2021/10/18 by Giulio Settanta
Physics and Astronomy · #Astronomy #Astroparticle physics #Dark Matter and Cosmic Phenomena #Dark matter #Detector #Measurements of neutrino speed #Neutrino #Neutrino Physics Research #Neutrino astronomy #Neutrino detector #Neutrino oscillation #Nuclear physics #Observatory #Particle physics #Particle physics theoretical and experimental studies #Physics #Scintillator #Solar neutrino #Solar neutrino problem #Supernova #hep-ex #physics.ins-det
paper · pdf · doi:10.1088/1742-6596/2156/1/012109
5 pages, 6 figures. Proceeding for the 17th International Conference on Topics in Astroparticle and Underground Physics
arxiv created 2021/10/18 · openalex publication_date 2021/12/01 · arxiv updated 2022/03/02 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The JUNO observatory, a 20 kt liquid scintillator detector to be completed in 2022 in China, belongs to the next-generation of neutrino detectors, which share the common features of having a multi-ton scale and an energy resolution at unprecedented levels. Beside the ambitious goal of neutrino mass ordering determination, the JUNO Collaboration plans also to perform a wide series of other measurements in the neutrino and astroparticle fields, rare processes and searches for new physics. The detector characteristics will allow the detection of neutrinos from many sources, like supernovae, the Sun, atmospheric and geoneutrinos. Other potential studies accessible to JUNO include the search for exotic processes, such as nucleon decays, Dark Matter and magnetic monopoles interactions, light sterile neutrinos production. This work reviews the physics potential of JUNO about non-reactor neutrino sources, highlighting the unique contributions that the experiment will give to the various fields in the forthcoming years.