List of neutrino experiments
This is a non-exhaustive 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 | |||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
ANNIE | Accelerator Neutrino Neutron Interaction Experiment | SciBooNE Hall, Illinois, USA | future | |||||||||||
ANTARES | Astronomy with a Neutrino Telescope and Abyss Environmental RESearch | ATM, CR, AGN, PUL | ν e, ν μ, ν τ |
Mediterranean Sea, France | 2006– | |||||||||
ARIANNA | Antarctic Ross Ice-Shelf ANtenna Neutrino Array | S, CR, AGN, ? | ν e, ν μ, ν τ |
Ross Ice Shelf, Antarctica | future | |||||||||
BDUNT (NT-200+) | Baikal Deep Underwater Neutrino Telescope | S, ATM, LS, AGN, PUL | ν e, ν μ, ν τ |
CC, NC | Water (H2O) | Cherenkov | ~10 GeV | Lake Baikal, Russia | 1993– | |||||
BOREXINO | BORon EXperiment | LS | ν e |
νx + e− → νx + e− | ES | LOS shielded by water | Scintillation | 250–665 keV | Gran Sasso, Italy | May 2007– | ||||
CLEAN | Cryogenic Low-Energy Astrophysics with Neon | LS, SN, WIMP | ν e |
νx + e− → νx + e− ν |
ES ES |
Liquid Ne (10 t) | Scintillation | future | ||||||
COBRA | Cadmium zinc telluride 0-neutrino double-Beta Research Apparatus | 64Zn + e− → 64Ni + e+ 70Zn → 70Ge + e− + e− 106Cd → 106Pd + e+ + e+ 108Cd + e− + e− → 108Pd 114Cd → 114Sn + e− + e− 116Cd → 116Sn + e− + e− 120Te + e− → 120Sn + e+ 128Te → 128Xe + e− + e− 130Te → 130Xe + e− + e− |
BB | Cadmium zinc telluride | Gran Sasso, Italy | 2007– | ||||||||
Daya Bay | Daya Bay Reactor Neutrino Experiment | R | ν e |
ν e + p → e+ + n |
CC | Gd-doped LAB (LOS) | Scintillation | 1.8 MeV | Daya Bay, China | 2011– | ||||
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– | ||||
EXO-200 | Enriched Xenon Observatory | 134Xe → 134Ba + e− + e− 136Xe → 136Ba + e− + e− |
BB | Liquid Xenon | WIPP, New Mexico | 2009– | ||||||||
GALLEX | GALLium EXperiment | LS | ν e |
ν e + 71Ga → 71Ge + e− |
CC | GaCl3 ( t) 30 | Radiochemical | 233.2 keV | Gran Sasso, Italy | 1991–1997 | ||||
GERDA | The GERmanium Detector Array | BB | ν e |
76Ge → 76As + e− + e− | BB | HPGe | Semiconductor | Gran Sasso, Italy | ||||||
GNO | Gallium Neutrino Observatory | LS | ν e |
ν e + 71Ga → 71Ge + e− |
CC | GaCl3 ( t) 30 | Radiochemical | 233.2 keV | Gran Sasso, Italy | May 1998–Jan 2002 | ||||
HALO | Helium And Lead Observatory | SN | ν e, νx |
ν e + 208Pb → e− + 209Bi* ν + 208Pb → ν + 208Pb* |
CC, NC | Lead ( t) and 793He | High-Z | ~10 MeV | Creighton Mine, Ontario | 2012– | ||||
HERON | Helium Roton Observation of Neutrinos | LS | ν e (mainly) |
ν e + e− → ν e + e− |
NC | Superfluid He | Rotational excitation | 1 MeV | future | |||||
HOMESTAKE–CHLORINE | Homestake chlorine experiment | S | ν e |
37Cl + ν e → 37Ar* + e− 37Ar* → 37Cl + e+ + ν e |
CC | C2Cl4 ( t) 615 | Radiochemical | 814 keV | Homestake Mine, South Dakota | 1967–1998 | ||||
HOMESTAKE–IODINE | Homestake iodine experiment | S | ν e |
ν + e− → ν + e− ν e + 127I → 127Xe + e− |
ES CC |
NaI in water | Radiochemical | 789 keV | Homestake Mine, South Dakota | future | ||||
ICARUS | Imaging Cosmic And Rare Underground Signal | S, ATM, GSN | ν e, ν μ, ν τ |
ν + e− → ν + e− | ES | Liquid Ar | Cherenkov | 5.9 MeV | Gran Sasso, Italy | 2010– | ||||
IceCube | IceCube Neutrino Detector | ATM, CR, AGN, ? | ν e, ν μ, ν τ |
ν + N → ν + Cascade , ν + N → Charged lepton + Cascade | 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 | ν μ |
ν μ+Fe→μ−+X |
CC (dominant), NC | Magnetised iron (50 kton) | RPC active detector elements | ~0.6 GeV | Theni, Tamil Nadu, India | 2012– (lab construction); 2018– (detector operation) | ||||
JUNO | Jiangmen Underground Neutrino Observatory | R | ν e |
ν e + p → e+ + n |
CC | LAB (LOS) + PPO + Bis-MSB | Scintillation | Kaiping, China | 2014– (construction) | |||||
Kamiokande | Kamioka Nucleon Decay Experiment | S, ATM | ν e |
ν + e− → ν + e− | ES | Water (H2O) | Cherenkov | 7.5 MeV | Kamioka, Japan | 1986–1995 | ||||
KamLAND | Kamioka Liquid Scintillator Antineutrino Detector | R | ν e |
ν e + p → e+ + n |
CC | LOS | Scintillation | 1.8 MeV | Kamioka, Japan | 2002– | ||||
