The Evolution of Proto-Strange Stars

Published 6 Sep 2013 in astro-ph.HE | (1309.1532v1)

Abstract: We perform 1D calculations of neutrino opacities inside a young "strange star" assumed to be the result of the conversion process of a normal neutron object. We evaluate the deleptonization and cooling timescales, which happen to be longer than the proto-NS analogues, and preliminary address the features of the emerging neutrino signal.

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