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001     911292
005     20221114130838.0
024 7 _ |a 10.22323/1.398.0229
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024 7 _ |a 2128/32539
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037 _ _ |a FZJ-2022-04585
100 1 _ |a Göttel, Alexandre
|0 P:(DE-Juel1)177019
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111 2 _ |a The European Physical Society Conference on High Energy Physics
|c Online conference
|d 2021-07-26 - 2021-07-30
|w jointly organized by Universität Hamburg and the research center DESY
245 _ _ |a JUNO potential in non-oscillation physics
260 _ _ |c 2022
|b Sissa Medialab Trieste, Italy
295 1 0 |a Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021) - Sissa Medialab Trieste, Italy, 2022. - ISBN - doi:10.22323/1.398.0229
300 _ _ |a Volume 398
336 7 _ |a CONFERENCE_PAPER
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520 _ _ |a The Jiangmen Underground Neutrino Observatory (JUNO) is a next-generation liquid scintillator experiment being built in the Guangdong province in China. JUNO's target mass of 20 kton will be contained in a 35.4 m acrylic vessel, itself submerged in a water pool, under about 700 m of granite overburden. Surrounding the acrylic vessel are 17612 20'' PMTs and 25600 3'' PMTs. The main goal of JUNO, whose construction is scheduled for completion in 2022, is a 3-4σ determination of the neutrino mass ordering (MO) using reactor neutrinos within six years, as well as a precise measurement of $θ_{12}$, $Δm^2_{21}$, and $Δm^2_{31}$. JUNO's large target mass, low background, and dual calorimetry, leading to an excellent energy resolution and low threshold, allows for a rich physics program with many applications in neutrino physics. The large target mass will allow for high-statistics solar-, geo-, and atmospheric neutrino measurements. JUNO will also be able to measure neutrinos from galactic core-collapse supernovae, detecting about 10,000 events for a supernova at 10 kpc, and achieve a 3σ discovery of the diffuse supernova neutrino background in ten years. It can also study non-standard interactions e.g. proton decay, indirect dark matter searches, and probe for Lorentz invariance violations. This paper covers this extensive range of non-oscillation topics on which JUNO will be able to shed light.
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856 4 _ |u https://juser.fz-juelich.de/record/911292/files/EPS-HEP2021_229.pdf
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