Probing supernova physics with neutrino oscillations
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Probing supernova physics with neutrino oscillations

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Probing supernova physics with neutrino oscillations

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Minakata, Hisakazu; Nunokawa, Hiroshi; Tomàs, Ricard; Furtado Valle, José Wagner Perfil
Aquest document és un/a article, creat/da en: 2002
We point out that solar neutrino oscillations with large mixing angle as evidenced in current solar neutrino data have a strong impact on strategies for diagnosing collapse-driven supernova (SN) through neutrino observations. Such oscillations induce a significant deformation of the energy spectra of neutrinos, thereby allowing us to obtain otherwise inaccessible features of SN neutrino spectra. We demonstrate that one can determine temperatures and luminosities of non-electron flavor neutrinos by observing bar{nu}_{e} from galactic SN in massive water Cherenkov detectors by the charged current reactions on protons.

    Minakata, Hisakazu Nunokawa, Hiroshi Tomàs, Ricard Furtado Valle, José Wagner 2002 Probing supernova physics with neutrino oscillations Physics Letters B 542 3-4 239 244
http://dx.doi.org/10.1016/S0370-2693(02)02376-6
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