Neutrino oscillations in the earth suggest a terrestrial test of solution to solar neutrino problem

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Earth Atmosphere, Neutrinos, Oscillations, Solar Neutrinos, Annual Variations, Diurnal Variations, Particle Production, Radiation Detectors, Underground Structures

Scientific paper

It is generally believed that a complete spectroscopy of solar neutrinos, which is far from being achieved in the near future, is required in order to verify the Mikheyev-Smirnov-Wolfenstein (MSW) solution of the solar neutrino problem and to unfold the values of neutrino masses and mixings that nature has selected. However, the authors show here that the MSW solution of the solar neutrino problem can be tested with present equipment - the 'Bethe solution' yields sizeable oscillations of atmospheric neutrinos in the Earth which can be detected with the massive underground proton decay detectors, while the 'Rosen-Gelb' additional solutions yield diurnal and seasonal modulations of the solar neutrino flux which perhaps can be detected by the radio-chemical Cl and Ga detectors.

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