List of neutrino experiments

Short description: none

Neutrino experiments are scientific studies investigating the properties of neutrinos, which are subatomic particles that are very difficult to detect due to their weak interactions with matter. Neutrino experiments are essential for understanding the fundamental properties of matter and the universe's behaviour at the subatomic level. Here is a non-exhaustive list of neutrino experiments and neutrino detectors.

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, United States  | future | [1]
ANTARES | Astronomy with a Neutrino Telescope and Abyss Environmental RESearch  | ATM, CR, AGN, PUL  | νe, νμ, ντ |  |  | Seawater | Cherenkov |  | Mediterranean Sea, France  | 2006–2022  | [2]
ARIANNA | Antarctic Ross Ice-Shelf ANtenna Neutrino Array  | S, CR, AGN, ?  | νe, νμ, ντ |  |  |  |  |  | Ross Ice Shelf, Antarctica | future  | [3]
BDUNT (NT-200+)
Baikal-GVD  | Baikal Deep Underwater Neutrino Telescope /
Gigaton Volume Detector  | S, ATM, LS, AGN, PUL  | νe, νμ, ντ |  | CC, NC  | Water (H2O)  | Cherenkov | ≈10 GeV  | Lake Baikal, Russia  | 1993–  | [4]
[5]
BOREXINO  | BORon EXperiment  | LS  | νe | νx \+ e− → νx \+ e− | ES  | LOS shielded by water  | Scintillation | 250–665 keV  | Gran Sasso, Italy  | May 2007–  | [6] [7]
BUST | Baksan Underground Scintillation Telescope  |  |  |  |  |  | Scintillation |  | Baksan River valley, Russia  | 1977–  | [8]
CCM  | Coherent CAPTAIN-Mills  | AC  | νe |  | CC  | Liquid Argon | Scintillation | 50 keV  | Los Alamos Neutron Science Center | 2019-  | [9]
CHANDLER | Carbon Hydrogen AntiNeutrino Detector with a Lithium Enhanced Raghavan-optical-lattice  | R  | νe | νe \+ p → e+ \+ n | CC  | WLS Plastic Scintillating Cubes and Lithium-6-loaded Zinc Sulfide Sheets  | Scintillation  | 1.8 MeV  | North Anna, Virginia, US  | June 2017-  | [10]
CLEAN | Cryogenic Low-Energy Astrophysics with Neon  | LS, SN, WIMP  | νe | νx \+ e− → νx \+ e−

νe \+ The element Chemistry:Neon does not exist. → νe \+ The element Chemistry:Neon does not exist.

| ES
ES  | Liquid Ne (10 t)  | Scintillation |  | SNOLAB
Ontario, Canada  | future | [11]
COBRA | Cadmium zinc telluride 0-neutrino double-Beta Research Apparatus  |  |  | The element Chemistry:Zinc does not exist. \+ e− → The element Chemistry:Nickel does not exist. \+ e+
The element Chemistry:Zinc does not exist. → The element Chemistry:Germanium does not exist. \+ e− \+ e−
The element Chemistry:Cadmium does not exist. → The element Chemistry:Palladium does not exist. \+ e+ \+ e+
The element Chemistry:Cadmium does not exist. \+ e− \+ e− → The element Chemistry:Palladium does not exist.
The element Chemistry:Cadmium does not exist. → The element Chemistry:Tin does not exist. \+ e− \+ e−
The element Chemistry:Cadmium does not exist. → The element Chemistry:Tin does not exist. \+ e− \+ e−
The element Chemistry:Tellurium does not exist. \+ e− → The element Chemistry:Tin does not exist. \+ e+
The element Chemistry:Tellurium does not exist. → The element Chemistry:Xenon does not exist. \+ e− \+ e−
The element Chemistry:Tellurium does not exist. → The element Chemistry:Xenon does not exist. \+ e− \+ e− | BB  | Cadmium zinc telluride |  |  | Gran Sasso, Italy  | 2007–  | [12]
COHERENT | COHERENT  | AC  | νμ, νμ, νe | ν \+ nucleus → ν \+ nucleus  | ES (NC), CC  | 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-  | [13]
CONUS / CONUS+ | COherent Neutrino nUcleus Scattering  | R  | νe | νe \+ nucleus → νe \+ nucleus  | ES (NC)  | HPGe  | Coherent Elastic Neutrino Nucleus Scattering (CEvNS)  | 4 detectors: 160eV, 170eV, 180eV and 250eV [1] | Brokdorf Nuclear Power Plant, Germany (CONUS);

