TY - JOUR
T1 - JUNO Physics Prospects
AU - The JUNO Collaboration
AU - de André, João Pedro Athayde Marcondes
AU - Abusleme, Angel
AU - Adam, Thomas
AU - Ahmad, Shakeel
AU - Ahmed, Rizwan
AU - Aiello, Sebastiano
AU - Akram, Muhammad
AU - An, Fengpeng
AU - An, Qi
AU - Andronico, Giuseppe
AU - Anfimov, Nikolay
AU - Antonelli, Vito
AU - Antoshkina, Tatiana
AU - Asavapibhop, Burin
AU - Auguste, Didier
AU - Babic, Andrej
AU - Balashov, Nikita
AU - Baldini, Wander
AU - Barresi, Andrea
AU - Basilico, Davide
AU - Baussan, Eric
AU - Bellato, Marco
AU - Bergnoli, Antonio
AU - Birkenfeld, Thilo
AU - Blin, Sylvie
AU - Blum, David
AU - Blyth, Simon
AU - Bolshakova, Anastasia
AU - Bongrand, Mathieu
AU - Bordereau, Clément
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 - Callegari, Riccardo
AU - Cammi, Antonio
AU - Campeny, Agustin
AU - Cao, Chuanya
AU - Cao, Guofu
AU - Cao, Jun
AU - Lin, Guey Lin
N1 - Publisher Copyright:
© Copyright owned by the author(s).
PY - 2022/3/18
Y1 - 2022/3/18
N2 - JUNO is a multi-purpose underground neutrino observatory being constructed in the south of China. The main detector, with a 20 kton liquid scintillator target instrumented with about 18k 20” PMT and about 26k 3” PMT, will be strategically located 53 km from the Taishan and Yangjiang Nuclear Power Plants. Using reactor antineutrinos, JUNO will be able to measure several neutrino oscillation parameters with sub-percent precision as well as to determine the neutrino mass ordering to ∼3 σ over 6 years of operation. Furthermore, JUNO will have a broad physics program, ranging from studying neutrinos from other sources, such as solar and supernova neutrinos, to searching for BSM physics such as proton decay. This talk will give an overview on the JUNO’s broad physics potential.
AB - JUNO is a multi-purpose underground neutrino observatory being constructed in the south of China. The main detector, with a 20 kton liquid scintillator target instrumented with about 18k 20” PMT and about 26k 3” PMT, will be strategically located 53 km from the Taishan and Yangjiang Nuclear Power Plants. Using reactor antineutrinos, JUNO will be able to measure several neutrino oscillation parameters with sub-percent precision as well as to determine the neutrino mass ordering to ∼3 σ over 6 years of operation. Furthermore, JUNO will have a broad physics program, ranging from studying neutrinos from other sources, such as solar and supernova neutrinos, to searching for BSM physics such as proton decay. This talk will give an overview on the JUNO’s broad physics potential.
UR - http://www.scopus.com/inward/record.url?scp=85145576619&partnerID=8YFLogxK
M3 - Conference article
AN - SCOPUS:85145576619
SN - 1824-8039
VL - 395
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 1194
T2 - 37th International Cosmic Ray Conference, ICRC 2021
Y2 - 12 July 2021 through 23 July 2021
ER -