Abstract
We discuss various relativistic models describing ground-state properties of spherical nuclei, are discussed. Relativistic mean-field and Hartree-Fock theories, which serve as a startingpoint 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. (orig.)
Citation Formats
Boersma, H F, and Malfliet, R.
From nuclear matter to finite nuclei. Pt. 2. Relativistic theories for finite nuclei.
Netherlands: N. p.,
1993.
Web.
Boersma, H F, & Malfliet, R.
From nuclear matter to finite nuclei. Pt. 2. Relativistic theories for finite nuclei.
Netherlands.
Boersma, H F, and Malfliet, R.
1993.
"From nuclear matter to finite nuclei. Pt. 2. Relativistic theories for finite nuclei."
Netherlands.
@misc{etde_10153572,
title = {From nuclear matter to finite nuclei. Pt. 2. Relativistic theories for finite nuclei}
author = {Boersma, H F, and Malfliet, R}
abstractNote = {We discuss various relativistic models describing ground-state properties of spherical nuclei, are discussed. Relativistic mean-field and Hartree-Fock theories, which serve as a startingpoint 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. (orig.)}
place = {Netherlands}
year = {1993}
month = {Aug}
}
title = {From nuclear matter to finite nuclei. Pt. 2. Relativistic theories for finite nuclei}
author = {Boersma, H F, and Malfliet, R}
abstractNote = {We discuss various relativistic models describing ground-state properties of spherical nuclei, are discussed. Relativistic mean-field and Hartree-Fock theories, which serve as a startingpoint 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. (orig.)}
place = {Netherlands}
year = {1993}
month = {Aug}
}