arXiv:astro-ph/9703138·v1·Astrophysics
Finite Temperature Quark Matter and Supernova Explosion
Alessandro Drago🇮🇹 · Ubaldo Tambini🇮🇹
Abstract
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.
Comments: RevTeX file + 5 postscript figures