Monte Carlo simulation assesses neutrino detection in a deep-underwater Cherenkov detector, suggesting feasibility for supernova events.
We present a complete Monte Carlosimulation of the response of a realistic model of a deep-underwater Cherenkov detector to Supernova neutrinos. The various sources of noise are discussed in detail and a statistical treatment of the data is proposed based upon the integration on a properly chosen time interval. The results show that the neutrino flux emitted by a Supernovaexploding in our Galaxy can be detected from such a telescope
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Ernesto et al. (2003) studied this question.
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