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.
- Received 10 November 1998
DOI:https://doi.org/10.1103/PhysRevD.59.061302
©1999 American Physical Society