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SK-IV collected data on various natural sources of neutrinos, as well as acted as the far detector for the Tokai-to-Kamioka (T2K) long baseline neutrino oscillation experiment. SK-IV continued until June 2018. After that, the detector underwent a full refurbishment during Autumn of 2018. On 29 January 2019 the detector resumed data acquisition ...
Schematic of the KamLAND detector 36°25′21″N 137°18′55″E / 36.4225°N 137.3153°E / 36.4225; 137.3153 [ 1 ] : 105 The Kamioka Liquid Scintillator Antineutrino Detector (KamLAND) is an electron antineutrino detector at the Kamioka Observatory , an underground neutrino detection facility in Hida, Gifu ,
A chlorine detector in the former Homestake Mine near Lead, South Dakota, containing 520 short tons (470 metric tons) of fluid, was the first to detect the solar neutrinos, and made the first measurement of the deficit of electron neutrinos from the sun (see Solar neutrino problem).
KamLAND (Kamioka Liquid Scintillator Antineutrino Detector) is a 1.0 kiloton detector located at the Kamioka Observatory in Japan. Results based on a live-time of 749 days and presented in 2005 mark the first detection of geoneutrinos. The total number of antineutrino events was 152, of which 4.5 to 54.2 were geoneutrinos.
Kamioka Nucleon Decay Experiment S, ATM ν e: ν + e − → ν + e −: ES Water (H 2 O) 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 ...
T2K ("Tokai to Kamioka") is a particle physics experiment studying the oscillations of the accelerator neutrinos.The experiment is conducted in Japan by the international cooperation of about 500 physicists and engineers with over 60 research institutions from several countries from Europe, Asia and North America [1] and it is a recognized CERN experiment (RE13).
A history of large water Cherenkov detectors in Japan, and long-baseline neutrino oscillation experiments associated with them, excluding HK: 1983-1996: Kamiokande (Kamioka Nucleon Decay Experiment), which main goal was proton decay searches (the Nobel Prize in Physics 2002 for Masatoshi Koshiba) – the predecessor of Super-Kamiokande [1]
With current detectors, it is difficult to directly measure the DSNB on the order of 10 6 eV due to high background signal from solar neutrinos, reactor antineutrinos, and radioactivity. As a result, multiple experiments have made attempts to probe the DSNB signal at a magnitude above (10 7 eV) to place upper limits on the flux and detection ...