Li (i=1–3) subshell fluorescence and Coster-Kronig yields for elements with 70⩽Z⩽92

Calculation of Coster-Kronig Enhancement Factors of the Some Elements in the Atomic Number Range 50 ≤ Z ≤ 59

“…We calculated that the presence of nonradiative transitions cause changes in the X-ray intensities. It is known that the nonradiative transitions compete with radiative transitions, and they together determine both the absolute and the relative intensities of generated X-rays [11]. The values of the Coster-Kronig enhancement factors (for κ α1 , κ α2 and κ β1 , κ β2 ) versus atomic number have been shown in Figs.…”

“…Recently, many researchers have investigated fluorescence cross-sections, the Coster-Kronig transitions, fluorescence yields for various elements [3][4][5][6][7][8][9][10][11]. Chemical effects on the K β /K α intensity ratios and on the enhancement of the Coster-Kronig transitions have been investigated [12,13].…”

Variation of Coster-Kronig enhancement factors at different excitation energies of the elements in the atomic number range 41 ≤ Z ≤ 49

“…2 There are many researchers who have examined XRF cross-sections, CK transitions; fluorescence yields for some elements. [3][4][5][6][7][8][9][10][11][12][13] DOI: http://dx.doi.org/10.32571/ijct.634210 E-ISSN:2602-277X…”

Synchrotron radiation induced X‐ray production cross sections of 66Dy at energies across its Li (i = 1–3) subshell absorption edges

“…The reliability of the IPA models [1] has been tested through measurements of the L i (i = 1-3) subshell XRP cross sections at incident photon energies much above the L i absorption edge energies of different elements by a number of authors. [11][12][13][14] However, to the best of our knowledge, similar investigations at incident photon energies in vicinity of the L i absorption edges of rare earth elements are not available in literature.…”