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

页码：158021 / 1580210

页数：10

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