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The Neutron Halo in Heavy Nuclei Calculated with the Gogny Force

B. Nerlo-Pomorska·K. Pomorski·J. F. Berger·J. Decharge
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Abstract

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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B. Nerlo-Pomorska, K. Pomorski, J. F. Berger, J. Decharge. 2000-06-27. The Neutron Halo in Heavy Nuclei Calculated with the Gogny Force. https://doi.org/10.1007/s10050-000-4502-1

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