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SUMMARY:Supernova neutrino signal and neutrino masses: A powerful statisti
 cal approach
DTSTART;VALUE=DATE-TIME:20050510T100000Z
DTEND;VALUE=DATE-TIME:20050510T110000Z
DTSTAMP;VALUE=DATE-TIME:20261113T080827Z
UID:indico-event-1428@indico.ific.uv.es
DESCRIPTION:Extracting informations on the neutrino mass values from a Sup
 ernova neutrino signal\, without any reference to additional astrophysical
  events as time benchmarks for measuring possible neutrino time of flight 
 delays\, is a challeging statistical problem and requires powerful as well
  as robust methods. We describe a strategy that\, with the present neutrin
 o detectors\, could allow to reach a sensitivity of the order of 1 eV. The
 refore\,a Galactic Supernova explosion occuring the next few years could s
 till provide interesting informations on the neutrino masses\; however we 
 argue that future megatonne neutrino detectors will not be competitive wit
 h the next generation of triitum beta decay experiments.\n\nhttps://indico
 .ific.uv.es/event/1428/
LOCATION:Edf. Institutos de Investigación Sala Seminarios IFIC
URL:https://indico.ific.uv.es/event/1428/
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