Linking solar and long baseline terrestrial neutrino experiments

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dc.creatorAkhmedov, E. Kh.
dc.creatorBranco, G. C.
dc.creatorRebelo, M. N.
dc.date1999-12-01
dc.date1999-12-04
dc.date.accessioned2026-07-07T10:53:16Z
dc.date.available2026-07-07T10:53:16Z
dc.descriptionWe show that in the framework of three light neutrino species with hierarchical masses and assuming no fine tuning between the entries of the neutrino mass matrix, one can use the solar neutrino data to obtain information on the element $U_{e3}$ of the lepton mixing matrix. Conversely, a measurement of $U_{e3}$ in atmospheric or long baseline accelerator or reactor neutrino experiments would help discriminate between possible oscillation solutions of the solar neutrino problem.
dc.descriptionrevtex, 4 pages, no figures. Discussion of the LOW solution modified; results unchanged. References added
dc.identifierhttps://arxiv.org/abs/hep-ph/9912205
dc.identifierhttp://arxiv.org/abs/hep-ph/9912205
dc.identifierPhys.Rev.Lett.84:3535,2000
dc.identifierdoi:10.1103/PhysRevLett.84.3535
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185424
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.titleLinking solar and long baseline terrestrial neutrino experiments
dc.typetext

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