Stringent limits on quark star masses due to the chiral transition temperature

Details Stringent limits on quark star masses due to the chiral transition temperature Stringent limits on quark star masses due to the chiral transition temperature

2001-06-08

arxiv.org/abs/hep-ph/0106090v2

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages with figs (v2: minor grammatical changes)

Scientific paper

Recent finite-temperature QCD lattice data are analyzed within a
quasiparticle model, and extrapolated to nonzero chemical potential. Determined
by the chiral transition temperature, the resulting equation of state of charge
neutral, $\beta$-stable deconfined matter limits the mass and the size of quark
stars.

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