1. The Jiangmen Underground Neutrino Observatory (JUNO)
- Author
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Cedric Cerna, Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and JUNO
- Subjects
Nuclear and High Energy Physics ,Sterile neutrino ,Cherenkov detector ,Physics::Instrumentation and Detectors ,Cherenkov counter: water ,Physics beyond the Standard Model ,Dark matter ,scintillation counter: liquid ,energy resolution ,cosmic background radiation ,7. Clean energy ,01 natural sciences ,law.invention ,Nuclear physics ,law ,0103 physical sciences ,Neutrino ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,010306 general physics ,Neutrino oscillation ,Instrumentation ,detector: design ,activity report ,Jiangmen Underground Neutrino Observatory ,Physics ,JUNO ,photomultiplier ,010308 nuclear & particles physics ,Detector ,High Energy Physics::Phenomenology ,Photomultipliers ,neutrino: detector ,High Energy Physics::Experiment - Abstract
The Jiangmen Underground Neutrino Observatory (JUNO) is an experiment under construction in China with the primary goal of determining the neutrino mass hierarchy (MH) with reactor anti-neutrinos. The JUNO detector system consists of a central detector, an active veto system and a calibration system. The central detector is a 35 m diameter transparent acrylic sphere containing a 20 kton liquid scintillator neutrino target. A primary photo-detection system consisting of 18,000 large (20” diameter) dynode and micro-channel plate photomultipliers surrounds the central detector. A second interlaced photo-detection system is made of 25,600 small (3” diameter) photomultipliers working in the single photo-electron regime for the reactor anti-neutrino detection. The detector is designed to achieve an unprecedented energy resolution of 3% @1MeV and an absolute energy scale uncertainty better than 1%. A veto system, consisting of a water Cherenkov detector and a top tracker, is used help maximally remove cosmogenic backgrounds. Due to its unprecedented scale and precision, JUNO will be an exceptional multipurpose detector with a rich physics program in neutrino oscillation , geo-neutrinos, astrophysical neutrinos and the search for physics beyond the Standard Model (sterile neutrinos, dark matter, proton decay and others).
- Published
- 2019
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