Neutron stars, supernova explosions and the transition to quark matter

DOI10.1016/S0375-9474(99)85105-7zbMath0995.85003arXivastro-ph/9904124OpenAlexW2017921190MaRDI QIDQ1598654

Alessandro Drago

Publication date: 23 May 2002

Published in: Nuclear Physics. A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/9904124

zbMATH Keywords

MIT bag modelfinite temperature equation of statehybrid star structure

Mathematics Subject Classification ID

Nuclear physics (81V35) Strong interaction, including quantum chromodynamics (81V05) Galactic and stellar structure (85A15)

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