Equation of state for dense QCD and quark stars

被引:53
作者
Andersen, JO
Strickland, M
机构
[1] Univ Utrecht, Inst Theoret Phys, NL-3584 CE Utrecht, Netherlands
[2] Duke Univ, Dept Phys, Durham, NC 27701 USA
来源
PHYSICAL REVIEW D | 2002年 / 66卷 / 10期
关键词
D O I
10.1103/PhysRevD.66.105001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We calculate the equation of state for degenerate quark matter to leading order in hard-dense-loop (HDL) perturbation theory. We solve the Tolman-Oppenheimer-Volkov equations to obtain the mass-radius relation for dense quark stars. Both the perturbative QCD and the HDL equations of state have a large variation with respect to the renormalization scale for muless than or similar to1 GeV which leads to large theoretical uncertainties in the quark star mass-radius relation.
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页数:7
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