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

• Published in: Nuclear physics. A Vol. 635; no. 1; pp. 231 - 256
• Main Authors: Chabanat, E., Bonche, P., Haensel, P., Meyer, J., Schaeffer, R.
• Format: Journal Article
• Language: English
• Published: Elsevier B.V 25-05-1998
• Subjects: 21.30.+y; 21.10.−k; 21.60.−n; 21.60.Jz
• ISSN: 0375-9474
• DOI: 10.1016/S0375-9474(98)00180-8

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.
S
2
n
,
S
2
p
and r.m.s. radii for different isotopic and isotonic series.