Finite Temperature Quark Matter and Supernova Explosion
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We 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.
RevTeX file + 5 postscript figures
RevTeX file + 5 postscript figures