JUNO Non-oscillation Physics
arXiv:2110.09263 · doi:10.1088/1742-6596/2156/1/012109
Abstract
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.
arXiv comment5 pages, 6 figures. Proceeding for the 17th International Conference on Topics in Astroparticle and Underground Physics
References in corpus (7)
- Neutrino Physics with JUNO
- Atmospheric neutrino flux calculation using the NRLMSISE00 atmospheric model
- JUNO Conceptual Design Report
- Measurements of the atmospheric neutrino flux by Super-Kamiokande: energy spectra, geomagnetic effects, and solar modulation
- JUNO sensitivity to low energy atmospheric neutrino spectra
- GIGJ: a crustal gravity model of the Guangdong Province for predicting the geoneutrino signal at the JUNO experiment
- JUNO Physics and Detector