Status of a hybrid three-neutrino interpretation of neutrino data
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Data
2002-05-13
Autores
Guzzo, M. M.
de Holanda, P. C.
Maltoni, M.
Nunokawa, H.
Tortola, M. A.
Valle, JWF
Título da Revista
ISSN da Revista
Título de Volume
Editor
Elsevier B.V.
Resumo
We re-analyse the non-standard interaction (NSI) solutions to the solar neutrino problem in the light of the latest solar as well as atmospheric neutrino data. The latter require oscillations (OSC), while the former do not. Within such a three-neutrino framework the solar and atmospheric neutrino sectors are connected not only by the neutrino mixing angle theta(13) constrained by reactor and atmospheric data, but also by the flavour-changing (FC) and non-universal (NU) parameters accounting for the solar data. Since the NSI solution is energy-independent the spectrum is undistorted, so that the global analysis observables are the solar neutrino rates in all experiments as well as the Super-Kamiokande day-night measurements. We find that the NSI description of solar data is slightly better than that of the OSC solution and that the allowed NSI regions are determined mainly by the rate analysis. By using a few simplified ansatzes for the NSI interactions we explicitly demonstrate that the NSI values indicated by the solar data analysis are fully acceptable also for the atmospheric data. (C) 2002 Elsevier B.V. B.V. All rights reserved.
Descrição
Palavras-chave
neutrino oscillations, solar and atmospheric neutrinos, neutrino mass and mixing, non-standard neutrino interactions
Como citar
Nuclear Physics B. Amsterdam: Elsevier B.V., v. 629, n. 1-3, p. 479-490, 2002.