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arXiv · hep-ph/9902261

Implications of Super-Kamiokande atmospheric low-energy data for solar neutrino oscillations

C. Giunti·C. W. Kim·U. W. Lee·V. A. Naumov
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Abstract

It is shown that the high-Delta m^2 part of the large mixing angle MSW solution of the solar neutrino problem is disfavored by the Super-Kamiokande data for low-energy upward-going events. A quantitative bound is obtained in the three-neutrino scheme with a negligibly small element U_{e3} of the neutrino mixing matrix, as indicated by the result of the CHOOZ long-baseline antinu_e->antinu_e oscillation experiment.

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C. Giunti, C. W. Kim, U. W. Lee, V. A. Naumov. 1999-02-11. Implications of Super-Kamiokande atmospheric low-energy data for solar neutrino oscillations. https://arxiv.org/abs/hep-ph/9902261

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