scholarly journals Determination of Mass Absorption Coefficients of Al, Cr, Ni, Zn, Se, Zr, Sn, Sb, Gd, Au, Pb and Bi for the CuLα Line

1973 ◽  
Vol 37 (5) ◽  
pp. 493-495
Author(s):  
Kazuo Masato ◽  
Eiji Niki
1968 ◽  
Vol 1 (6) ◽  
pp. 695-706 ◽  
Author(s):  
G D Hughes ◽  
J B Woodhouse ◽  
I A Bucklow

1957 ◽  
Vol 28 (1) ◽  
pp. 98-105 ◽  
Author(s):  
Burton L. Henke ◽  
Richard White ◽  
Bruno Lundberg

1976 ◽  
Vol 31 (8) ◽  
pp. 887-897 ◽  
Author(s):  
J. D. Stephenson

AbstractA method is proposed, which primarily determines screening constants for incomplete atomic shells from the experimental ionization potentials of spin-paired Pauli-type orbitals. The method is complimentary and in addition to the standard Sommerfeld approach, which derives screening constants from X-ray spin doublet term differences. Atomic photoelectric absorption cross sections are computed from screened hydrogen-like eigenfunctions for low atomic number elements Z = 6 to 15, using a range of incident photon energies between 1 and 30 keV. Comparison with experiment and alternate more exact theories shows, that improved cross sections are obtained for the more important incomplete L-shell contributions. X-ray photoelectric mass absorption coefficients for low Z elements (Z= 6 to 15), employing 33 characteristic X-ray energies {NiKα (0.852 keV) to AgKβ (24.942 keV)}, are given.


Sign in / Sign up

Export Citation Format

Share Document