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JUNO physics and detector

  • JUNO Collaboration
  • Pontificia Universidad Católica de Chile
  • Institut Pluridisciplinaire Hubert Curien
  • Pakistan Institute of Nuclear Science and Technology
  • Università di Catania
  • East China University of Science and Technology
  • Institute of High Energy Physics Chinese Academy of Science
  • University of Science and Technology of China
  • Joint Inst. for Nuclear Research
  • University of Milan
  • Chulalongkorn University
  • University Paris-Sud
  • Comenius University
  • University of Ferrara
  • Universit̀ Degli Studi di Milano-Bicocca
  • Dipartimento di Fisica 'G. Galilei' and INFN
  • Sez. di Roma Tre
  • RWTH Aachen University
  • University of Tübingen
  • National Taiwan University
  • l'institut du thorax
  • National United University Taiwan
  • CENBG
  • University of Padova
  • Aix-Marseille Université
  • Wuhan University
  • Politecnico di Milano
  • Dongguan University of Technology
  • Tsinghua University
  • Institute of Modern Physics Chinese Academy of Sciences
  • National Chiao Tung University
  • North China Electric Power University
  • Sun Yat-Sen University
  • Beijing Institute of Spacecraft Systems Engineering
  • Universidade Estadual de Londrina
  • Università di Perugia
  • Université Libre de Bruxelles
  • University of California, Irvine
  • Johannes Gutenberg University
  • Suranaree University of Technology
  • Charles University in Prague
  • Moscow State University
  • Institute for Nuclear Research of the Russian Academy of Sciences
  • Zhengzhou University
  • University of Jyväskylä
  • Wuyi University
  • Guangxi University
  • Harbin Institute of Technology
  • Chinese Academy of Geological Sciences
  • Forschungszentrum Jülich (FZJ)
  • Jinan University
  • Beijing Normal University
  • Xi'an Jiaotong University
  • Universität Hamburg
  • China Institute of Atomic Energy
  • Shandong University
  • Shanghai Jiao Tong University
  • A.I. Alikhanyan National Science Laboratory (YerPhi)
  • Nankai University
  • National University of Defense Technology (NUDT)
  • University of Chinese Academy of Sciences
  • University of South China
  • Jilin University
  • Xiamen University
  • Beijing University
  • INFN, Laboratori Nazionali Di Frascati
  • Institute of Electronics and Computer Science Latvia
  • Universidad Técnica Federico Santa María
  • Pontifícia Universidade Católica do Rio de Janeiro
  • Nanjing University
  • National Astronomical Research Institute of Thailand
  • Technical University of Munich
  • Chongqing University

Research output: Contribution to journalReview articlepeer-review

304 Scopus citations

Abstract

The Jiangmen Underground Neutrino Observatory (JUNO) is a 20 kton liquid scintillator detector in a laboratory at 700-m underground. An excellent energy resolution and a large fiducial volume offer exciting opportunities for addressing many important topics in neutrino and astro-particle physics. With six years of data, the neutrino mass ordering can be determined at a 3–4σ significance and the neutrino oscillation parameters sin2θ12, Δm21 2, and |Δm32 2| can be measured to a precision of 0.6% or better, by detecting reactor antineutrinos from the Taishan and Yangjiang nuclear power plants. With ten years of data, neutrinos from all past core-collapse supernovae could be observed at a 3σ significance; a lower limit of the proton lifetime, 8.34×1033 years (90% C.L.), can be set by searching for p→ν̄K+; detection of solar neutrinos would shed new light on the solar metallicity problem and examine the vacuum-matter transition region. A typical core-collapse supernova at a distance of 10 kpc would lead to ∼5000 inverse-beta-decay events and ∼2000 (300) all-flavor neutrino–proton (electron) elastic scattering events in JUNO. Geo-neutrinos can be detected with a rate of ∼400 events per year. Construction of the detector is very challenging. In this review, we summarize the final design of the JUNO detector and the key R&D achievements, following the Conceptual Design Report in 2015 (Djurcic et al., 2015). All 20-inch PMTs have been procured and tested. The average photon detection efficiency is 28.9% for the 15,000 MCP PMTs and 28.1% for the 5000 dynode PMTs, higher than the JUNO requirement of 27%. Together with the >20 m attenuation length of the liquid scintillator achieved in a 20-ton pilot purification test and the >96% transparency of the acrylic panel, we expect a yield of 1345 photoelectrons per MeV and an effective relative energy resolution of 3.02%/E(MeV ) in simulations (Abusleme et al., 2021). To maintain the high performance, the underwater electronics is designed to have a loss rate <0.5% in six years. With degassing membranes and a micro-bubble system, the radon concentration in the 35 kton water pool could be lowered to <10 mBq/m3. Acrylic panels of radiopurity <0.5 ppt U/Th for the 35.4-m diameter liquid scintillator vessel are produced with a dedicated production line. The 20 kton liquid scintillator will be purified onsite with Alumina filtration, distillation, water extraction, and gas stripping. Together with other low background handling, singles in the fiducial volume can be controlled to ∼10Hz. The JUNO experiment also features a double calorimeter system with 25,600 3-inch PMTs, a liquid scintillator testing facility OSIRIS, and a near detector TAO.

Original languageEnglish
Article number103927
JournalProgress in Particle and Nuclear Physics
Volume123
DOIs
StatePublished - Mar 2022

Keywords

  • JUNO
  • neutrino detector
  • neutrino physics

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