Neutrino asymmetry in general relativistic rotating radiative stars

Details Neutrino asymmetry in general relativistic rotating radiative stars Neutrino asymmetry in general relativistic rotating radiative stars

2002-10-31

arxiv.org/abs/gr-qc/0210107v1

Int.J.Mod.Phys.D12:1047-1052,2003

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Latex file

Scientific paper

10.1142/S0218271803003323

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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