Systematic Study of the Nuclear Structure for Some Exotic Nuclei Using Skyrme-Hartree-Fock Method

The ground state charge, neutron, proton and matter densities, the associated nuclear radii and the binding energy per nucleon of B-8, Ne-17, Al-23 and P-27 halo nuclei have been investigated using the Skyrme-Hartree-Fock (SHF) model with the new SKxs25 parameters. According to the calculated results, it is found that the SHF model with these Skyrme parameters provides a good description on the nuclear structure of above proton-rich halo nuclei. The elastic charge form factors of B-8 and Ne-17 halo nuclei and those of their stable isotopes B-10 and Ne-20 are calculated using plane-wave Born approximation with the charge density distributions obtained by SHF model to investigate the effect of the extended charge distributions of proton-rich nuclei on the elastic electron scattering. Calculations show that the major difference between the elastic charge form factors of halo nuclei and those of their stable isotopes is caused by the variation in the charge density distributions, especially the details of the outer parts.