This is a non-exhaustive list of neutrino experiments, neutrino detectors, and neutrino telescopes.
| Abbreviation | Full name | Sensitivity[a] | Type of reaction[b] | Detector | Type of detector | Threshold energy | Location | Operation | ||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| ANNIE | Accelerator Neutrino Neutron Interaction Experiment | SciBooNE Hall, Illinois, United States | future | |||||||||
| ANTARES | Astronomy with a Neutrino Telescope and Abyss Environmental RESearch | ATM, CR, AGN, PUL | Mediterranean Sea, France | 2006– | ||||||||
| ARIANNA | Antarctic Ross Ice-Shelf ANtenna Neutrino Array | S, CR, AGN, ? | Ross Ice Shelf, Antarctica | future | ||||||||
| BDUNT (NT-200+) | Baikal Deep Underwater Neutrino Telescope | S, ATM, LS, AGN, PUL | CC, NC | Water (H2O) | Cherenkov | ≈10 GeV | Lake Baikal, Russia | 1993– | ||||
| BOREXINO | BORon EXperiment | LS | ES | LOS shielded by water | Scintillation | 250–665 keV | Gran Sasso, Italy | May 2007– | ||||
| CHANDLER | Carbon Hydrogen AntiNeutrino Detector with a Lithium Enhanced Roghavan-optical-lattice | R | CC | WLS Plastic Scintillating Cubes and Lithium-6-loaded Zinc Sulfide Sheets | Scintillation | 1.8 MeV | North Anna, Virginia, USA | June 2017- | ||||
| CLEAN | Cryogenic Low-Energy Astrophysics with Neon | LS, SN, WIMP | ES ES |
Liquid Ne (10 t) | Scintillation | future | ||||||
| COBRA | Cadmium zinc telluride 0-neutrino double-Beta Research Apparatus | BB | Cadmium zinc telluride | Gran Sasso, Italy | 2007– | |||||||
| COHERENT | COHERENT | AC | NC | CsI[Na], NaI[Tl], HPGe, LAr | Coherent Elastic Neutrino Nucleus Scattering (CEvNS) | few keV nuclear recoil energy | Spallation Neutron Source at Oak Ridge National Laboratory | Nov 2016- | ||||
| Daya Bay | Daya Bay Reactor Neutrino Experiment | R | CC | Gd-doped LAB (LOS) | Scintillation | 1.8 MeV | Daya Bay, China | 2011– | ||||
| Double Chooz | Double Chooz Reactor Neutrino Experiment | R | CC | Gd-doped LOS | Scintillation | 1.8 MeV | Chooz, France | 2011– | ||||
| DUNE | Deep Underground Neutrino Experiment | Liquid argon | Scintillation | Homestake Mine (South Dakota) | construction start 2017 | |||||||
| EXO-200 | Enriched Xenon Observatory | BB | Liquid Xenon | WIPP, New Mexico | 2009– | |||||||
| GALLEX | GALLium EXperiment | LS | CC | GaCl3 (30 t) | Radiochemical | 233.2 keV | Gran Sasso, Italy | 1991–1997 | ||||
| GERDA | The GERmanium Detector Array | BB | BB | HPGe | Semiconductor | Gran Sasso, Italy | ||||||
| GNO | Gallium Neutrino Observatory | LS | CC | GaCl3 (30 t) | Radiochemical | 233.2 keV | Gran Sasso, Italy | May 1998–Apr 2003 | ||||
| GRAND | Giant Radio Array for Neutrino Detection | AGN, CR, ? | CC | Electromagnetic waves caused by τ− through extensive air showers in the atmosphere. |
Radio | 1017 eV | China | Proposed | ||||
| HALO | Helium And Lead Observatory | SN | CC, NC | Lead (79 t) and 3He | High-Z | ≈10 MeV | Creighton Mine, Ontario | 2012– | ||||
| HERON | Helium Roton Observation of Neutrinos | LS | NC | Superfluid He | Rotational excitation | 1 MeV | future | |||||
| HOMESTAKE–CHLORINE | Homestake chlorine experiment | S | CC | C2Cl4 (615 t) | Radiochemical | 814 keV | Homestake Mine, South Dakota | 1967–1998 | ||||
