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A new parametric equation of state and quark stars

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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

quark starsolid quark mattermass radius relationmassive pulsar

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

10973002, 109350012009CB824800

2011

高能物理与核物理
中国物理学会

高能物理与核物理

SCI
ISSN:0254-3052
年,卷(期):2011.35(7)