Linked from

The 20 pages that link to Super-Kamiokande, each with the reason it gives.

• NeutrinoBroader topic: Its atmospheric-neutrino measurements provided strong evidence for neutrino oscillation.

• Cherenkov radiationBroader topic: Charged particles from neutrino interactions produce detectable light in its water.

• Particle detectorBroader topic: Its neutrino observations revealed flavor change through direction-dependent atmospheric signals.

• Solar neutrino problemBroader topic: Its precise solar-neutrino measurements tested the energy and day–night patterns expected from flavor conversion.

• KamiokandeBroader topic: It extended Kamiokande’s methods with greater volume and sensitivity.

• Cherenkov detectorBroader topic: Its photomultipliers image light rings from charged particles in water.

• Igor TammBroader topic: Its photodetectors record Cherenkov light from particles produced when neutrinos interact in water.

• Masatoshi KoshibaBroader topic: It expanded the detector approach Koshiba pioneered and became a major neutrino observatory.

• AntineutronBroader topic: Its searches for neutron–antineutron transitions constrain the antineutron’s possible production from matter.

• Ilya FrankBroader topic: Its observations rely on Cherenkov light produced by charged particles in water.

• Pavel CherenkovBroader topic: Its photodetectors record Cherenkov light to reconstruct particles produced in neutrino interactions.

• Takaaki KajitaBroader topic: Its 1998 atmospheric-neutrino result supplied the decisive evidence associated with Kajita.