The Neutron Halo in Heavy Nuclei Calculated with the Gogny Force

Details The Neutron Halo in Heavy Nuclei Calculated with the Gogny Force The Neutron Halo in Heavy Nuclei Calculated with the Gogny Force

2000-06-27

arxiv.org/abs/nucl-th/0006061v1

Eur.Phys.J.A8:19-29,2000

Physics

Nuclear Physics

Nuclear Theory

13 pages in Latex and 17 figures in eps

Scientific paper

10.1007/s10050-000-4502-1

The proton and neutron density distributions, one- and two-neutron separation energies and radii of nuclei for which neutron halos are experimentally observed, are calculated using the self-consistent Hartree-Fock-Bogoliubov method with the effective interaction of Gogny. Halo factors are evaluated assuming hydrogen-like antiproton wave functions. The factors agree well with experimental data. They are close to those obtained with Skyrme forces and with the relativistic mean field approach.

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