The Equation of State for Dense QCD and Quark Stars

Details The Equation of State for Dense QCD and Quark Stars The Equation of State for Dense QCD and Quark Stars

2002-06-20

arxiv.org/abs/hep-ph/0206196v2

Phys.Rev. D66 (2002) 105001

Physics

High Energy Physics

High Energy Physics - Phenomenology

7 pages, 3 figures

Scientific paper

10.1103/PhysRevD.66.105001

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 quark chemical potential below 1 GeV which leads to large theoretical uncertainties in the quark star mass-radius relation.

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