Effects of the density dependence of the symmetry energy on neutron stars

被引：0

作者：

刘晓进 ^{[1
]}

吴琛 ^{[1
]}

任中洲 ^{[1
,2
]}

机构：

[1] Physics Department,Nanjing University

[2] Center of Theoretical Nuclear Physics,National Laboratory of Heavy Ion Accelerator

来源：

中国物理C | 2010年 / 11期

基金：

中国国家自然科学基金;

关键词：

symmetry energy; neutron stars; relativistic mean field approximation; quark-meson coupling;

D O I：

暂无

中图分类号：

P145.6 [脉冲星（中子星）];

学科分类号：

070401 ;

摘要：

In this paper,we include the density dependence behavior of the symmetry energy in the improved quark mass density dependent (IQMDD) model.Under the mean field approximation,this model is applied to investigate neutron star matter and neutron stars successfully.Effects of the density dependence of the symmetry energy on neutron stars are described.

引用

页码：1709 / 1713

页数：5