Cooling Delay for Protoquark Stars due to Neutrino Trapping

Details Cooling Delay for Protoquark Stars due to Neutrino Trapping Cooling Delay for Protoquark Stars due to Neutrino Trapping

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004csqn.conf..399b&link_type=abstract

COMPACT STARS The Quest for New States of Dense Matter. Proceedings of the KIAS-APCTP International Symposium on Astro-Hadron Ph

Physics

Scientific paper

The 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 Topac ~ 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.

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