« Neutrino Burst from Supernova and Supernova Relic neutrinos » |
Katsuhiko Sato |
Collapse-driven supernovae are the most luminous neutrino source in the
universe. If a supernova appears at the center of our Galaxy, 10,000 events are detected by Superkamiokande, and it is expected fruitful information on the supernova core and neutrino physics are obtained. After reviewing the recent simulations of stellar core collapse, we show how the neutrino burst time profile and spectra are modified by neutrino oscillation. We also show the spectra of relic neutrinos emitted by past supernovae, and discuss the possibility of the detection of this neutrino background. |
vendredi 19 mars 2004 - 11:00 Salle des séminaires Évry Schatzman, Institut d'Astrophysique de Paris |
Page web du séminaire / Seminar's webpage |