Finite Temperature Quark Matter and Supernova Explosion
天体物理学
2008-11-26 v1 核理论
摘要
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.
引用
@article{arxiv.astro-ph/9703138,
title = {Finite Temperature Quark Matter and Supernova Explosion},
author = {Alessandro Drago and Ubaldo Tambini},
journal= {arXiv preprint arXiv:astro-ph/9703138},
year = {2008}
}
备注
RevTeX file + 5 postscript figures