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

被引：1776

作者：

Chabanat, E

Bonche, P

Haensel, P

Meyer, J

Schaeffer, R

机构：

[1] Univ Lyon 1, IN2P3, CNRS, Inst Phys Nucl, F-69622 Villeurbanne, France

[2] CEA Saclay, Serv Phys Theor, F-91191 Gif Sur Yvette, France

[3] Polish Acad Sci, N Copernicus Astron Ctr, PL-00716 Warsaw, Poland

来源：

NUCLEAR PHYSICS A | 1998年 / 635卷 / 1-2期

关键词：

D O I：

10.1016/S0375-9474(98)00180-8

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

In a first paper Skyrme effective forces were revisited in order to improve their isospin properties away from the beta 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-2n, S-2p and r.m.s. radii for different isotopic and isotonic series. (C) 1998 Elsevier Science B.V.

引用

页码：231 / 256

页数：26

共 83 条

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