Clusters in Nuclear Matter and the Equation of State for Astrophysical Applications

被引：7
作者：
Typel, Stefan [1 ]
机构：
[1] GSI Helmholtzzentrum Schwerionenforsch GmbH, D-64291 Darmstadt, Germany
来源：
XII HADRON PHYSICS | 2013年 / 1520卷
关键词：
nuclear matter; equation of state; cluster formation and dissolution; medium effects; relativistic density functional; MEAN-FIELD THEORY; NEUTRON-STAR; DENSE MATTER; SUPERNOVA; MODELS; HOT;
D O I：
10.1063/1.4795946
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：
Thermodynamic properties and the composition of dense matter are affected strongly by correlations leading to the formation of nuclei at densities below nuclear saturation density. These features of the equation of state (EoS) are essential in astrophysical applications, e. g. the simulation of core-collapse supernovae. Theoretical approaches to consider correlation effects on different levels of approximation are discussed. A generalized relativistic density functional approach is presented that exhibits the correct limits at low and high densities.
引用
收藏
页码：68 / 102
页数：35
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