Relativistic Calculations of N-Shell X-Ray Emission Rates

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Abstract

Radiative transition probabilities filling vacancies in atomic N subshells have been calculated relativistically for six elements with atomic number between Z= 66 and 92. The relativistic Hartree-Fock-Slater wave functions are used and contributions from all multipoles are included. The results are compared with those of nonrelativistic calculations. Relativistic effects are found to be significant for the transition involving N1- and N2-shell vacancies.

Original languageEnglish
Pages (from-to)3782-3787
Number of pages6
JournalJournal of the Physical Society of Japan
Volume53
Issue number11
DOIs
Publication statusPublished - jan. 1 1984

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ASJC Scopus subject areas

  • Physics and Astronomy(all)

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