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What is Neutrino Oscillations and Solar Problem about?

The document discusses the Mikheyev-Smirnov-Wolfenstein (MSW) solution to the solar-neutrino problem, identifying three classes of neutrino oscillation parameters that could explain the observed deficit of solar neutrinos. It highlights that while the gallium solar-neutrino experiment can test two of these alternatives, the third could lead to detectable oscillations of atmospheric neutrinos on Earth. The authors present analytical and numerical methods to solve neutrino propagation equations, supporting th

Author

sbsatyabrata07

Language

EN