Abstract
The ground-state properties of the nucleus 100Sn have been studied by the non-relativistic mean-field approach with Skyrme interactions, the relativistic mean-field approach with the Hartree approximation and the density-dependent relativistic mean-field approach. We compare and discuss the numerical results of average binding energies, and matter root-mean-square radii of proton and neutron distributions. It is shown that the non-relativistic, relativistic and density-dependent relativistic mean-field theories can be successfully applied to the nucleus near the proton drip line.
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