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We discuss the importance of observing supernova neutrinos. By analyzing theSN1987A observations of Kamiokande-II, IMB and Baksan, we show that theyprovide a 2.5{\sigma} support to the standard scenario for the explosion. Wediscuss in this context the use of neutrinos as trigger for the search of thegravity wave impulsive emission. We derive a bound on the neutrino mass usingthe SN1987A data and argue, using simulated data, that a future galacticsupernova could probe the sub-eV region.

Using supernova neutrinos to monitor the collapse, to search for gravity waves and to probe neutrino masses