The birth of strange matter from two-flavor quark matter in a neutron star

Details The birth of strange matter from two-flavor quark matter in a neutron star The birth of strange matter from two-flavor quark matter in a neutron star

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phlb..319..199d&link_type=abstract

Physics Letters B, Volume 319, Issue 1-3, p. 199-202.

Physics

16

Scientific paper

The phase transition of two-flavor quark matter into strange matter in the interior of a neutron star is studied. It is shown that the timescale of the transition is below 0.1 ωs and the s-quark semileptonic processes are of significance in neutrino emissions during the transition. Owing to these processes, the transition in a young neutron star of 1.4Msolar mass will liberate more than 3×1051 erg of energy as a neutrino burst.

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