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

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dc.creatorPeshier, A.
dc.creatorKampfer, B.
dc.creatorSoff, G.
dc.date2001-06-08
dc.date2001-06-15
dc.date.accessioned2026-07-07T03:44:44Z
dc.date.available2026-07-07T03:44:44Z
dc.descriptionRecent 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.
dc.description4 pages with figs (v2: minor grammatical changes)
dc.identifierhttps://arxiv.org/abs/hep-ph/0106090
dc.identifierhttp://arxiv.org/abs/hep-ph/0106090
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/40685
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleStringent limits on quark star masses due to the chiral transition temperature
dc.typetext

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