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VERSION:2.0
PRODID:-//CERN//INDICO//EN
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SUMMARY:Pulsar velocities and neutrinos
DTSTART;VALUE=DATE-TIME:19980601T140000Z
DTEND;VALUE=DATE-TIME:19980601T150000Z
DTSTAMP;VALUE=DATE-TIME:20260618T105955Z
UID:indico-event-1076@indico.ific.uv.es
DESCRIPTION:Neutrino oscillations\, biased by the magnetic field\, alter t
 he shape of the neutrinosphere in a cooling protoneutron star emerging fro
 m the supernova collapse. The resulting anisotropy in the momentum of outg
 oing neutrinos can be the origin of the observed proper motions of pulsars
 . The connection between the pulsars velocities and neutrino oscillations 
 results in a prediction for the tau neutrino mass of order 100 eV.\n\nhttp
 s://indico.ific.uv.es/event/1076/
LOCATION:Dpto. de Fisica Teorica (UVEG) Sala Seminarios
URL:https://indico.ific.uv.es/event/1076/
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