Leibstadt Nuclear Power Plant, Switzerland (CONUS+)

| 2018-2022 (CONUS);

2022-Ongoing (CONUS+)

| [14]
Daya Bay | Daya Bay Reactor Neutrino Experiment  | R  | νe | νe \+ p → e+ \+ n | CC  | Gd-doped LAB (LOS)  | Scintillation | 1.8 MeV  | Daya Bay, China  | 2011–2020  | [15]
Double Chooz | Double Chooz Reactor Neutrino Experiment  | R  | νe | νe \+ p → e+ \+ n | CC  | Gd-doped LOS | Scintillation | 1.8 MeV  | Chooz, France  | 2011–2017  | [16]
DUNE | Deep Underground Neutrino Experiment  | AC, ATM, (S), SN  | all  |  | NC, CC, (ES)  | Liquid argon | Scintillation & Time projection chamber | around 10 MeV  | Sanford Underground Research Facility | construction start 2017 | [17]
ENUBET | Enhanced NeUtrino BEams from kaon Tagging  | AC  | νe, νμ
νe, νμ | νe \+ n → e− \+ p (+π, +X)
νμ \+ n → μ− \+ p (+π, +X)

νe \+ p → e+ \+ n (+π, +X)
νμ \+ p → μ+ \+ n (+π, +X)

| CC

(NC)

|  |  |  |  | future  | [18]
ESSnuSB | The European Spallation Source neutrino Super Beam  | AC  | νμ, νμ(Background: νe,νe)  |  |  | Water  | Water Cherenkov MEMPHYS detector  | 0.36 GeV  | Garpenberg, Lund, Sweden  | future by 2023  | [2][3][19]
FASER | ForwArd Search ExpeRiment  | C  | νe, νμ, ντ | ν \+ N → ℓ \+ X  | CC + NC  | Tungsten | Emulsion  | >10 GeV  | Large Hadron Collider | 2022-  | [20]
EXO-200 | Enriched Xenon Observatory  |  |  | The element Chemistry:Xenon does not exist. → The element Chemistry:Barium does not exist. \+ e− \+ e−
The element Chemistry:Xenon does not exist. → The element Chemistry:Barium does not exist. \+ e− \+ e− | BB  | Liquid Xenon |  |  | WIPP, New Mexico  | 2009–  | [21]
GALLEX | GALLium EXperiment  | LS  | νe | νe \+ The element Chemistry:Gallium does not exist. → The element Chemistry:Germanium does not exist. \+ e− | CC  | GaCl3 (30 t)  | Radiochemical | 233.2 keV  | Gran Sasso, Italy  | 1991–1997  | [22]
GERDA  | The GERmanium Detector Array  | BB  | νe | The element Chemistry:Germanium does not exist. → The element Chemistry:Arsenic does not exist. \+ e− \+ e− | BB  | HPGe  | Semiconductor  | ~20 keV  | Gran Sasso, Italy  | 2015-2019  | [23]
GRAND | Giant Radio Array for Neutrino Detection  | AGN, CR, ?  | ντ | ντ \+ N → τ− \+ X  | CC  | Electromagnetic waves caused by τ− through extensive air showers in the atmosphere.  | Radio | 1017 eV  | China  | Proposed  | [24]
HALO  | Helium And Lead Observatory  | SN  | νe, νx | νe \+ The element Chemistry:Lead does not exist. → e− \+ The element Chemistry:Bismuth does not exist.*
ν \+ The element Chemistry:Lead does not exist. → ν \+ The element Chemistry:Lead does not exist.*  | CC, NC  | Lead (79 t) and 3He | High-Z  | ≈10 MeV  | Creighton Mine, Ontario  | 2012–  | [25]
HERON  | Helium Roton Observation of Neutrinos  | LS  | νe (mainly)  | νe \+ e− → νe \+ e− | NC  | Superfluid He  | Rotational excitation  | 1 MeV  |  | future | [26]
HOMESTAKE–CHLORINE  | Homestake chlorine experiment  | S  | νe | The element Chemistry:Chlorine does not exist. \+ νe → The element Chemistry:Argon does not exist.* + e−
The element Chemistry:Argon does not exist.* → The element Chemistry:Chlorine does not exist. \+ e+ \+ νe | CC  | C2Cl4 (615 t)  | Radiochemical | 814 keV  | Homestake Mine, South Dakota  | 1967–1998  | [27]
HOMESTAKE–IODINE  | Homestake iodine experiment  | S  | νe | ν \+ e− → ν \+ e−
νe \+ The element Chemistry:Iodine does not exist. → The element Chemistry:Xenon does not exist. \+ e− | ES
CC  | NaI in water  | Radiochemical | 789 keV  | Homestake Mine, South Dakota  | future | [28]
Hyper-Kamiokande | Hyper-Kamiokande  | S, ATM, SN, AC  | νe, νμ
νe, νμ | νe \+ e− → νe \+ e−

