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arXiv · hep-ph/0106090

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

A. Peshier·B. Kampfer·G. Soff
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Abstract

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, $β$-stable deconfined matter limits the mass and the size of quark stars.

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A. Peshier, B. Kampfer, G. Soff. 2001-06-15. Stringent limits on quark star masses due to the chiral transition temperature. https://arxiv.org/abs/hep-ph/0106090

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