atomic and Molecular Physics, 1983
- Angular Distribution of XePhotoelectrons: Disagreement between Experiment and TheoryPhysical Review Letters, 1983
- Photoionisation of helium to He+(n=2)Journal of Physics B: Atomic and Molecular Physics, 1980
- Photoionization of the outer shells of neon, argon, krypton, and xenon using the relativistic random-phase approximationPhysical Review A, 1979
- (e, 2e) spectroscopyPhysics Reports, 1976
- Photoionization of helium above the n=2 thresholdJournal of Physics B: Atomic and Molecular Physics, 1972
- Lamb Shift Excitation Energy in the Ground State of the Helium AtomPhysical Review B, 1962