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Confronting spin flavor solutions of the solar neutrino problem with current and future solar neutrino data

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Confronting spin flavor solutions of the solar neutrino problem with current and future solar neutrino data

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dc.contributor.author Barranco, Juan
dc.contributor.author Miranda, O.G.
dc.contributor.author Rashba, Timur I.
dc.contributor.author Semikoz, Victor B.
dc.contributor.author Furtado Valle, José Wagner
dc.date.accessioned 2015-10-22T10:25:41Z
dc.date.available 2015-10-22T10:25:41Z
dc.date.issued 2002
dc.identifier.citation Barranco, Juan Miranda, O.G. Rashba, Timur I. Semikoz, Victor B. Furtado Valle, José Wagner 2002 Confronting spin flavor solutions of the solar neutrino problem with current and future solar neutrino data Physical Review D 66 9 093009
dc.identifier.uri http://hdl.handle.net/10550/47848
dc.description.abstract We show that spin flavor precession solutions to the solar neutrino problem, although preferred by the latest solar data, are ruled out by the first results from the KamLAND reactor experiment, at more than 3_sigma. An illustrative chi2 plot comparing these descriptions with oscillations is given.
dc.language.iso eng
dc.relation.ispartof Physical Review D, 2002, vol. 66, num. 9, p. 093009
dc.subject Física
dc.title Confronting spin flavor solutions of the solar neutrino problem with current and future solar neutrino data
dc.type journal article es_ES
dc.date.updated 2015-10-22T10:25:41Z
dc.identifier.doi 10.1103/PhysRevD.66.093009
dc.identifier.idgrec 031772
dc.rights.accessRights open access es_ES

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