Oscillator strengths for the beryllium isoelectronic sequence

C. D. Lin and W. R. Johnson
Phys. Rev. A 15, 1046 – Published 1 March 1977
PDFExport Citation

Abstract

Oscillator strengths for the outer shells of the beryllium isoelectronic sequence are obtained using the relativistic random phase approximation in which the relativistic effects are included nonperturbatively. The results agree well with other accurate calculations that have been carried out for low-Z elements. For high-Z elements, our results should be very reliable. Both length and velocity formulas are used to calculate the oscillator strengths. The velocity formula is very sensitive to the weak inner-shell coupling, whereas the length formula is not. Inner-shell excitation energies and oscillator strengths are examined and compared with the helium isoelectronic sequence to show the effect of outer-shell screening.

  • Received 19 October 1976

DOI:https://doi.org/10.1103/PhysRevA.15.1046

©1977 American Physical Society

Authors & Affiliations

C. D. Lin* and W. R. Johnson

  • Center for Astrophysics, Harvard College Observatory and Smithsonian Astrophysical Observatory, Cambridge, Massachusetts 02138

  • *Permanent address: Department of Physics, University of Notre Dame, Notre Dame, Ind. 46556.
  • Permanent address: Department of Physics, Kansas State University, Manhattan, Kans. 66506.

References (Subscription Required)

Click to Expand
Issue

Vol. 15, Iss. 3 — March 1977

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
×