Neutron star matter in a relativistic mean-field theory

被引：1
|
作者：
Manka, R [1 ]
Bednarek, I [1 ]
Przybyla, G [1 ]
机构：
[1] Silesian Univ, Inst Phys, Uniwersytecka 4, PL-40007 Katowice, Poland
来源：
PHYSICAL REVIEW C | 2000年 / 62卷 / 01期
关键词：
D O I：
10.1103/PhysRevC.62.015802
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 nucleon effective mass, binding energy, and neutron star configuration in the relativistic mean-field (RMF) theory are considered. The calculations are motivated by the construction of the equation of state for a neutron star in the RMF theory. The equations of state for different parameter sets are calculated using the Feynman-Bogoliubov variational method for temperature different from zero. Various equations of state enable the construction of neutron star models.
引用
收藏
页码：158021 / 1580210
页数：10
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