A new parametric equation of state and quark stars
A new parametric equation of state and quark stars
Abstract
It is still a matter of debate to understand the equation of state of cold matter with supra-nuclear density in compact stars because of unknown non-perturbative strong interaction between quarks. Nevertheless, it is speculated from an astrophysical view
关键词
参数方程/夸克星/核子相互作用/强相互作用/表面相互作用/天体物理学/相互作用势/状态方程Key words
quark star/solid quark matter/mass radius relation/massive pulsar引用本文复制引用
基金项目
出版年
2011
NETL
NSTL
万方数据