This is a list of neutrino experiments, neutrino detectors, and neutrino telescopes. | Abbreviation | Full name | Sensitivity[a] | Type | Induced reaction | Type of reaction[b] | Detector | Type of detector | Threshold energy | Location | Operation | Home page | | ANTARES | Astronomy with a Neutrino Telescope and Abyss Environmental RESearch | | | | | | | | Mediterranean Sea, France | 2006– | [1] | | BOREXINO | BORon EXperiment | LS | νe | νx + e− → νx + e− | ES | LOS shielded by water | Scintillation | 250–665 keV | Gran Sasso, Italy | May 2007– | [2] [3] | | CLEAN | Cryogenic Low-Energy Astrophysics with Neon | LS, SN, WIMP | νe | νx + e− → νx + e− νe + 20Ne → νe + 20Ne | ES ES | Liquid Ne (10 t) | Scintillation | | | future | [4] | | Daya Bay | Daya Bay Reactor Neutrino Experiment | R | νe | νe + p → e+ + n | CC | Gd-doped LOS | Scintillation | 1.8 MeV | Daya Bay, China | 2009– | [5] | | Double CHOOZ | Double Chooz Reactor Neutrino Experiment | R | νe | νe + p → e+ + n | CC | Gd-doped LOS | Scintillation | 1.8 MeV | Chooz, France | 2008– | [6] | | EXO-200 | Enriched Xenon Observatory | | | | | | | | WIPP, New Mexico | 2009- | [7] | | GALLEX | GALLium EXperiment | LS | νe | νe + 71Ga → 71Ge + e− | CC | GaCl3 (30 t) | Radiochemical | 233.2 keV | Gran Sasso, Italy | 1991–1997 | [8] | | GNO | Gallium Neutrino Observatory | LS | νe | νe + 71Ga → 71Ge + e− | CC | GaCl3 (30 t) | Radiochemical | 233.2 keV | Gran Sasso, Italy | May 1998–Jan 2002 | [9] | | HERON | Helium Roton Observation of Neutrinos | LS | νe (mainly) | νe + e− → νe + e− | NC | Superfluid He | Rotational excitation | 1 MeV | | future | [10] | | HOMESTAKE–CHLORINE | Homestake chlorine experiment | S | νe | 37Cl + νe → 37Ar* + e− 37Ar* → 37Cl + e+ + νe | CC | C2Cl4 (615 t) | Radiochemical | 814 keV | Homestake Mine, South Dakota | 1967–1998 | [11] | | HOMESTAKE–IODINE | Homestake iodine experiment | S | νe | ν + e− → ν + e− νe + 127I → 127Xe + e− | ES CC | NaI in water | Radiochemical | 789 keV | Homestake Mine, South Dakota | future | [12] | | ICARUS | Imaging Cosmic And Rare Underground Signal | S, ATM, GSN | νe, νμ, ντ | ν + e− → ν + e− | ES | Liquid Ar | Cherenkov | 5.9 MeV | Gran Sasso, Italy | | [13] | | IceCube | IceCube Neutrino Detector | S, ATM, CR, ? | νe, νμ, ντ | ν + e− → ν + e− | ES | Water ice (1 km3) | Cherenkov | ~10 MeV | South Pole, Antarctica | 2006– | [14] | | Kamiokande | Kamioka Nucleon Decay Experiment | S, ATM | νe | ν + e− → ν + e− | ES | Water (H2O) | Cherenkov | 7.5 MeV | Kamioka, Japan | 1986–1995 | [15] | | KamLAND | Kamioka Liquid Scintillator Antineutrino Detector | | | | | | | | Kamioka, Japan | 2002– | [16] | | KM3NeT | KM3 Neutrino Telescope | | | | | | | | Mediterranean Sea, ? | 2009– | [17] | | LENS | Low Energy Neutrino Spectroscopy | LS | νe | νe + 115In → 115Sn + νe + 2γ | CC | In-doped LOS | Scintillation | 120 keV | | | [18] [19] | | Majorana | Neutrinoless Double Beta Decay in 76Ge to measure neutrino mass | | | | | | | | Homestake Mine, South Dakota | future (~2010) | [20] | | MOON | Molybdenum Observatory Of Neutrinos | LS, LSN | νe | νe + 100Mo → 100Tc + e− | CC | 100Mo (1 kt) + MoF6 (gas) | Scintillation | 168 keV | Washington, USA | | [21] | | MiniBooNE | Mini Booster Neutrino Experiment | AC | νe, νμ | νe + 12C → e− + X | CC | Mineral oil (1 kton) | Cherenkov | ~100 keV | Illinois,USA | 2002– | [22] | | NEMO Experiment | Neutrino Ettore Majorana Observatory | | | | | | | | Fréjus Road Tunnel, Italy/France | 2003– | [23] | | NEMO Telescope | NEutrino Mediterranean Observatory | | | | | | | | Mediterranean Sea, Italy | 2007– | [24] | | NOνA | NuMI Off-Axis νe Appearance | | | | | | | | Illinois and Minnesota,United States | 2011– | [25] | | OPERA | Oscillation Project with Emulsion-tRacking Apparatus | | ντ | | | | | | LNGS (Italy) and CERN | 2008– | [26] | | SAGE | Soviet–American Gallium Experiment | LS | νe | νe + 71Ga → 71Ge + e− | CC | GaCl3 | Radiochemical | 233.2 keV | Baksan Valley, Russia | 1990–2006 | [27] | | SNO | Sudbury Neutrino Observatory | S, ATM, GSN | νe, νμ, ντ | νe + 2D → 2p + e− νx + 2D → νx + n + p νe + e− → νe + e− | CC NC ES | Heavy water (1 kt D2O) | Cherenkov | 3.5 MeV | Creighton Mine, Ontario | 1999–2006 | [28] | | SNO+ | SNO with liquid scintillator | | | | | | | | Creighton Mine, Ontario | 2009– | [29] | | SK | Super-Kamiokande | S, ATM, GSN | νe, νμ, ντ | νe + e− → νe + e− νe + n → e− + p νe + p → e+ + n | ES CC CC | Water (H2O) | Cherenkov | | Kamioka, Japan | 1996– | [30] [31] | | UNO | Underground Nucleon decay and neutrino Observatory | S, ATM, GSN, RSN | νe, νμ, ντ | νe + e− → νe + e− | ES | Water (440 kt H2O) | Cherenkov | | Henderson Mine, Colorado | future | [32] | ^[a] Solar neutrino (S), Low-energy solar neutrino (LS), Reactor neutrino (R), Terrestrial neutrino (T), Atmospheric neutrino (ATM), Accelerator neutrino (AC), Cosmic ray neutrino (CR), Supernova neutrino (SN), Low-energy supernova neutrino (LSN), Active galactic nuclei neutrino (AGN), Pulsar neutrino (PUL) ^[b] Elastic scattering (ES), Neutral current (NC), Charged current (CC) [edit] See also | Neutrino detectors, experiments, and facilities | | | Operating | |  | | | Construction | | | | Retired | | | | Proposed | | | | Cancelled | | | | See also | List of neutrino experiments | | |