Pulsar kicks from neutrino oscillations
arXiv:astro-ph/9811144 · doi:10.1103/PhysRevD.59.061302
Abstract
Neutrino oscillations can explain the observed motion of pulsars. We show that two different models of neutrino emission from a cooling neutron star are in good quantitative agreement and predict the same order of magnitude for the pulsar kick velocity, consistent with the data.
revtex; 4 pages
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