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Neutrino transport: no asymmetry in equilibrium
A small asymmetry in the flux of neutrinos emitted by a hot newly-born neutron star could explain the observed motions of pulsars. However, even in the presence of parity-violating processes with anisotropic scattering amplitudes, no asymmetry is generated in thermal equilibrium. We explain why this...
| Autores principales: | , , |
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| Lenguaje: | eng |
| Publicado: |
1998
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1016/S0370-2693(98)00918-6 http://cds.cern.ch/record/357287 |
| _version_ | 1780892545361903616 |
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| author | Kusenko, Alexander Segre, Gino Vilenkin, Alexander |
| author_facet | Kusenko, Alexander Segre, Gino Vilenkin, Alexander |
| author_sort | Kusenko, Alexander |
| collection | CERN |
| description | A small asymmetry in the flux of neutrinos emitted by a hot newly-born neutron star could explain the observed motions of pulsars. However, even in the presence of parity-violating processes with anisotropic scattering amplitudes, no asymmetry is generated in thermal equilibrium. We explain why this no-go theorem stymies some of the proposed explanations for the pulsar ``kick'' velocities. |
| id | cern-357287 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 1998 |
| record_format | invenio |
| spelling | cern-3572872023-03-14T20:37:01Zdoi:10.1016/S0370-2693(98)00918-6http://cds.cern.ch/record/357287engKusenko, AlexanderSegre, GinoVilenkin, AlexanderNeutrino transport: no asymmetry in equilibriumAstrophysics and AstronomyA small asymmetry in the flux of neutrinos emitted by a hot newly-born neutron star could explain the observed motions of pulsars. However, even in the presence of parity-violating processes with anisotropic scattering amplitudes, no asymmetry is generated in thermal equilibrium. We explain why this no-go theorem stymies some of the proposed explanations for the pulsar ``kick'' velocities.A small asymmetry in the flux of neutrinos emitted by a hot newly-born neutron star could explain the observed motions of pulsars. However, even in the presence of parity-violating processes with anisotropic scattering amplitudes, no asymmetry is generated in thermal equilibrium. We explain why this no-go theorem stymies some of the proposed explanations for the pulsar “kick” velocities.A small asymmetry in the flux of neutrinos emitted by a hot newly-born neutron star could explain the observed motions of pulsars. However, even in the presence of parity-violating processes with anisotropic scattering amplitudes, no asymmetry is generated in thermal equilibrium. We explain why this no-go theorem stymies some of the proposed explanations for the pulsar ``kick'' velocities.astro-ph/9806205CERN-TH-98-192CERN-TH-98-192oai:cds.cern.ch:3572871998-06-16 |
| spellingShingle | Astrophysics and Astronomy Kusenko, Alexander Segre, Gino Vilenkin, Alexander Neutrino transport: no asymmetry in equilibrium |
| title | Neutrino transport: no asymmetry in equilibrium |
| title_full | Neutrino transport: no asymmetry in equilibrium |
| title_fullStr | Neutrino transport: no asymmetry in equilibrium |
| title_full_unstemmed | Neutrino transport: no asymmetry in equilibrium |
| title_short | Neutrino transport: no asymmetry in equilibrium |
| title_sort | neutrino transport: no asymmetry in equilibrium |
| topic | Astrophysics and Astronomy |
| url | https://dx.doi.org/10.1016/S0370-2693(98)00918-6 http://cds.cern.ch/record/357287 |
| work_keys_str_mv | AT kusenkoalexander neutrinotransportnoasymmetryinequilibrium AT segregino neutrinotransportnoasymmetryinequilibrium AT vilenkinalexander neutrinotransportnoasymmetryinequilibrium |