Neutrino asymmetry in general relativistic rotating radiative stars
classification
🌀 gr-qc
keywords
neutrinoasymmetrygeneralradiativerelativisticstarsapproximationcoefficient
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.