Abstract
We analyze the 1496 days of SuperKamiokande data to put limits on the νe, νμ+ντ and components of the diffuse flux of supernova neutrinos, in different energy intervals and for different neutrino energy spectra. By considering the presence of only one component at a time, we find the following bounds at 90% CL and for neutrino energy E>19.3MeV: Φνe<73.3-154cm-2s -1, Φνμ+ντ<(1.0-1.4) × 103cm-2s-1 and , where the intervals account for varying the neutrino spectrum. In the interval E = 22.9-36.9MeV, we find Φνe<39-54cm-2s-1, which improves on the existing limit from SNO in the same energy window. Our results for νμ+ντ and improve by about four orders of magnitude the previous best constraints from LSD.
Original language | English (US) |
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Article number | 033 |
Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 2008 |
Issue number | 8 |
DOIs | |
State | Published - Aug 1 2008 |
Keywords
- Neutrino experiments
- Neutrino properties
- Star formation
- Supernova neutrinos
ASJC Scopus subject areas
- Astronomy and Astrophysics