Linked from

The 24 pages that link to Cherenkov radiation, each with the reason it gives.

• Cosmic rayRelated: Relativistic shower particles produce brief Cherenkov flashes observed by ground telescopes.

• Neutrino astronomyRelated: Neutrino detectors use this light to record charged particles produced by neutrino interactions.

• Phase velocityRelated: The relevant threshold compares particle speed with phase speed, not vacuum light speed.

• Group velocityRelated: The condition compares particle speed with phase velocity, not group velocity.

• Super-KamiokandeRelated: Charged particles from neutrino interactions produce the light recorded by the detector.

• IceCube Neutrino ObservatoryRelated: Charged particles from neutrino interactions emit the blue light IceCube’s sensors detect.

• Dispersion relationRelated: The medium’s dispersion relation sets the phase-speed threshold for emission.

• Sudbury Neutrino ObservatoryRelated: Photomultiplier tubes recorded Cherenkov light from charged particles produced in SNO’s reactions.

• KamiokandeRelated: Charged particles from neutrino interactions produced the light Kamiokande recorded.

• Particle identificationRelated: Its emission threshold and angle reveal particle velocity.

• Masatoshi KoshibaRelated: Neutrino interactions in water can produce charged particles whose Cherenkov light reveals their passage.

• Takaaki KajitaRelated: Water-Cherenkov detectors identify neutrino interactions through the light patterns charged particles leave behind.

• High-energy astrophysicsRelated: Ground-based gamma-ray telescopes detect brief Cherenkov flashes from atmospheric particle showers.

• Cosmic rays and astroparticlesRelated: Air-shower telescopes use its brief flashes to reconstruct particle cascades.