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VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Constraining neutrino physics with cosmological observations
DTSTART;VALUE=DATE-TIME:20060127T110000Z
DTEND;VALUE=DATE-TIME:20060127T120000Z
DTSTAMP;VALUE=DATE-TIME:20261113T015001Z
UID:indico-event-1476@indico.ific.uv.es
DESCRIPTION:According to the standard model of cosmology\, a thermal backg
 round of relic neutrinos at T=1.9 K fills up the present Universe\, in a s
 imilar way as the photons of the cosmic microwave background radiation do.
  The presence and the properties of this neutrino background affect the co
 smological evolution\; this means in turn that cosmological observations c
 an be used to indirectly measure their properties. In particular\, we can 
 obtain informations about the neutrino mass and about non-standard feature
 s\, such as the presence of large cosmological lepton asymmetry.\n\nhttps:
 //indico.ific.uv.es/event/1476/
LOCATION:Edf. Institutos de Investigación Sala Seminarios IFIC
URL:https://indico.ific.uv.es/event/1476/
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