νe \+ n → e− \+ p (+π, +X)
νμ \+ n → μ− \+ p (+π, +X)
νe \+ p → e+ \+ n (+π, +X)
νμ \+ p → μ+ \+ n (+π, +X)

| ES, CC, (NC)  | water | Cherenkov | 200 MeV  | Tokai and Kamioka, Japan | 2027-
(under construction)  | [29]
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  | 2010–  | [30]
IceCube  | IceCube Neutrino Detector  | ATM, CR, AGN, ?  | νe, νμ, ντ | ν \+ N → ν \+ Cascade , ν \+ N → Charged lepton + Cascade  | CC, NC  | Water ice (1 km3)  | Cherenkov | ≈10 GeV  | South Pole, Antarctica | 2006–  | [31]
India-based Neutrino Observatory | Iron Calorimeter Detector @ India-based Neutrino Observatory  | ATM  | νμ | νμ+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)  | [32]
JUNO | Jiangmen Underground Neutrino Observatory  | R  | νe | νe \+ p → e+ \+ n | CC  | LAB (LOS) + PPO + Bis-MSB  | Scintillation |  | Kaiping, China  | 2014– (construction)  | [33]
Kamiokande  | Kamioka Nucleon Decay Experiment  | S, ATM  | νe | ν \+ e− → ν \+ e− | ES  | Water (H2O)  | Cherenkov | 7.5 MeV  | Kamioka, Japan  | 1986–1995  | [34]
KamLAND  | Kamioka Liquid Scintillator Antineutrino Detector  | R  | νe | νe \+ p → e+ \+ n | CC  | LOS | Scintillation | 1.8 MeV  | Kamioka, Japan  | 2002–  | [35]
KATRIN | Karlsruhe Tritium Neutrino experiment  | MTR, ATR  | νe | The element Chemistry:Hydrogen does not exist. → The element Chemistry:Helium does not exist. \+ e− \+ νe | CC  | Spectrometer | Semiconductor | ≈ 0.45 eV  | Germany  | 2019-  | [36]
KM3NeT | KM3 Neutrino Telescope  | S, ATM, CR, SN, AGN, PUL  | νμ,νe,ντ |  |  | Sea water (≈5 km3)  | Cherenkov  |  | Mediterranean Sea | 2014–  | [37]
LAGUNA  | Large Apparatus studying Grand Unification and Neutrino Astrophysics  |  |  |  |  |  |  |  |  | future | [38]
LEGEND  | The Large Enriched Germanium Experiment for Neutrinoless ββ Decay  | BB  | νe | The element Chemistry:Germanium does not exist. → The element Chemistry:Arsenic does not exist. \+ e− \+ e− | BB  | HPGe  | Semiconductor  | ~50 keV  | Gran Sasso, Italy  | 2023-  | [39]
LENS  | Low Energy Neutrino Spectroscopy  | LS  | νe | νe \+ The element Chemistry:Indium does not exist. → The element Chemistry:Tin does not exist. \+ νe \+ 2γ | CC  | In-doped LOS | Scintillation | 120 keV  |  | proposed  | [40] [41]
Majorana Demonstrator | The Majorana Demonstrator | BB  | νe | The element Chemistry:Germanium does not exist. → The element Chemistry:Arsenic does not exist. \+ e− \+ e− | BB  | HPGe  | Semiconductor  | ~2 keV  | Homestake Mine, South Dakota  | 2015-2021  | [42]
MicroBooNE |  | AC, SN  | νe, νμ |  | ES, NC, CC  | Liquid Argon  | TPC  | few MeV  | Illinois, United States  | 2014-  | [43]
