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

Details A Skyrme parametrization from subnuclear to neutron star densitiesPart II. Nuclei far from stabilities A Skyrme parametrization from subnuclear to neutron star densitiesPart II. Nuclei far from stabilities

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998nupha.635..231c&link_type=abstract

Nuclear Physics A, Volume 635, Issue 1-2, p. 231-256.

Physics

Nuclear Physics

569

Scientific paper

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 nuclei 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.

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