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Solar neutrino problem accounting for self-consistent magnetohydrodynamics solution for solar magnetic fields

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Solar neutrino problem accounting for self-consistent magnetohydrodynamics solution for solar magnetic fields

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dc.contributor.author	Rashba, Timur I.
dc.contributor.author	Miranda, O.G.
dc.contributor.author	Peña Garay, Carlos
dc.contributor.author	Semikoz, Victor B.
dc.contributor.author	Furtado Valle, José Wagner
dc.date.accessioned	2015-10-22T10:48:04Z
dc.date.available	2015-10-22T10:48:04Z
dc.date.issued	2001
dc.identifier.citation	Rashba, Timur I. Miranda, O.G. Peña Garay, Carlos Semikoz, Victor B. Furtado Valle, José Wagner 2001 Solar neutrino problem accounting for self-consistent magnetohydrodynamics solution for solar magnetic fields Nuclear Physics B-Proceedings Supplements 95 123 129
dc.identifier.uri	http://hdl.handle.net/10550/47851
dc.description.abstract	The analysis of the resonant spin-flavour (RSF) solutions to the solar neutrino problem in the framework of simplest analytic solutions to the solar magneto-hydrodynamics (MHD) equations is presented. We performed the global fit of the recent solar neutrino data, including event rates as well as day and night recoil electron spectra induced by solar neutrino interactions in SuperKamiokande. We compare quantitatively our simplest MHD-RSF fit with vacuum oscillation (VAC) and MSW--type (SMA, LMA and LOW) solutions to the solar neutrino problem using a common well-calibrated theoretical calculation and fit procedure and find MHD-RSF fit to be somewhat better than those obtained for the favored neutrino oscillation solutions. We made the predictions for future experiments to disentangle the MHD-RSF scenario from other scenarios.
dc.language.iso	eng
dc.relation.ispartof	Nuclear Physics B-Proceedings Supplements, 2001, vol. 95, p. 123-129
dc.subject	Física
dc.title	Solar neutrino problem accounting for self-consistent magnetohydrodynamics solution for solar magnetic fields
dc.type	journal article	es_ES
dc.date.updated	2015-10-22T10:48:04Z
dc.identifier.doi	10.1016/S0920-5632(01)01067-2
dc.identifier.idgrec	031787
dc.rights.accessRights	open access	es_ES