| HOMESTAKE–IODINE | Homestake iodine experiment | S | ES CC |
NaI in water | Radiochemical | 789 keV | Homestake Mine, South Dakota | future | ||||
| Hyper-Kamiokande | Hyper-Kamiokande | S, ATM, SN, AC | ES, CC, (NC) | water | Cherenkov | 200 MeV | Tokai and Kamioka, Japan | 2027- (under construction) |
||||
| ICARUS | Imaging Cosmic And Rare Underground Signal | S, ATM, GSN | ES | Liquid Ar | Cherenkov | 5.9 MeV | Gran Sasso, Italy | 2010– | ||||
| IceCube | IceCube Neutrino Detector | ATM, CR, AGN, ? | CC, NC | Water ice (1 km3) | Cherenkov | ≈10 GeV | South Pole, Antarctica | 2006– | ||||
| India-based Neutrino Observatory | Iron Calorimeter Detector @ India-based Neutrino Observatory | ATM | CC (dominant), NC | Magnetised iron (50 kton) | RPC active detector elements | ≈0.6 GeV | Theni, Tamil Nadu, India | 2012– (lab construction); 2018– (detector operation)
NOTE: Many social movements would potentially stop this construction. |
||||
| JUNO | Jiangmen Underground Neutrino Observatory | R | CC | LAB (LOS) + PPO + Bis-MSB | Scintillation | Kaiping, China | 2014– (construction) | |||||
| Kamiokande | Kamioka Nucleon Decay Experiment | S, ATM | ES | Water (H2O) | Cherenkov | 7.5 MeV | Kamioka, Japan | 1986–1995 | ||||
| KamLAND | Kamioka Liquid Scintillator Antineutrino Detector | R | CC | LOS | Scintillation | 1.8 MeV | Kamioka, Japan | 2002– | ||||
| KM3NeT | KM3 Neutrino Telescope | S, ATM, CR, SN, AGN, PUL | Sea water (≈5 km3) | Cherenkov | Mediterranean Sea | 2014– | ||||||
| LAGUNA | Large Apparatus studying Grand Unification and Neutrino Astrophysics | future | ||||||||||
| LENS | Low Energy Neutrino Spectroscopy | LS | CC | In-doped LOS | Scintillation | 120 keV | ||||||
| Majorana Demonstrator | The Majorana Demonstrator | BB | BB | HPGe | Semiconductor | 2039 keV | Homestake Mine, South Dakota | construction start 2012 | ||||
| MicroBooNE | AC, SN | ES, NC, CC | Liquid Argon | TPC | few MeV | Illinois, United States | 2014- | |||||
| MINERvA | Main Injector ExpeRiment for v-A | AC | CC, NC | Solid scintillator, targets of Liquid helium, Carbon, Water, Iron, Lead | Scintillation | ≈0.5 GeV | Illinois, United States | 2009– | ||||
| MiniBooNE | Mini Booster Neutrino Experiment | AC | CC | Mineral oil (1000 t) | Cherenkov | ≈100 keV | Illinois, United States | 2002– | ||||
| MINOS | Main Injector Neutrino Oscillation Search | AC, ATM | CC, NC | Solid scintillator | Scintillation | ≈0.5 GeV | Illinois and Minnesota, United States | 2005–2012 | ||||
| MINOS+ | Upgraded electronics for MINOS | AC, ATM | CC, NC | Solid scintillator | Scintillation | ≈0.5 GeV | Illinois and Minnesota, United States | 2013– | ||||
| NEMO-3 | Neutrino Ettore Majorana Observatory | BB | BB | Tracker + calorimeter | He+Ar wire chamber, plastic scintillators | 150 keV | Modane Underground Laboratory, Fréjus Road Tunnel, France | 2003–2011 | ||||
| MOON | Molybdenum Observatory Of Neutrinos | LS, LSN | CC | 100 Mo (1 kt) + MoF6 (gas) |
Scintillation | 168 keV | Washington, United States | |||||
| NEMO Telescope | NEutrino Mediterranean Observatory | Mediterranean Sea, Italy | 2007– | |||||||||
