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QCD phase transition in rotaing neutron star, Neutrino beaming and Gamma-ray bursters
We have studied the emission of neutrinos from a rotating hybrid star. We
find that the emission is predominantly confined to a very small angle,
provided the core of the star is in a mixed phase of quarks and hadrons and the
size of such a mixed phase is small. Annihilation of neutrinos to produce gamma
rays has been discussed. The estimated duration of the burst is found to be
within the observational range.Comment: Modified manuscript with 9 pages including 3 ps figures, Accepted for
publication in Phys. Lett.
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