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Pulsar acceleration by asymmetric emission of sterile neutrinos
A convincing explanation for the observed pulsar large peculiar velocities is still missing. We argue that any viable particle physics solution would most likely involve the resonant production of a non-interacting neutrino $\nu_s$ of mass $m_{\nu_s}\sim$ 20--50 keV. We propose a model where anisotr...
| Autores principales: | , |
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| Lenguaje: | eng |
| Publicado: |
2000
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1086/319452 http://cds.cern.ch/record/444167 |