Future Solar Neutrino Experiments and Neutrino Spin-Flavour Precession

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dc.creatorBilenky, S. M.
dc.creatorGiunti, C.
dc.date1993-12-02
dc.date.accessioned2026-07-07T03:56:38Z
dc.date.available2026-07-07T03:56:38Z
dc.descriptionThe main features of the observables in the SNO and Super-Kamiokande solar neutrino experiments in the case of neutrino spin and/or spin-flavour precession in the magnetic field of the sun are discussed. It is shown without any model dependent assumption that in the case of Majorana transition magnetic moments the NC event rate $N^{\mathrm{NC}}$ does not depend on time and a measurement of $N^{\mathrm{NC}}$ will allow to determine the initial flux of $^8\mathrm{B}$ neutrinos with a theoretical uncertainty of a few \%. In the case of Dirac magnetic moments the NC event rate will depend on time and we obtain a model independent lower bound for the transition probability of initial $ν_e$'s into right-handed sterile neutrinos.
dc.descriptionDFTT 75/93. 11 pages, 1 figure (included). Compressed Postscript file. If you prefer the uncompressed postscript file or a hardcopy of the paper, please write to GIUNTI@TO.INFN.IT
dc.identifierhttps://arxiv.org/abs/hep-ph/9312211
dc.identifierhttp://arxiv.org/abs/hep-ph/9312211
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/45057
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleFuture Solar Neutrino Experiments and Neutrino Spin-Flavour Precession
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