KM3NeT | KM3 Neutrino Telescope | S, ATM, CR, SN, AGN, PUL | ν μ,ν e,ν τ |
Sea water (~5 km3) | Cherenkov | Mediterranean Sea | ||||||||
LAGUNA | Large Apparatus studying Grand Unification and Neutrino Astrophysics | future | ||||||||||||
LBNE/DUNE | Long-Baseline Neutrino Experiment / Deep Underground Neutrino Experiment | Homestake Mine (South Dakota) | future | |||||||||||
LENS | Low Energy Neutrino Spectroscopy | LS | ν e |
ν e + 115In → 115Sn + ν e + 2γ |
CC | In-doped LOS | Scintillation | 120 keV | ||||||
Majorana Demonstrator | The Majorana Demonstrator | BB | ν e |
76Ga → 76As + e− + e− | BB | HPGe | Semiconductor | 2039 keV | Homestake Mine, South Dakota | construction start 2012 | ||||
MicroBooNE | AC, SN | ν e, ν μ |
ES, NC, CC | Liquid Argon | TPC | few MeV | Illinois, USA | 2014 | ||||||
MINERvA | Main Injector ExpeRiment for v-A | AC | ν μ |
many | CC, NC | Solid scintillator, targets of Liquid helium, Carbon, Water, Iron, Lead | Scintillation | ~0.5 GeV | Illinois, USA | 2009– | ||||
MiniBooNE | Mini Booster Neutrino Experiment | AC | ν e, ν μ |
ν e + 12C → e− + X |
CC | Mineral oil ( t) 1000 | Cherenkov | ~100 keV | Illinois, USA | 2002– | ||||
MINOS | Main Injector Neutrino Oscillation Search | AC, ATM | ν e, ν μ |
ν μ+nucleus→μ−+X |
CC, NC | Solid scintillator | Scintillation | ~0.5 GeV | Illinois and Minnesota, United States | 2005–2012 | ||||
MINOS+ | Upgraded electronics for MINOS | AC, ATM | ν e, ν μ, |
ν μ+nucleus→μ−+X |
CC, NC | Solid scintillator | Scintillation | ~0.5 GeV | Illinois and Minnesota, United States | 2013– | ||||
NEMO Experiment | Neutrino Ettore Majorana Observatory | Fréjus Road Tunnel, Italy/France | 2003– | |||||||||||
MOON | Molybdenum Observatory Of Neutrinos | LS, LSN | ν e |
ν e + 100Mo → 100Tc + e− |
CC | 100Mo ( kt) + 1 MoF6 (gas) | Scintillation | 168 keV | Washington, USA | |||||
NEMO Telescope | NEutrino Mediterranean Observatory | Mediterranean Sea, Italy | 2007– | |||||||||||
NEVOD | Cherenkov water detector NEVOD | ATM, CR | ν μ |
ν μ + n → μ− + p ν μ + p → μ+ + n |
CC | Water (H2O) | Cherenkov | ~2 GeV | Moscow, Russia | 1993– | ||||
NOνA | NuMI Off-Axis νe Appearance | AC | ν e, ν μ |
ν e+nucleus→e−+X |
CC | Liquid scintillator | Scintillation | ~0.1 GeV | Illinois and Minnesota, United States | 2011– | ||||
OPERA | Oscillation Project with Emulsion-tRacking Apparatus | AC | ν τ |
ν τ+nucleus→τ−+X |
CC | Lead/Emulsion | Nuclear Emulsion | ~1.0 GeV | LNGS (Italy) and CERN | 2008– | ||||
RENO | Reactor Experiment for Neutrino Oscillation | R | ν e |
ν e + p → e+ + n |
CC | Gd-doped LOS | Scintillation | 1.8 MeV | South Korea | 2011– | ||||
SAGE | Soviet–American Gallium Experiment | LS | ν e |
ν e + 71Ga → 71Ge + e− |
CC | GaCl3 | Radiochemical | 233.2 keV | Baksan Valley, Russia | 1990–2006 | ||||
SciBooNE | SciBar (Scintillator Bar) Booster Neutrino Experiment | AC | ν μ |
ν μ + 12C → μ− + X |
CC, NC | Plastic (CH,10 ton) | Scintillation | ~100 keV | Illinois, USA | 2007–2008 | ||||
SNO | Sudbury Neutrino Observatory | S, ATM, GSN | ν e, ν μ, ν τ |
ν e + 2D → 2p + e− νx + 2D → νx + n + p ν e + e− → ν e + e− |
CC NC ES |
Heavy water ( kt D2O) 1 | Cherenkov | 3.5 MeV | Creighton Mine, Ontario | 1999–2006 | ||||
SNO+ | SNO with liquid scintillator | S,LS,R,T,
SN,LSN |
ν e |
νx + e− → νx + e−
ν |
ES, BB | linear alkylbenzene (LAB) + PPO | Scintillation | ≈≤1MeV | Creighton Mine, Ontario | 2014– | ||||
Super-K | Super-Kamiokande | S, ATM, GSN | ν e, ν μ, ν τ |
ν e + e− → ν e + e− ν e + n → e− + p ν e + p → e+ + n |
ES CC CC |
Water (H2O) | Cherenkov | 200 MeV | Kamioka, Japan | 1996– | ||||
T2K | Tokai to Kamioka | AC | ν e, ν μ ν e, ν μ |
ν e + n → e− + p (+π, +X) ν |
CC
(NC) |
Water (H2O) | Cherenkov |
|
Tokai, Japan Kamioka, Japan | 2011- | ||||
UNO | Underground Nucleon decay and neutrino Observatory | S, ATM, GSN, RSN | ν e, ν μ, ν τ |
ν e + e− → ν e + e− |
ES | Water ( kt 440 H2O) | Cherenkov | Henderson Mine, Colorado | future | |||||
^[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
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