Abstract
Relativistic calculations for radiative transition rates between atomic inner shells have been made analytically by the use of the Hartree-Fock-Roothaan method. The atomic electrons are taken to be in the single-particle states in the central potential and expressed in terms of Slater-type orbitals. Retardation effects, all multipole contributions of the radiation field, and the effect of finite nuclear size are included. The calculated results are in agreement with the numerical calculations by the relativistic Hartree-Fock and Hartree-Fock-Slater models.
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