Neutrino asymmetry in general relativistic rotating radiative stars
arXiv:gr-qc/0210107 · doi:10.1142/S0218271803003323
Abstract
Neutrino asymmetry in general relativistic radiative spacetime exterior to spinning stars is investigating by making use of Newmann-Penrose (NP) spin coefficient formalism. It is shown that neutrino current depends on the direction of rotation of the star. The solution is obtained in test field approximation where the neutrinos do not generate gravitational fields.
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