Supernova Neutrinos and the absolute scale of neutrino masses - a Bayesian approach
| dc.creator | Nardi, Enrico | |
| dc.date | 2004-12-02 | |
| dc.date.accessioned | 2026-07-07T03:54:00Z | |
| dc.date.available | 2026-07-07T03:54:00Z | |
| dc.description | 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. | |
| dc.description | 4 pages. Contribution to the proceedings of the Fifth Latin American Simposium on High Energy Physics (V-SILAFAE) Lima, Peru, July 12-17, 2004 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0412024 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0412024 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/44066 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Supernova Neutrinos and the absolute scale of neutrino masses - a Bayesian approach | |
| dc.type | text |