Three flavor neutrino oscillation constraints from accelerator, reactor, atmospheric and solar neutrino experiments

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dc.creatorYasuda, Osamu
dc.creatorMinakata, Hisakazu
dc.date1996-02-24
dc.date.accessioned2026-07-07T03:58:55Z
dc.date.available2026-07-07T03:58:55Z
dc.descriptionWe discuss constraints on three flavor neutrino mixings from the accelerator and reactor experiments, the Kamiokande multi-GeV data, and the solar neutrino observations. The LSND result is excluded at 90\%CL by the constraints imposed by all the data of reactor and accelerator experiments and the Kamiokande multi-GeV data if the mass scale required for the solution to the solar neutrino problem is hierarchically small. The region of a set of the effective two-flavor mixing parameters ($Δm^2$, $\sin^22θ$) is given for the channel $ν_μ\rightarrowν_e$ which is allowed at 90\%CL by the multi-GeV Kamiokande data alone.
dc.descriptionLaTeX, 14 pages + 1 PostScript figure
dc.identifierhttps://arxiv.org/abs/hep-ph/9602386
dc.identifierhttp://arxiv.org/abs/hep-ph/9602386
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/46009
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThree flavor neutrino oscillation constraints from accelerator, reactor, atmospheric and solar neutrino experiments
dc.typetext

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