Neutrino asymmetry in general relativistic rotating radiative stars
L.C. Garcia de Andrade
TL;DR
This paper investigates how neutrino asymmetry depends on the rotation of stars in a general relativistic setting using NP formalism, revealing that neutrino current varies with stellar rotation direction.
Contribution
It introduces a novel analysis of neutrino asymmetry in rotating radiative spacetimes using NP formalism, highlighting the dependence on stellar rotation direction.
Findings
Neutrino current depends on the star's rotation direction
Solution obtained in test field approximation
Neutrino asymmetry varies with stellar rotation
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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