MINERvA  | Main Injector ExpeRiment for v-A  | AC  | νμ | many  | CC, NC  | Solid scintillator, targets of Liquid helium, Carbon, Water, Iron, Lead | Scintillation  | ≈0.5 GeV  | Illinois, United States  | 2009–2019  | [44]
MiniBooNE | Mini Booster Neutrino Experiment  | AC  | νe, νμ | νe \+ The element Chemistry:Carbon does not exist. → e− \+ X | CC  | Mineral oil (1000 t)  | Cherenkov | ≈100 keV  | Illinois, United States  | 2002–  | [45]
MINOS | Main Injector Neutrino Oscillation Search  | AC, ATM  | νe, νμ | νμ+nucleus → μ−+X  | CC, NC  | Solid scintillator  | Scintillation  | ≈0.5 GeV  | Illinois and Minnesota, United States  | 2005–2012  | [46]
MINOS+ | Upgraded electronics for MINOS  | AC, ATM  | νe, νμ,  | νμ+nucleus → μ−+X  | CC, NC  | Solid scintillator  | Scintillation  | ≈0.5 GeV  | Illinois and Minnesota, United States  | 2013–  | [47]
MOON  | Molybdenum Observatory Of Neutrinos  | LS, LSN  | νe | νe \+ The element Chemistry:Molybdenum does not exist. → The element Chemistry:Technetium does not exist. \+ e− | CC  | The element Chemistry:Molybdenum does not exist. (1 kt) + MoF6 (gas)  | Scintillation | 168 keV  | Washington, United States  |  | [48]
NEMO-3 | Neutrino Ettore Majorana Observatory  | BB  | νe | The element Chemistry:Molybdenum does not exist. → The element Chemistry:Ruthenium does not exist. \+ 2 e−
The element Chemistry:Selenium does not exist. → The element Chemistry:Krypton does not exist. \+ 2 e− | BB  | Tracker + calorimeter  | He+Ar wire chamber, plastic scintillators  | 150 keV  | Modane Underground Laboratory, Fréjus Road Tunnel, France  | 2003–2011  | [49]
NEMO Telescope  | NEutrino Mediterranean Observatory  |  |  |  |  |  |  |  | Mediterranean Sea, Italy  | 2007–  | [50]
Neutrino-4  | Neutrino-4 Reactor Neutrino Experiment  | R  | νe | νe \+ p → e+ \+ n | CC  | liquid organic scintillator loaded with Gd  | Scintillation | ≈2 MeV  | Dimitrovgrad, Russia  | 2014–  | [4]
NEVOD | Cherenkov water detector NEVOD  | ATM, CR  | νμ | νμ \+ n → μ− \+ p
νμ \+ p → μ+ \+ n | CC  | Water (H2O)  | Cherenkov | ≈2 GeV  | Moscow, Russia  | 1993–  | [51]
NEXT  | Neutrino Experiment with a Xenon Time Projection Chamber  | BB  |  | The element Chemistry:Xenon does not exist. → The element Chemistry:Barium does not exist. \+ 2 e− | BB  | Gaseous Xenon  | Time projection chamber | ≈10 keV  | Canfranc, Spain  | 2016–  | [52]
NOνA  | NuMI Off-Axis νe Appearance  | AC  | νe, νμ | νe+nucleus → e−+X  | CC  | Liquid scintillator  | Scintillation  | ≈0.1 GeV  | Illinois and Minnesota, United States  | 2011–  | [53]
NUCLEUS  | NUCLEUS  | R  | νe | νe \+ nucleus → νe \+ nucleus  | ES (NC)  | CaWO4 / Al2O3  | Phonon-mediated Transition-edge sensor Bolometer | 20 eV[5] | Technical University of Munich, Germany (Development);

