From nuclear matter to finite nuclei. 2. Relativistic theories for finite nuclei
Nov 15, 199360 pages
Published in:
- Phys.Rev.C 49 (1994) 1495-1515
Report number:
- KVI-1003
Citations per year
Abstract: (APS)
We discuss various relativistic models describing ground-state properties of spherical nuclei. Relativistic mean-field and Hartree-Fock theories, which serve as a starting point for subsequent models, are reviewed. Using a density-dependent parametrization of the Dirac-Brueckner G matrix in nuclear matter, we achieve an effective Dirac-Brueckner-Hartree-Fock model for finite nuclei. Finite nuclei results obtained with this model are compared with the less advanced density-dependent mean-field model, which simulates Dirac-Brueckner calculations for nuclear matter as well. It is shown that the effective Dirac-Brueckner-Hartree-Fock approach most successfully reproduces experimental data concerning spherical nuclei.Note:
- In Kyoto U., Yukawa Inst. Library only
- 21.65.+f
- 21.30.+y
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