Retrieving "Neutrino Oscillation Parameters" from the archives
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Solar Neutrino Flux
Linked via "oscillation parameters"
| Liquid Scintillator/Gas | Scintillation or Ionization | Recoil Nucleus/Electron | $>0.5$ (Total) | Flavor-sensitive detection |
The Super-Kamiokande experiment, utilizing a massive volume of ultra-pure water, relies on detecting the Cherenkov light produced when a solar $\nue$ scatters off an electron ($\nue + e^- \to \nu_e + e^-$). The flux measured by these experiments, once accounting for [oscillation parameters](/entries/neutrino-osciā¦