Finite Temperature Quark Matter and Supernova Explosion

Astronomy and Astrophysics – Astrophysics

Scientific paper

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RevTeX file + 5 postscript figures

Scientific paper

10.1088/0954-3899/25/5/302

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.

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