List of neutrino experiments

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List of neutrino experiments, neutrino detectors and neutrino telescopes.

[edit] General data

General data
Abbreviation Experiment Place Home page Collaborators Scheduled operation
ANTARES Astronomy with a Neutrino Telescope and Abyss Environmental RESearch Mediterranean Sea, France [1] 2006
BOREXINO BORon EXperiment Gran Sasso, Italy [2] [3] LNGS, INFN et al. May 2007
CLEAN Cryogenic Low-Energy Astrophysics with Neon ([4], PDF) LANL future
Daya Bay Daya Bay Reactor Neutrino Experiment Daya Bay, China [5] 2009
Double Chooz Double Chooz Reactor Neutrino Experiment Chooz, Ardennes, France [6] 2008–
EXO future
GALLEX GALLium EXperiment Gran Sasso, Italy [7] LNGS, INFN 19911997
GNO Gallium Neutrino Observatory Gran Sasso, Italy [8] LNGS, INFN May 1998–Jan 2002
HERON Helium Roton Observation of Neutrinos [9] LBNL future
HOMESTAKE–CHLORINE Homestake chlorine experiment Homestake mine, South Dakota, USA [10] BNL 19671998
HOMESTAKE–IODINE Homestake iodine experiment Homestake mine, South Dakota, USA [11] BNL future
ICARUS Imaging Cosmic And Rare Underground Signal Gran Sasso, Italy [12] CERN et al.
IceCube IceCube Neutrino Detector South Pole, Antarctica [13] 2006
Kamiokande Kamioka Nucleon Decay Experiment Kamioka, Japan [14] 19861995
KamLAND Kamioka Liquid Scintillator Antineutrino Detector Kamioka, Japan [15] 2002-
KM3NeT KM3 Neutrino Telescope Mediterranean, ? [16] 2009
LENS Low Energy Neutrino Spectroscopy [17] [18] VT, ORNL, UNC, BNL, INR
Majorana Neutrinoless Double Beta Decay in 76Ge to measure neutrino mass Homestake, SD, USA [19] Duke, LANL, LBNL, LLNL, ORNL, PNNL, TUNL, NC State, Osaka U, Queen's U, U Alberta, U Chicago, UNC, USC, USD, UT, UW, ITEP, JINR future (~2010)
MOON Molybdenum Observatory Of Neutrinos Washington, USA [20]
MiniBooNE Mini Booster Neutrino Experiment Illinois,USA [21] Fermilab 2002
NEMO TELESCOPE NEutrino Mediterranean Observatory Mediterranean Sea, Italy [22] 2007–
NOνA NuMI Off-Axis νe Appearance Illinois and Minnesota,USA [23] Fermilab and the University of Minnesota 2011
SAGE Soviet–American Gallium Experiment Baksan valley, Russia [24] 19902006
SNO Sudbury Neutrino Observatory Creighton Mine, Greater Sudbury, Ontario, Canada [25] SNOLAB, LBNL 1999–2006
SNO+ SNO with liquid scintillator Creighton Mine, Greater Sudbury, Ontario, Canada [26] Queen's University, SNOLAB, et al. 2009–
SK Super-Kamiokande Kamioka, Gifu, Japan [27] [28] 1996
UNO Underground Nucleon decay and neutrino Observatory Henderson mine, Colorado [29] NUSL future

[edit] Technical data

Technical data
Abbreviation Sensitivity
(1)
Sensitivity
(2)
Induced reaction* Type of
reaction
Detector Type of
detector
threshold
energy
BOREXINO lS νe νx + e → νx + e
ES
LOS shielded by water scintillation 250–665 keV
Double Chooz R \bar\nu_e \bar\nu_e + p → e+ + n
CC
Gd-doped LOS scintillation 1.8 MeV
CLEAN lS, SN, WIMP νe vx + e → vx + e
ve + 20Ne → ve + 20Ne
ES

ES
10 t liquid Ne scintillation  ???
GALLEX lS νe ve+71Ga → 71Ge+e
CC
GaCl3 (30 t Ga) radiochemical 233.2 keV
GNO lS νe ve+71Ga → 71Ge+e
CC
GaCl3 (30 t Ga) radiochemical 233.2 keV
HERON lS mainly νe ve + e → ve + e
NC
superfluid
He
rotational
excitation
1 MeV
HOMESTAKE–CHLORINE S νe 37Cl+ve37Ar*+e
37Ar*37Cl + e+ + ve
CC
C2Cl4 (615 t) radiochemical 814 keV
HOMESTAKE–IODINE S νe ve + e → ve + e
ve + 127I → 127Xe + e
ES

CC
NaI in water radiochemical 789 keV
ICARUS S, ATM, GSN νe, νμ, ντ ve + e → ve + e
ES
liquid Ar Cherenkov 5.9 MeV
IceCube S, ATM, CR, ? νe, νμ, ντ ve + e → ve + e
etc.
ES
1 km³ H2O (ice) ice Cherenkov ~10 MeV
Kamiokande S, ATM νe ve + e → ve + e
ES
H2O Cherenkov 7.5 MeV
LENS lS νe ve + 115In → 115Sn+e+2γ
CC
LOS doped by In scintillation 120 keV
MiniBooNE AC νe, νμ ve+12C → e + X
CC
mineral oil (1 kton) Cherenkov ~100 MeV
MOON lS, lSN νe ve+100Mo → 100Tc+e
CC
100Mo (1 t) + MoF6 (gas) scintillation 168 keV
SAGE lS νe ve+71Ga → 71Ge+e
CC
GaCl3 radiochemical 233.2 keV
SNO S, ATM, GSN νe, νμ, ντ ve + 21D →p++p++e
vx + 21D →vx+no+p+
ve + e → ve + e
CC

NC

ES
1000 t D2O heavy water Čerenkov 3.5 MeV
Super Kamiokande S, ATM, GSN νe, νμ, ντ ve + e → ve + e
ve + no → e + p+
ve + p+ → e+ + no
ES

CC
H2O water Cherenkov
UNO S, ATM, GSN, RSN νe, νμ, ντ ve + e → ve + e
ES
440 kt H2O water Cherenkov ???

Notation

Sensitivity (1)

  • solar neutrinos (S)
  • low-energy solar neutrinos (ls)
  • reactor neutrino experiment (R)
  • terrestrial neutrinos (T)
  • atmospheric neutrinos (ATM)
  • accelerator experiment (AC)
  • cosmic ray (CR)
  • supernova neutrinos (S)
  • low-energy supernova neutrinos (lSN)
  • Active Galactic Nuclei (AGN)
  • neutrinos from pulsars (PUL)

Sensitivity (2)

  • electron neutrino (νe)
  • muon neutrino (νμ)
  • tau neutrino (ντ)

Type of process

  • elastic scattering (ES)
  • neutral current (NC)
  • charged current (CC)

Detector

  • Liquid organic scintillator (LOS)

Research Institution

Languages