RelativisticL-shell Auger and Coster-Kronig rates and fluorescence yields

Extension of atomic configuration sets of the Non-LTE model in the application to the Kα diagnostics of hot dense matter

“…As an example, a few transition energies of configurations within the STA from [K 1 L 8 M 6 ] to [K 2 L 7 M 6 ] of P-like copper ions are computed by a DHS (Dirac-Hartree-Slater) code [19] and listed in the Table 2. There are 131 configurations belonging to the superconfiguration [K 1 L 8 M 6 ] and Ka 2 energies range from 8049.5 to 8080.7 eV for copper ions.…”

K-shell fluorescence yields for elements with 6≤Z≤99

“…The K-shell fluorescence yield of an atom is defined as the probability that a vacancy in the K-shell is filled through a radiative transition. Several attempts have been made, in a tabular form, for measuring (Al-Nasr et al, 1987;Arora et al, 1981;Ahmad, 1979;Broyles et al, 1953;Bertrand et al, 1959;Bambynek et al, 1965;Brabets et al, 1959;Balakrishna et al, 1994;Brunner, 1987;Bhan et al, 1981;Famoux, 1985;Casnati et al, 1991;Chen et al, 1979;Drever and Moljk, 1957;Durak and Sahin, 1998;Erman and Sujkowski, 1961;Espenschied and Hoffmann, 1978;Egorov et al, 1989;Fairbrother et al, 1957;Forest and Easterda, 1959;Freedman et al, 1977;Frey et al, 1958;Garg et al, 1985;Godeau, 1961;Gray, 1956;Graham and Merritt, 1961;Apaydın and Tıras -oglu, 2006;Geidelman et al, 1988;Gurov et al, 1981;Harrison et al, 1955;Han et al, 2007;Heintze, 1955;Hagedoorn and Konijn, 1957;Hagedoorn and Wapstra, 1960;Hoffman and Dropesky, 1958;Hribar et al, 1977;Konstantinov et al, 1961;Kramer et al, 1962;Kramer, 1961;Konstantinov et al, 196...…”

FLYCHK: Generalized population kinetics and spectral model for rapid spectroscopic analysis for all elements

“…We have performed a study of the form by comparing this rate with values calculated by Dirac-Hartree-Slater (DHS) code [23] and found that the gaunt factor 0.15 gives a better agreement than the standard value 0.12.…”