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QCD phase transition in rotating neutron star,neutrino beaming and gamma-ray bursters
Authors:Abhijit Bhattacharyya  Sanjay K Ghosh  Sibaji Raha
Institution:1. Department of Physics, Scottish Church College, 1 & 3, Urquhart Square, Kolkata 700 006, India;2. Department of Physics and Centre for Astroparticle Physics & Space Science, Bose Institute, 93/1, A.P.C. Road, Kolkata 700 009, India
Abstract: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.
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