Cooling delay for protoquark stars due to neutrino trapping

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dc.creatorBerdermann, J.
dc.creatorBlaschke, D.
dc.creatorGrigorian, H.
dc.date2004-04-05
dc.date.accessioned2026-07-07T02:12:50Z
dc.date.available2026-07-07T02:12:50Z
dc.descriptionThe influence of neutrino trapping (NT) on the early cooling evolution of hot proto quark stars (PQS) with initial temperatures in the range T ~ 40 MeV is studied. Within a simplified model for the neutrino transport it is shown that the time for reaching neutrino opacity temperature of T_{opac} ~ 1 MeV is about 10 sec. This is an order of magnitude larger than without NT and of the same order as the duration long gamma ray bursts.
dc.description10 pages, 6 figures, contribution to the KIAS-APCTP International Symposium in Astro-Hadron Physics, Seoul, Korea, November 11-14, 2003
dc.identifierhttps://arxiv.org/abs/astro-ph/0404079
dc.identifierhttp://arxiv.org/abs/astro-ph/0404079
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7593
dc.subjectAstrophysics
dc.titleCooling delay for protoquark stars due to neutrino trapping
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