Quark matter in neutron stars

被引：18
作者：
Alford, Mark G. [1 ]
机构：
[1] Washington Univ, Dept Phys, St Louis, MO 63130 USA
来源：
NUCLEAR PHYSICS A | 2009年 / 830卷
关键词：
COLOR-FLAVOR LOCKING; SYMMETRY-BREAKING; SUPERCONDUCTIVITY; QCD; NEUTRALITY; EQUATIONS; STATE;
D O I：
10.1016/j.nuclphysa.2009.09.034
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：
According to quantum chromodynamics, matter at ultra-high density and low temperature is a quark liquid, with a condensate of Cooper pairs of quarks near the Fermi surface ("color superconductivity"). This paper reviews the physics of color superconductivity, and discusses some of the proposed signatures by which we might detect quark matter in neutron stars.
引用
收藏
页码：385C / 392C
页数：8
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