Abstract
We review briefly the performance of self-consistent mean field models in connection with exotic nuclei. Two variants are discussed, the Skyrme-Hartree-Fock (SHF) method and the relativistic mean-field (RMF) model. The basic properties are summarized. Applications to neutron rich Sn isotopes and to superheavy elements are discussed. As effects slightly beyond mean field, we present recent results on low lying 2 + excitations in Sn isotopes and in 186 Pb.
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