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Probing supernova physics with neutrino oscillations

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Probing supernova physics with neutrino oscillations

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dc.contributor.author Minakata, Hisakazu
dc.contributor.author Nunokawa, Hiroshi
dc.contributor.author Tomàs, Ricard
dc.contributor.author Furtado Valle, José Wagner
dc.date.accessioned 2015-10-22T10:28:33Z
dc.date.available 2015-10-22T10:28:33Z
dc.date.issued 2002
dc.identifier.citation 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
dc.identifier.uri http://hdl.handle.net/10550/47849
dc.description.abstract 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.
dc.language.iso eng
dc.relation.ispartof Physics Letters B, 2002, vol. 542, num. 3-4, p. 239-244
dc.subject Física
dc.title Probing supernova physics with neutrino oscillations
dc.type journal article es_ES
dc.date.updated 2015-10-22T10:28:34Z
dc.identifier.doi 10.1016/S0370-2693(02)02376-6
dc.identifier.idgrec 031776
dc.rights.accessRights open access es_ES

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