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Probing supernova physics with neutrino oscillations

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Probing supernova physics with neutrino oscillations

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.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.rights.uri	info:eu-repo/semantics/openAccess
dc.source	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.subject	Física
dc.title	Probing supernova physics with neutrino oscillations
dc.type	info:eu-repo/semantics/article
dc.date.updated	2015-10-22T10:28:34Z
dc.identifier.doi	http://dx.doi.org/10.1016/S0370-2693(02)02376-6
dc.identifier.idgrec	031776