Wavelength dependence of the photoelectron angular distributions of the rare gases

J. L. Dehmer, W. A. Chupka, J. Berkowitz, and W. T. Jivery
Phys. Rev. A 12, 1966 – Published 1 November 1975
PDFExport Citation

Abstract

Photoelectron angular distributions for the valence p shells of the rare gases have been measured up to a photon energy of 40.8 eV (48.4 eV for Ne) using resonance radiation from a hollow-cathode discharge lamp. This work extends the range of existing absolute measurements on Ne, Kr, and Xe. Comparison with HartreeFock and RPAE (random-phase approximation with exchange) calculations indicates excellent agreement for Ne. However, the present results, particularly for Xe, add to earlier evidence that data for Ar, Kr, and Xe show systematic deviations from theory, especially at the higher photoelectron kinetic energies. For Kr and Xe, we report asymmetry parameters separately for processes leading to the P32,122 spin-orbit states of the residual ion. The Xe results indicate that β32β12 is positive for λ461 Å, but changes sign in the range λ350400 Å. At 304 Å, β32β12=0.30, which agrees with a recent calculation based on the Dirac-Slater model.

  • Received 17 July 1975

DOI:https://doi.org/10.1103/PhysRevA.12.1966

©1975 American Physical Society

Authors & Affiliations

J. L. Dehmer, W. A. Chupka*, J. Berkowitz, and W. T. Jivery

  • Argonne National Laboratory, Argonne, Illinois 60439

  • *Present address: Dept. of Chemistry, Yale University, New Haven, Conn. 06520.

References (Subscription Required)

Click to Expand
Issue

Vol. 12, Iss. 5 — November 1975

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review A

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×