arXiv · hep-ph/0412024
Supernova Neutrinos and the absolute scale of neutrino masses - a Bayesian approach
Abstract
We apply Bayesian methods to study the sensitivity to neutrino masses of a Galactic supernova neutrino signal. Our procedure makes use of the full statistics of events and is remarkably independent of astrophysical assumptions. Present detectors can reach a sensitivity down to $m_ν\sim 1$ eV. Future megaton detectors can yield up to a factor of two improvement; however, they will not be competitive with the next generation of tritium $β$-decay and neutrinoless double $β$-decay experiments.
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Enrico Nardi. 2004-12-02. Supernova Neutrinos and the absolute scale of neutrino masses - a Bayesian approach. https://arxiv.org/abs/hep-ph/0412024
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