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SUMMARY:Phenomenological Aspects of Supernova Neutrinos
DTSTART;VALUE=DATE-TIME:20060301T110000Z
DTEND;VALUE=DATE-TIME:20060301T120000Z
DTSTAMP;VALUE=DATE-TIME:20261113T005636Z
UID:indico-event-1483@indico.ific.uv.es
DESCRIPTION:Core-collapse Supernovae (SNe) are one of the most energetic e
 xplosive events known. These occur at the end of a massive ($M \\gtrsim 8 
 M_\\odot$) star's lifetime\, and implies an energy release of the order of
  $O(10^{53})~erg$.\nFrom a particle physics point of view neutrinos turn o
 ut to be essential in such events. First they are thought to play a key ro
 le during the explosion phase and in the posterior cooling and deleptoniza
 tion of the star. On the other hand they are responsible to carry away aro
 und $99\\%$ of the total energy emitted. Therefore these neutrinos could b
 e easily detected in the case of a nearby supernova in the existent or pla
 nned neutrino detectors\, what could provide a lot of information about bo
 th neutrino properties and the supernova itself.\nIn this talk I will give
  an overview on the phenomenology involving these neutrinos. I will review
  the main features of the neutrino spectra and their propagation through t
 he SN envelope\, as well as the current related uncertainties. Then I will
  describe the expected signal in the case of a future galactic SN\, and it
 s implications in the determination of neutrino properties and SN physics.
 \n\nhttps://indico.ific.uv.es/event/1483/
LOCATION:Edf. Institutos de Investigación Sala Seminarios IFIC
URL:https://indico.ific.uv.es/event/1483/
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