Chooz Nuclear Power Plant, France

| 2017 (R&D);

Future (Experiment)

| [54]
OPERA  | Oscillation Project with Emulsion-tRacking Apparatus  | AC  | ντ | ντ+nucleus → τ−+X  | CC  | Lead/Emulsion  | Nuclear Emulsion  | ≈1.0 GeV  | LNGS (Italy) and CERN | 2008–  | [55]
Auger | Pierre Auger Observatory  | CR  |  |  |  |  | Cherenkov  |  | Argentina  |  | [56]
Project 8  | Project 8 experiment  | ATR  | νe | The element Chemistry:Hydrogen does not exist. → The element Chemistry:Helium does not exist. \+ e− \+ νe | CC  | Microwave Cavity | Radio | ≈ 0.04 eV  | USA, Germany  | future | [57]
RENO | Reactor Experiment for Neutrino Oscillation  | R  | νe | νe \+ p → e+ \+ n | CC  | Gd-doped LOS | Scintillation | 1.8 MeV  | South Korea  | 2011–  |
RNO-G  | Radio Neutrino Observatory Greenland  | CR, AGN, ?  | νe, νμ, ντ |  | CC, NC  | In-Ice  | Radio  | >10 PeV  | Summit Camp, Greenland | 2021–  | [58]
SAGE  | Soviet–American Gallium Experiment  | LS  | νe | νe \+ The element Chemistry:Gallium does not exist. → The element Chemistry:Germanium does not exist. \+ e− | CC  | Ga (metallic)  | Radiochemical | 233.2 keV  | Baksan River valley, Russia  | 1989–  | [59]
SciBooNE | SciBar (Scintillator Bar) Booster Neutrino Experiment  | AC  | νμ | νμ \+ The element Chemistry:Carbon does not exist. → μ− \+ X | CC, NC  | Plastic (CH,10 ton)  | Scintillation | ≈100 keV  | Illinois, United States  | 2007–2008  | [60]
SNO | Sudbury Neutrino Observatory  | S, ATM, GSN  | νe, νμ, ντ | νe \+ The element Chemistry:Deuterium does not exist. → 2p \+ e−
νx \+ The element Chemistry:Deuterium does not exist. → νx \+ n \+ p
νe \+ e− → νe \+ e− | CC

ES  | Heavy water (1 kt D2O)  | Cherenkov | 3.5 MeV  | Creighton Mine, Ontario  | 1999–2006  | [61]
SNO+ | SNO with liquid scintillator  | S,LS,R,T,

