Abstract
The non-locality and non-linearity of the atomic relativistic Hartree-Fock (RHF) equations have hampered the formulation of a consistent non-relativistic reduction. In the paper a reduction technique is presented that yields an RHF equation for which all terms are correct to second order in m-1. The results and techniques presented should be of use for practical calculations of atomic X-ray transition rates and energies.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Journal of Physics B: Atomic and Molecular Physics
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
