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VERSION:2.0
PRODID:-//CERN//INDICO//EN
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SUMMARY:Pulsar acceleration by asymmetric emission of sterile neutrinos
DTSTART;VALUE=DATE-TIME:20000718T140000Z
DTEND;VALUE=DATE-TIME:20000718T150000Z
DTSTAMP;VALUE=DATE-TIME:20261012T054641Z
UID:indico-event-1184@indico.ific.uv.es
DESCRIPTION:A convincing explanation for the observed pulsars large peculi
 ar velocities is still missing. We argue that any viable particle physics 
 solution would most likely involve the resonant production of a non-intera
 cting neutrino $\\nu_s$ of mass $m_{\\nu_s}\\sim 20-50\\\,$keV. We propose
  a model where anisotropic magnetic field configurations strongly bias the
  resonant spin flavour precession of tau antineutrinos into $\\nu_s$ . The
  asymmetric emission of $\\nu_s$ from the core can produce sizeable natal 
 kicks and account for recoil velocities of several hundred kilometers per 
 second.\n\nhttps://indico.ific.uv.es/event/1184/
LOCATION:Edf. Institutos de Investigación Sala Seminarios IFIC
URL:https://indico.ific.uv.es/event/1184/
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