Finite Temperature Quark Matter and Supernova Explosion

Preprint

21 March 1997

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/9703138

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.

Keywords

SUPERNOVA EXPLOSION
FINITE TEMPERATURE
TEMPERATURE QUARK
QUARK MATTER
NEUTRON STAR
CHIRAL

All Related Versions

Version 1, 1997-03-21, ArXiv
Published version: Journal of Physics G: Nuclear and Particle Physics, 25 (5), 971.

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