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Confronting Spin Flavor Solutions of the Solar Neutrino Problem with current and future solar neutrino data

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arxiv hep-ph/0207326 v3 pith:FD4537E6 submitted 2002-07-26 hep-ph

J. Barranco , O.G. Miranda , T.I. Rashba , V.B. Semikoz , J.W.F. Valle This is my paper · ORCID
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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.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Neutrino electromagnetic properties and sterile dipole portal in light of the first solar CE$\nu$NS data

    hep-ph 2024-12 conditional novelty 6.0 of 10

    The paper derives the first 90% CL limits on neutrino magnetic moments, millicharges, and the sterile dipole portal from solar 8B CEνNS data in XENONnT and PandaX-4T.

  2. 2020 Global reassessment of the neutrino oscillation picture

    hep-ph 2020-06 unverdicted novelty 3.0 of 10

    Updated global fit of neutrino oscillation data gives precise measurements of mixing parameters with a 2.5 sigma preference for normal mass ordering.

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