2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/178542Neutrino 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 pagesAstrophysicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenologytext