Search results
Results From The WOW.Com Content Network
The Kamioka Liquid Scintillator Antineutrino Detector (KamLAND) is an electron antineutrino detector at the Kamioka Observatory, an underground neutrino detection facility in Hida, Gifu, The device is situated in a drift mine shaft in the old KamiokaNDE cavity in the Japanese Alps .
Super-Kamiokande (abbreviation of Super-Kamioka Neutrino Detection Experiment, also abbreviated to Super-K or SK; Japanese: スーパーカミオカンデ) [2] is a neutrino observatory located under Mount Ikeno near the city of Hida, Gifu Prefecture, Japan.
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).
The ice itself is the detector medium. The direction of incident neutrinos is determined by recording the arrival time of individual photons using a three-dimensional array of detector modules each containing one photomultiplier tube. This method allows detection of neutrinos above 50 GeV with a spatial resolution of approximately 2 degrees.
The Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo (神岡 宇宙 素粒子 研究 施設, Kamioka Uchū Soryūshi Kenkyū Shisetsu, Japanese pronunciation: [kamioka ɯtɕɯː soɾʲɯꜜːɕi keŋkʲɯː ɕiseꜜtsɯ]) is a neutrino and gravitational waves laboratory located underground in the Mozumi mine of the Kamioka Mining and Smelting Co. near the Kamioka ...
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 ...
If the dark matter particles interact weakly, they may produce neutrinos through annihilation or decay. Those neutrinos could be visible in the HK detector as an excess of neutrinos from the direction of large gravitational potentials such as the galactic centre, the Sun or the Earth, over an isotropic atmospheric neutrino background. [3]: 281 ...
The K2K experiment (KEK to Kamioka) was a neutrino experiment that ran from June 1999 to November 2004. It used muon neutrinos from a well-controlled and well-understood beam to verify the oscillations previously observed by Super-Kamiokande using atmospheric neutrinos.