Time variations of solar neutrino signals and the RSFCN hypothesis

Resonant spin--flavour conversion of neutrinos (RSFCN) in twisting magnetic fields might be at the origin of the apparent anticorrelation between the $^{37}$Ar production--rate in the Homestake solar neutrino detector and the solar activity. Moreover, it can account for the results of all solar neut...

Descripción completa

Detalles Bibliográficos
Autor principal: Krastev, P.I.
Lenguaje:eng
Publicado: 1993
Materias:
Particle Physics - Phenomenology
Acceso en línea:https://dx.doi.org/10.1016/0370-2693(93)90046-K
http://cds.cern.ch/record/243888
_version_ 1780885116489302016
author Krastev, P.I.
author_facet Krastev, P.I.
author_sort Krastev, P.I.
collection CERN
description Resonant spin--flavour conversion of neutrinos (RSFCN) in twisting magnetic fields might be at the origin of the apparent anticorrelation between the $^{37}$Ar production--rate in the Homestake solar neutrino detector and the solar activity. Moreover, it can account for the results of all solar neutrino experiments reported so far including the recent results of GALLEX and SAGE.
id cern-243888
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1993
record_format invenio
spelling cern-2438882023-03-14T20:45:53Zdoi:10.1016/0370-2693(93)90046-Khttp://cds.cern.ch/record/243888engKrastev, P.I.Time variations of solar neutrino signals and the RSFCN hypothesisParticle Physics - PhenomenologyResonant spin--flavour conversion of neutrinos (RSFCN) in twisting magnetic fields might be at the origin of the apparent anticorrelation between the $^{37}$Ar production--rate in the Homestake solar neutrino detector and the solar activity. Moreover, it can account for the results of all solar neutrino experiments reported so far including the recent results of GALLEX and SAGE.Resonant spin--flavour conversion of neutrinos (RSFCN) in twisting magnetic fields might be at the origin of the apparent anticorrelation between the $~{37}$Ar production--rate in the Homestake solar neutrino detector and the solar activity. Moreover, it can account for the results of all solar neutrino experiments reported so far including the recent results of GALLEX and SAGE.Resonant spin--flavour conversion of neutrinos (RSFCN) in twisting magnetic fields might be at the origin of the apparent anticorrelation between the $~{37}$Ar production--rate in the Homestake solar neutrino detector and the solar activity. Moreover, it can account for the results of all solar neutrino experiments reported so far including the recent results of GALLEX and SAGE.Resonant spin-flavour conversion of neutrinos (RSFCN) in twisting magnetic fields might be at the origin of the apparent anticorrelation between the 37 Ar production rate in the Homestake solar neutrino detector and the solar activity. Moreover, it can account for the results of all solar neutrino experiments reported so far including the recent results of GALLEX and SAGE.hep-ph/9211293CERN-TH-6648-92IFP-458-UNCCERN-TH-6648-92IFP-458-UNCoai:cds.cern.ch:2438881993
spellingShingle Particle Physics - Phenomenology
Krastev, P.I.
Time variations of solar neutrino signals and the RSFCN hypothesis
title Time variations of solar neutrino signals and the RSFCN hypothesis
title_full Time variations of solar neutrino signals and the RSFCN hypothesis
title_fullStr Time variations of solar neutrino signals and the RSFCN hypothesis
title_full_unstemmed Time variations of solar neutrino signals and the RSFCN hypothesis
title_short Time variations of solar neutrino signals and the RSFCN hypothesis
title_sort time variations of solar neutrino signals and the rsfcn hypothesis
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/0370-2693(93)90046-K
http://cds.cern.ch/record/243888
work_keys_str_mv AT krastevpi timevariationsofsolarneutrinosignalsandthersfcnhypothesis

Ejemplares similares