Neutron star in relativistic mean-field approximation

被引：0

作者：

Sun, BX ^{[1
]}

Jia, HY

Meng, J

Zhao, EG

机构：

[1] Chinese Acad Sci, Inst Theoret Phys, Beijing 100080, Peoples R China

[2] Peking Univ, Dept Tech Phys, Beijing 100871, Peoples R China

[3] Natl Lab Heavy Ion, Ctr Theoret Nucl Phys, Lanzhou 730000, Peoples R China

来源：

HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION | 2000年 / 24卷

关键词：

neutron star matter; relativistic mean mean-field approximation;

D O I：

暂无

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 equations of state of the neutron star matter are calculated in the relativistic mean-field approximation with different couplings of the hyperons. The properties of neutron stars are studied by solving the Oppenheimer-Volkoff equation. It shows that these properties change distinctly as different couplings of hyperons are concerned.

引用

页码：69 / 72

页数：4