| NEVOD | Cherenkov water detector NEVOD | ATM, CR | CC | Water (H2O) | Cherenkov | ≈2 GeV | Moscow, Russia | 1993– | ||||
| NEXT | Neutrino Experiment with a Xenon Time Projection Chamber | BB | BB | Gaseous Xenon | Time projection chamber | ≈10 keV | Canfranc, Spain | 2016– | ||||
| NOνA | NuMI Off-Axis νe Appearance | AC | CC | Liquid scintillator | Scintillation | ≈0.1 GeV | Illinois and Minnesota, United States | 2011– | ||||
| OPERA | Oscillation Project with Emulsion-tRacking Apparatus | AC | CC | Lead/Emulsion | Nuclear Emulsion | ≈1.0 GeV | LNGS (Italy) and CERN | 2008– | ||||
| Auger | Pierre Auger Observatory | CR | Cherenkov | Argentina | ||||||||
| RENO | Reactor Experiment for Neutrino Oscillation | R | CC | Gd-doped LOS | Scintillation | 1.8 MeV | South Korea | 2011– | ||||
| SAGE | Soviet–American Gallium Experiment | LS | CC | Ga (metallic) | Radiochemical | 233.2 keV | Baksan River valley, Russia | 1989– | ||||
| SciBooNE | SciBar (Scintillator Bar) Booster Neutrino Experiment | AC | CC, NC | Plastic (CH,10 ton) | Scintillation | ≈100 keV | Illinois, United States | 2007–2008 | ||||
| SNO | Sudbury Neutrino Observatory | S, ATM, GSN | CC NC ES |
Heavy water (1 kt D2O) | Cherenkov | 3.5 MeV | Creighton Mine, Ontario | 1999–2006 | ||||
| SNO+ | SNO with liquid scintillator | S,LS,R,T,
SN,LSN |
ES, BB | linear alkylbenzene (LAB) + PPO | Scintillation | ≈≤1MeV | Creighton Mine, Ontario | 2014– | ||||
| SoLid | Short baseline Oscillation Search with Lithium-6 Detector | R | CC | plastic and anorganic scintillator | Scintillation | ≈2 MeV | Mol, Belgium | 2015- | ||||
| STEREO | STErile neutrino REactor Oscillation experiment | R | CC | liquid organic scintillator loaded with Gd | Scintillation | ≈2 MeV | Grenoble, France | 2013- | ||||
| Super-K | Super-Kamiokande | S, ATM, GSN | ES CC CC |
Water (H2O) | Cherenkov | 200 MeV | Kamioka, Japan | 1996– | ||||
| SuperNEMO | SuperNEMO | BB | BB | Tracker + calorimeter | He+Ar wire chamber, plastic scintillators | 150 keV | Modane Underground Laboratory, Fréjus Road Tunnel, France | 2017- | ||||
| T2K | Tokai to Kamioka | AC | CC
(NC) |
Water (H2O) | Cherenkov |
|
Tokai, Japan Kamioka, Japan | 2011- | ||||
| UNO | Underground Nucleon decay and neutrino Observatory | S, ATM, GSN, RSN | ES | Water (440 kt H2O) | Cherenkov | Henderson Mine, Colorado | future | |||||
| ENUBET | Enhanced NeUtrino BEams from kaon Tagging | AC | CC
(NC) |
^[a] Accelerator neutrino (AC), Active galactic nuclei neutrino (AGN), Atmospheric neutrino (ATM), Cosmic ray neutrino (CR), Low-energy solar neutrino (LS), Low-energy supernova neutrino (LSN), Pulsar neutrino (PUL), Reactor neutrino (R), Solar neutrino (S), Supernova neutrino (SN), Terrestrial neutrino (T).
^[b] Double beta decay (BB), Charged current (CC), Elastic scattering (ES), Neutral current (NC).
See also
Aspera European Astroparticle network[icon]
"Experiments". Neutrino Unbound. Istituto Nazionale di Fisica Nucleare. 24 February 2017. Retrieved 2017-02-28. Regularly updated index of neutrino physics research.
Hellenica World - Scientific Library
Retrieved from "http://en.wikipedia.org/"
All text is available under the terms of the GNU Free Documentation License