SN,LSN

| νe | νx \+ e− → νx \+ e−

νe \+ p → e+ \+ n

| ES, BB  | linear alkylbenzene (LAB) \+ PPO  | Scintillation | ≈≤1MeV  | Creighton Mine, Ontario  | 2014–  | [62]
SoLid  | Short baseline Oscillation Search with Lithium-6 Detector  | R  | νe | νe \+ p → e+ \+ n | CC  | plastic and anorganic scintillator  | Scintillation | ≈2 MeV  | Mol, Belgium  | 2015-  | [63]
STEREO | STErile neutrino REactor Oscillation experiment  | R  | νe | νe \+ p → e+ \+ n | CC  | liquid organic scintillator loaded with Gd  | Scintillation | ≈2 MeV  | Grenoble, France  | 2013–  | [64]
Super-K | Super-Kamiokande  | S, ATM, GSN  | νe, νμ, ντ | νe \+ e− → νe \+ e−
νe \+ n → e− \+ p
νe \+ p → e+ \+ n | ES

CC  | Water (H2O)  | Cherenkov | 200 MeV  | Kamioka, Japan  | 1996–  | [65] [66]
SuperNEMO  | SuperNEMO  | BB  | νe | The element Chemistry:Selenium does not exist. → The element Chemistry:Krypton does not exist. \+ 2 e−
The element Chemistry:Neodymium does not exist. → The element Chemistry:Samarium does not exist. \+ 2 e− | BB  | Tracker + calorimeter  | He+Ar wire chamber, plastic scintillators  | 150 keV  | Modane Underground Laboratory, Fréjus Road Tunnel, France  | 2017–  | [67]
TRIDENT  | TRopIcal DEep-sea Neutrino Telescope  | S, ATM, CR, SN, AGN, PUL  | νe, νμ, ντ |  | CC, NC  | Seawater (7.5 cubic km)  | Cherenkov |  | Western Pacific Ocean | Proposed

Pilot: 2026
Full operation: 2030

| [68]
T2K | Tokai to Kamioka  | AC  | νe, νμ
νe, νμ | νe \+ n → e− \+ p (+π, +X)
νμ \+ n → μ− \+ p (+π, +X)

νe \+ p → e+ \+ n (+π, +X)
νμ \+ p → μ+ \+ n (+π, +X)

| CC

(NC)

| Water (H2O) | Cherenkov |  |  | 200 MeV  |

|
|

Tokai, Japan Kamioka, Japan  | 2011–  | [69]
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  | abandoned  | [70]

^[a] Accelerator neutrino (AC), Active galactic nuclei neutrino (AGN), Atmospheric neutrino (ATM), Collider neutrino (C), 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), Molecular Tritium neutrino (MTR), Atomic Tritium neutrino (ATR), Electron Capture neutrino (EC).
^[b] Double beta decay (BB), Charged current (CC), Elastic scattering (ES), Neutral current (NC).

