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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 (sometimes referred to as the Davis experiment or Solar Neutrino Experiment and in original literature called Brookhaven Solar Neutrino Experiment or Brookhaven 37 Cl (Chlorine) Experiment) [1] was an experiment headed by astrophysicists Raymond Davis, Jr. and John N. Bahcall in the late 1960s.

  4. 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 ...

  5. Sudbury Neutrino Observatory - Wikipedia

    en.wikipedia.org/wiki/Sudbury_Neutrino_Observatory

    The neutrino is absorbed in the reaction and an electron is produced. Solar neutrinos have energies smaller than the mass of muons and tau leptons, so only electron neutrinos can participate in this reaction. The emitted electron carries off most of the neutrino's energy, on the order of 5–15 MeV, and is detectable. The proton which is ...

  6. Neutrinoless double beta decay - Wikipedia

    en.wikipedia.org/wiki/Neutrinoless_double_beta_decay

    The NuDoubt⁺⁺ experiment aims at the measurement of two-neutrino and neutrinoless positive double weak decays (2β⁺/ECβ⁺). [37] It is based on a new detector concept combining hybrid and opaque scintillators paired with a novel light read-out technique. [ 38 ]

  7. Helium and Lead Observatory - Wikipedia

    en.wikipedia.org/wiki/Helium_And_Lead_Observatory

    The idea of using lead to detect supernova neutrinos was originally proposed in 1996 by Cliff Hargrove as the "lead astronomical neutrino detector" (LAND), [7] and in 2004, Charles Duba, then a PhD student working on SNO, proposed re-using them for this purpose, prompting the renaming to HALO. Design of the current detector began in 2007.

  8. Gargamelle - Wikipedia

    en.wikipedia.org/wiki/Gargamelle

    Installation of the Gargamelle chamber body. Placement of the chamber in the oblong shaped magnet coils. The domain of neutrino physics was in rapid expansion in the 60's. . Neutrino experiments using bubble chambers were already running at the first synchrotron at CERN, the PS, and the question of the next generation of bubble chambers had been on the agenda for some ti

  9. Muon g-2 - Wikipedia

    en.wikipedia.org/wiki/Muon_g-2

    The next stage of muon g − 2 research was conducted at the Brookhaven National Laboratory (BNL) Alternating Gradient Synchrotron; the experiment was known as (BNL) Muon E821 experiment, [17] but it has also been called "muon experiment at BNL" or "(muon) g − 2 at BNL" etc. [7] Brookhaven's Muon g − 2 experiment was constructed from 1989 to 1996 and collected data from 1997 to 2001.