Radiative transition probabilities for vacancies in M sub-shells

1 July 1970

journal article
Published by IOP Publishing in Journal of Physics B: Atomic and Molecular Physics

Vol. 3 (7) , 916-924
https://doi.org/10.1088/0022-3700/3/7/004

Abstract

Numerical results for the radiative transition probabilities are presented when a vacancy exists in an M sub-shell over a wide range of atomic numbers. The relativistic Hartree-Fock-Slater atomic model is used.

Keywords

This publication has 10 references indexed in Scilit:

Relativistic calculation of atomic X-ray transition rates
The European Physical Journal A, 1970
Radiative Decay Rates of Vacancies in the $K$ and $L$ Shells
Physical Review B, 1969
Internal Conversion Coefficients with Relativistic Hartree-Fock Model for the Deformed Region
Physical Review B, 1967
Finite Nuclear Size Effects in $β$ Decay
Physical Review B, 1962
Retardation andKX-Ray Relative Intensities
Physical Review B, 1960
Relativistic calculation of the K-LL Auger spectrum
Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1959
Contribution à l’étude des processus de transitions radiatives et non radiatives dans le cortège électronique
Annales de Physique, 1958
Experimental Methods of X-ray Spectroscopy: Ordinary Wavelengths
Published by Springer Nature ,1957
Relativistic Radiative Transitions
Physical Review B, 1956
The intensity of X-ray spectrum lines of heavy elements
Mathematical Proceedings of the Cambridge Philosophical Society, 1936