## See also

* Aspera European Astroparticle network

## References

1. ↑ Ackermann, N.; Bonet, H.; Bonhomme, A.; Buck, C.; Fülber, K.; Hakenmüller, J.; Hempfling, J.; Heusser, G. et al. (2025). "Direct observation of coherent elastic antineutrino–nucleus scattering". Nature 643 (8074): 1229–1233. doi:10.1038/s41586-025-09322-2. PMID 40739024. Bibcode: 2025Natur.643.1229A.
2. ↑ Wildner, E.; Baussan, E.; Blennow, M.; Bogomilov, M.; Burgman, A.; Bouquerel, E.; Carlile, C.; Cederkäll, J. et al. (2016). "The Opportunity Offered by the ESSnuSB Project to Exploit the Larger Leptonic CP Violation Signal at the Second Oscillation Maximum and the Requirements of This Project on the ESS Accelerator Complex" (in en). Advances in High Energy Physics 2016: 1–16. doi:10.1155/2016/8640493. ISSN 1687-7357.
3. ↑ Dracos, Marcos (September 2018). "The European Spallation Source neutrino Super Beam". Journal of Physics: Conference Series 1067. doi:10.1088/1742-6596/1067/4/042001. ISSN 1742-6588.
4. ↑ A.P. Serebrov (2015). "Neutrino-4 Experiment on the Search for a Sterile Neutrino at the SM-3 Reactor". Journal of Experimental and Theoretical Physics 121 (4): 578–586. doi:10.1134/S1063776115100209. Bibcode: 2015JETP..121..578S.
5. ↑ Strauss, R.; Rothe, J.; Angloher, G.; Bento, A.; Gütlein, A.; Hauff, D.; Kluck, H.; Mancuso, M. et al. (2017-07-31). "The $$\nu $$-cleus experiment: a gram-scale fiducial-volume cryogenic detector for the first detection of coherent neutrino–nucleus scattering" (in en). The European Physical Journal C 77 (8): 506. doi:10.1140/epjc/s10052-017-5068-2. ISSN 1434-6052. https://link.springer.com/article/10.1140/epjc/s10052-017-5068-2.

## External links

* "Experiments". Istituto Nazionale di Fisica Nucleare. 24 February 2017. http://www.nu.to.infn.it/exp/. Regularly updated index of neutrino physics research.

* v
* t
* e

Neutrino detectors, experiments, and facilities

Discoveries|

* Cowan–Reines (νe)
* Lederman–Schwartz–Steinberger (νμ)
* DONUT (ντ)
* Neutrino oscillation
* SN 1987 neutrino burst

Operating
(divided by
primary
neutrino
source)|

| Astronomical|

* ANITA
* ANTARES
* BDUNT
* Borexino
* BUST
* HALO
* IceCube
* LVD
* NEVOD
* SAGE
* Super-Kamiokande
* SNEWS

|

Reactor|

* Daya Bay
* Double Chooz
* KamLAND
* RENO
* STEREO

Accelerator|

* ICARUS (Fermilab)
* MicroBooNE
* MINERνA
* MiniBooNE
* NA61/SHINE
* NOνA
* NuMI
* T2K
* COHERENT

0νββ|

* AMoRE
* COBRA
* CUORE
* EXO
* GERDA
* KamLAND-Zen
* MAJORANA
* NEXT
* PandaX
* XMASS

Other|

* KATRIN
* WITCH

Construction|

* ANNIE
* ARA
* ARIANNA
* BEST
* DUNE
* JUNO
* KM3NeT
* SNO+
* SuperNEMO

Retired|

* AMANDA
* CDHS
* Chooz
* CNGS
* Cuoricino
* DONUT
* ERPM
* GALLEX
* Gargamelle
* GNO
* Heidelberg-Moscow
* Homestake
* ICARUS
* IGEX
* IMB
* K2K
* Kamiokande
* KARMEN
* KGF
* LSND
* MACRO
* MINOS
* MINOS+
* NARC
* NEMO
* OPERA
* RICE
* SciBooNE
* SNO
* Soudan 2
* Utah

Proposed|

* CUPID
* GRAND
* Hyper-Kamiokande
* INO
* LAGUNA
* LEGEND
* LENA
* Neutrino Factory
* nEXO
* Nucifer
* SBND
* UNO
* JEM-EUSO
* WATCHMAN

Cancelled|

* DUMAND Project
* Long Baseline Neutrino Experiment
* NEMO Project
* NESTOR Project
* SOX
* BOREX

See also|

* BNO
* Kamioka Observatory
* LNGS
* SNOLAB
* List of neutrino experiments

0.00

(0 votes)

Original source: https://en.wikipedia.org/wiki/List of neutrino experiments. Read more

|

Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:List_of_neutrino_experiments&oldid=4336969"
*[v]: View this template
*[t]: Discuss this template
*[e]: Edit this template