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L shell fluorescence yields and coster—kronig transition probabilities for the elements with 25 ⩽ Z ⩽ 96
Author(s) -
Puri S.,
Mehta D.,
Chand B.,
Singh Nirmal,
Trehan P. N.
Publication year - 1993
Publication title -
x‐ray spectrometry
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.447
H-Index - 45
eISSN - 1097-4539
pISSN - 0049-8246
DOI - 10.1002/xrs.1300220507
Subject(s) - fluorescence , atomic physics , radiative transfer , l shell , shell (structure) , atomic number , physics , chemistry , dirac (video compression format) , range (aeronautics) , transition metal , electron shell , materials science , quantum mechanics , ion , ionization , earth's magnetic field , biochemistry , magnetic field , neutrino , composite material , catalysis
The values of L i sub‐shell fluorescence yields (ω i ) and Coster–Kronig transition probabilities ( f ij ) were evaluated using radiative and non‐radiative transition rates based on the relativistic Dirac–Hartree–Slater (RDHS) model for all the elements in the atomic number range 25 ⩽ Z ⩽ 96. The values of the Coster–Kronig‐corrected fluorescence (v i ) and average L shell fluorescence (ϖ L ) yields were also evaluated and least‐squares fitted to obtain the polynomials representing them as a function of atomic number.