Abstract
The Dirac-Brueckner-Hartree-Fock (DBHF) approximation, which has been successful in describing the saturation properties of infinite nuclear matter, is extended to the calculation of finite nuclei. As an example the ground-state properties of 16O are discussed. Inclusion of the relativistic effects yields a considerable increase for the raduis of the charge distribution with essentially no change of the calculated binding energy. This improves the agreement with the experimental data considerably.
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 callDisclaimer: 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.
