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  2. Cherenkov detector - Wikipedia

    en.wikipedia.org/wiki/Cherenkov_detector

    Cherenkov threshold detectors have been used for fast timing and time of flight measurements in particle detectors. More elaborate designs use the amount of light produced. Recording light from both primary and secondary particles, for a Cherenkov calorimeter the total light yield is proportional to the incident particle energy.

  3. Neutrino detector - Wikipedia

    en.wikipedia.org/wiki/Neutrino_detector

    Cherenkov radiation is produced whenever charged particles such as electrons or muons are moving through a given detector medium somewhat faster than the speed of light in that medium. In a Cherenkov detector, a large volume of clear material such as water or ice is surrounded by light-sensitive photomultiplier tubes.

  4. Accelerator Neutrino Neutron Interaction Experiment - Wikipedia

    en.wikipedia.org/wiki/Accelerator_Neutrino...

    The Accelerator Neutrino Neutron Interaction Experiment (ANNIE) is a water Cherenkov detector experiment designed to examine the nature of neutrino interactions. This experiment studies phenomena like proton decay, and neutrino oscillations, by analyzing neutrino interactions in gadolinium-loaded water and measuring their neutron yield.

  5. List of neutrino experiments - Wikipedia

    en.wikipedia.org/wiki/List_of_neutrino_experiments

    Cherenkov water detector NEVOD ATM, CR ν μ: ν μ + n → μ − + p ν μ + p → μ + + n: CC Water (H 2 O) Cherenkov: ≈2 GeV Moscow, Russia 1993– NEXT Neutrino Experiment with a Xenon Time Projection Chamber BB 136 Xe → 136 Ba + 2 e −: BB Gaseous Xenon Time projection chamber: ≈10 keV Canfranc, Spain 2016– NOνA: NuMI Off-Axis ...

  6. NEVOD - Wikipedia

    en.wikipedia.org/wiki/NEVOD

    NEVOD (Russian: НЕВОД, НЕйтринный ВОдный Детектор, Neutrino Water Detector; nevod means "dragnet" in Russian) is a neutrino detector and cosmic ray experiment that attempts to detect Cherenkov radiation arising from interactions between water and charged particles (mostly muons). It represents the first attempt to ...

  7. Pierre Auger Observatory - Wikipedia

    en.wikipedia.org/wiki/Pierre_Auger_Observatory

    Surface detector (SD) station, or 'tank', of the Pierre Auger Observatory. In 1967 University of Leeds had developed a water-Cherenkov detector (or surface station; a small water basin, 1.2 m deep; also called tank) and created a 12 km 2 detection area Haverah Park using 200 such tanks. They were arranged in groups of four in a triangular (Y ...

  8. Detection of internally reflected Cherenkov light - Wikipedia

    en.wikipedia.org/wiki/Detection_of_internally...

    In particle detectors a detection of internally reflected Cherenkov light (DIRC) detector measures the velocity of charged particles and is used for particle identification. It is a design of a ring imaging Cherenkov detector where Cherenkov light that is contained by total internal reflection inside the solid radiator has its angular ...

  9. Ring-imaging Cherenkov detector - Wikipedia

    en.wikipedia.org/.../Ring-imaging_Cherenkov_detector

    The ring-imaging detection technique was first proposed by Jacques Séguinot and Tom Ypsilantis, working at CERN in 1977. [1] Their research and development, of high precision single-photon detectors and related optics, lay the foundations for the design [2] [3] development [4] and construction of the first large-scale Particle Physics RICH detectors, at CERN's OMEGA facility [5] [6] [7] and ...