TY - JOUR
T1 - JUNO physics and detector
AU - JUNO Collaboration
AU - Abusleme, Angel
AU - Adam, Thomas
AU - Ahmad, Shakeel
AU - Ahmed, Rizwan
AU - Aiello, Sebastiano
AU - Akram, Muhammad
AU - An, Fengpeng
AU - An, Guangpeng
AU - An, Qi
AU - Andronico, Giuseppe
AU - Anfimov, Nikolay
AU - Antonelli, Vito
AU - Antoshkina, Tatiana
AU - Asavapibhop, Burin
AU - de Andre, Joao Pedro Athayde Marcondes
AU - Auguste, Didier
AU - Babic, Andrej
AU - Baldini, Wander
AU - Barresi, Andrea
AU - Baussan, Eric
AU - Bellato, Marco
AU - Bergnoli, Antonio
AU - Bernieri, Enrico
AU - Birkenfeld, Thilo
AU - Blin, Sylvie
AU - Blum, David
AU - Blyth, Simon
AU - Bolshakova, Anastasia
AU - Bongrand, Mathieu
AU - Bordereau, Clement
AU - Breton, Dominique
AU - Brigatti, Augusto
AU - Brugnera, Riccardo
AU - Bruno, Riccardo
AU - Budano, Antonio
AU - Buscemi, Mario
AU - Busto, Jose
AU - Butorov, Ilya
AU - Cabrera, Anatael
AU - Cai, Hao
AU - Cai, Xiao
AU - Cai, Yanke
AU - Cai, Zhiyan
AU - Cammi, Antonio
AU - Campeny, Agustin
AU - Cao, Chuanya
AU - Cao, Guofu
AU - Cao, Jun
AU - Caruso, Rossella
AU - Oberauer, Lothar
N1 - Publisher Copyright:
© 2021 Elsevier B.V.
PY - 2022/3
Y1 - 2022/3
N2 - 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.
AB - 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.
KW - JUNO
KW - neutrino detector
KW - neutrino physics
UR - http://www.scopus.com/inward/record.url?scp=85121911413&partnerID=8YFLogxK
U2 - 10.1016/j.ppnp.2021.103927
DO - 10.1016/j.ppnp.2021.103927
M3 - Review article
AN - SCOPUS:85121911413
SN - 0146-6410
VL - 123
JO - Progress in Particle and Nuclear Physics
JF - Progress in Particle and Nuclear Physics
M1 - 103927
ER -