2013
DOI: 10.1088/0953-4075/46/6/065001
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Relativistic calculations of M-shell decay rates and yields in Zn, Cd and Hg

Abstract: In this work, we calculate the radiative and radiationless transition probabilities of M-shell vacancies in Zn, Cd and Hg atoms using the Dirac–Fock method. The obtained transition probability values are then used to calculate the corresponding fluorescence, Auger and Coster–Kronig yields for each subshell that are compared to existing theoretical calculations. Average M-shell fluorescence yields are derived and compared with semi-empirical and experimental results.

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Cited by 11 publications
(1 citation statement)
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“…Continuum-state wave functions were obtained by solving the Dirac-Fock equations with the same atomic potential of the initial state, normalized to represent one ejected electron per unit energy. Radiationless rates were, however, calculated using the correct transition energies obtained in previous independent calculations of initial and final state wave functions and eigenvalues [37][38][39].…”
Section: A Relativistic Calculationsmentioning
confidence: 99%
“…Continuum-state wave functions were obtained by solving the Dirac-Fock equations with the same atomic potential of the initial state, normalized to represent one ejected electron per unit energy. Radiationless rates were, however, calculated using the correct transition energies obtained in previous independent calculations of initial and final state wave functions and eigenvalues [37][38][39].…”
Section: A Relativistic Calculationsmentioning
confidence: 99%