Velocities of pulsars and neutrino oscillations

Details Velocities of pulsars and neutrino oscillations Velocities of pulsars and neutrino oscillations

1996-06-25

arxiv.org/abs/hep-ph/9606428v2

Phys.Rev.Lett. 77 (1996) 4872-4875

Physics

High Energy Physics

High Energy Physics - Phenomenology

replaced with the final draft (to appear in Phys. Rev. Lett.); 10 pages, latex, epsf, 1 figure included, complete postscript f

Scientific paper

10.1103/PhysRevLett.77.4872

Neutrino oscillations, biased by the magnetic field, alter the shape of the neutrinosphere in a cooling protoneutron star emerging from the supernova collapse. The resulting anisotropy in the momentum of outgoing neutrinos can be the origin of the observed proper motions of pulsars. The connection between the pulsars velocities and neutrino oscillations results in a prediction for the tau neutrino mass of order 100 eV.

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