Astrophysical and Laboratory Constraints for the Dense Matter Equation of State

被引：3
|
作者：
Lattimer, James M. [1 ]
机构：
[1] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA
来源：
ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2011 | 2012年 / 1484卷
关键词：
neutron stars; dense matter; equation of state; nuclear symmetry energy; NEUTRON-STAR; COMPANION; NUCLEI;
D O I：
10.1063/1.4763414
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
New measurements of neutron star masses and radii have lead to powerful constraints on the dense matter equation of state. In the vicinity of the nuclear saturation density, the symmetry energy is the least well understood aspect of the nuclear force. Independent constraints from a variety of nuclear experiments are now able to refine the parameters of the symmetry energy.
引用
收藏
页码：319 / 326
页数：8
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