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A detailed general relativistic (GR) calculation of the neutrino path for ageneral metric describing a rotating star is studied. We have calculated theneutrino path along a plane, with the consideration that the neutrino does notat any time leave the plane. The expression for the minimum photosphere radius(MPR) is obtained and matched with the Schwarzschild limit. The MPR iscalculated for the stars with two different equations of state (EOS) eachrotating with two different velocities. The results shows that the MPR for thehadronic star is much greater than the quark star and the MPR increases as therotational velocity of the star decreases. The MPR along the polar plane islarger than that along the equatorial plane.

A General Relativistic study of the neutrino path and calculation of minimum photosphere for different stars