Symmetry energy in nuclei and neutron stars

被引:30
作者
Lattimer, James M. [1 ,2 ]
机构
[1] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA
[2] Yukawa Inst Theoret Phys, Kyoto 6068317, Japan
关键词
Nuclear matter; Neutron matter; Equation of state; Neutron stars; Supernovae; EQUATION; COLLAPSE; MASSES; STATE; MATTER;
D O I
10.1016/j.nuclphysa.2014.04.008
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
The symmetry energy plays an important role in nuclear astrophysics, ranging from the structure of nuclei to gravitational collapse to neutron stars. The BBAL paper by Bethe, Brown, et al., was among the first to recognize its importance. The role of the symmetry energy has evolved since that time when it represented one of the major uncertainties in modeling the equation of state of dense nuclear matter. At present, the parameters of the nuclear symmetry energy are tightly constrained by a concordance achieved from nuclear experiment, astrophysical observations, and ab initio theoretical calculations of neutron matter. (C) 2014 Elsevier B.V. All rights reserved.
引用
收藏
页码:276 / 295
页数:20
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