Feasibility of detecting B8 solar neutrinos at JUNO

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  • uploaded June 26, 2021

Discussion timeslot (ZOOM-Meeting): 20. July 2021 - 12:00
ZOOM-Meeting URL: https://desy.zoom.us/j/91999581729
ZOOM-Meeting ID: 91999581729
ZOOM-Meeting Passcode: ICRC2021
Corresponding Session: https://icrc2021-venue.desy.de/channel/38-The-Future-of-Neutrino-Telescopes-NU/78
Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-05/6

Abstract:
'In this talk we describe in detail the feasibility of detecting $^8$B solar neutrino at JUNO with three reaction channels (neutrino-electron elastic scattering, neutrino-$^{13}$C charged current, and neutral current interactions). A reduced 2 MeV threshold on the recoil electron energy is achievable with optimized background reduction strategies. The advantage of JUNO for charge and neutral current channel detection is a large amount of $^{13}$C (~0.2 kt). With ten years of data taking, about 60,000 ES signals and 600 NC/CC signal are expected. This leads to a simultaneous measurement of sin$^2theta_{12}$ and $Delta m^2_{21}$ using reactor antineutrinos and solar neutrinos in the JUNO detector.'

Authors: Jie Zhao | for the JUNO Collaboration
Collaboration: JUNO

Indico-ID: 1084
Proceeding URL: https://pos.sissa.it/395/1229

Tags:
Presenter: Jie Zhao

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