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  2. Irvine–Michigan–Brookhaven (detector) - Wikipedia

    en.wikipedia.org/wiki/Irvine–Michigan...

    IMB, the Irvine-Michigan-Brookhaven detector, was a nucleon decay experiment and neutrino observatory located in a Morton Salt company's Fairport mine on the shore of Lake Erie in the United States 600 meters underground. It was a joint venture of the University of California, Irvine, the University of Michigan, and the Brookhaven National ...

  3. Homestake experiment - Wikipedia

    en.wikipedia.org/wiki/Homestake_experiment

    The Homestake experiment was followed by other experiments with the same purpose, such as Kamiokande in Japan, SAGE in the former Soviet Union, GALLEX in Italy, Super Kamiokande, also in Japan, and SNO (Sudbury Neutrino Observatory) in Ontario, Canada. SNO was the first detector able to detect neutrino oscillation, solving the solar neutrino ...

  4. Raymond Davis Jr. - Wikipedia

    en.wikipedia.org/wiki/Raymond_Davis_Jr.

    Raymond Davis Jr. (October 14, 1914 – May 31, 2006) was an American chemist and physicist.He is best known as the leader of the Homestake experiment in the 1960s-1980s, which was the first experiment to detect neutrinos emitted from the Sun; for this he shared the 2002 Nobel Prize in Physics.

  5. Mary Bishai - Wikipedia

    en.wikipedia.org/wiki/Mary_Bishai

    Mary R. M. Bishai (born 1970) is an American physicist who is a Distinguished Scientist at Brookhaven National Laboratory.In 2023, she was elected spokesperson of Deep Underground Neutrino Experiment, and was made responsible for the 1,400 person collaboration.

  6. List of neutrino experiments - Wikipedia

    en.wikipedia.org/wiki/List_of_neutrino_experiments

    Daya Bay Reactor Neutrino Experiment R ν e: ν e + p → e + + n: CC Gd-doped LAB Scintillation: 1.8 MeV Daya Bay, China 2011–2020 Double Chooz: Double Chooz Reactor Neutrino Experiment R ν e: ν e + p → e + + n: CC Gd-doped LOS: Scintillation: 1.8 MeV Chooz, France 2011–2017 DUNE: Deep Underground Neutrino Experiment AC, ATM, (S), SN ...

  7. SuperNova Early Warning System - Wikipedia

    en.wikipedia.org/wiki/Supernova_Early_Warning_System

    The SuperNova Early Warning System (SNEWS) is a network of neutrino detectors designed to give early warning to astronomers in the event of a supernova in the Milky Way, our home galaxy, or in a nearby galaxy such as the Large Magellanic Cloud or the Canis Major Dwarf Galaxy. As of March 2021, [1] SNEWS has not issued any supernova alerts.

  8. Kamioka Liquid Scintillator Antineutrino Detector - Wikipedia

    en.wikipedia.org/wiki/Kamioka_Liquid_Scintillat...

    The Kamioka Liquid Scintillator Antineutrino Detector (KamLAND) is an electron antineutrino detector at the Kamioka Observatory, an underground neutrino detection facility in Hida, Gifu, The device is situated in a drift mine shaft in the old KamiokaNDE cavity in the Japanese Alps .

  9. K2K experiment - Wikipedia

    en.wikipedia.org/wiki/K2K_experiment

    The K2K experiment (KEK to Kamioka) was a neutrino experiment that ran from June 1999 to November 2004. It used muon neutrinos from a well-controlled and well-understood beam to verify the oscillations previously observed by Super-Kamiokande using atmospheric neutrinos .

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