Precision Measurement of Neutrino Oscillations
We precisely measure neutrino mixing angles and mass-squared differences at large-scale accelerator experiments to probe the origin of the matter–antimatter asymmetry of the universe.
We precisely measure neutrino mixing angles and mass-squared differences at large-scale accelerator experiments to probe the origin of the matter–antimatter asymmetry of the universe.
Using highly sensitive detectors installed deep underground, we search for direct interactions of dark matter (WIMPs), which are believed to account for approximately 27% of the mass of the universe.