A Skyrme parametrization from subnuclear to neutron star densities. Part II. Nuclei far from stabilities

For pt.I see ibid., vol.627, p.710-46, 1997. In a first paper Skyrme effective forces were revisited in order to improve their isospin properties away from the β stability line. In this paper, these forces are specifically adjusted to reproduce finite-nucleus properties. Spin-orbit terms and center of mass correlations are analyzed. New Skyrme parametrizations are proposed and some of their spectroscopic properties are presented, e.g. S2n, S2p and r.m.s. radii for different isotopic and isotonic series. (orig.)