Velocities of pulsars and neutrino oscillations
arXiv:hep-ph/9606428 · doi:10.1103/PhysRevLett.77.4872
Abstract
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.
replaced with the final draft (to appear in Phys. Rev. Lett.); 10 pages, latex, epsf, 1 figure included, complete postscript file is available at ftp://dept.physics.upenn.edu/pub/Kusenko/UPR705T.ps
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