Signatures of QCD Phase Transition in a Newborn Compact Star

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dc.creatorWong, K. -W.
dc.creatorChu, M. -C.
dc.date2003-04-29
dc.date2004-04-19
dc.date.accessioned2026-07-07T02:08:21Z
dc.date.available2026-07-07T02:08:21Z
dc.descriptionWe study the scenario that a new born strange quark star cools to the Quantum ChromoDynamics (QCD) phase transition temperature and converts to a neutron star, and we calculate the evolution of temperature and luminosity of the compact star. We argue that the conversion energy released can be of the order $10^{53}$ erg. We also propose that a second neutrino burst will be emitted at the completion of this phase transition.
dc.description6 pages, 1 figure, minor modified and subtitles added, typos corrected. Accepted for publication in Monthly Notice Letter
dc.identifierhttps://arxiv.org/abs/astro-ph/0304515
dc.identifierhttp://arxiv.org/abs/astro-ph/0304515
dc.identifierMon.Not.Roy.Astron.Soc. 350 (2004) L42
dc.identifierdoi:10.1111/j.1365-2966.2004.07849.x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6013
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Theory
dc.titleSignatures of QCD Phase Transition in a Newborn Compact Star
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