Finite Temperature Quark Matter and Supernova Explosion

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dc.creatorDrago, Alessandro
dc.creatorTambini, Ubaldo
dc.date1997-03-21
dc.date.accessioned2026-07-07T10:57:48Z
dc.date.available2026-07-07T10:57:48Z
dc.descriptionWe study the equation of state of quark matter at finite temperature, using a confinement model in which chiral symmetry remains broken in the deconfined phase. Implications for type II supernova explosion and for the structure and evolution of the proto-neutron star are discussed.
dc.descriptionRevTeX file + 5 postscript figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9703138
dc.identifierhttp://arxiv.org/abs/astro-ph/9703138
dc.identifierJ.Phys.G25:971-979,1999
dc.identifierdoi:10.1088/0954-3899/25/5/302
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186884
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleFinite Temperature Quark Matter and Supernova Explosion
dc.typetext

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