The Korean Physical Society 06130 22, Teheran-ro 7-gil, Gangnam-gu, Seoul, Republic of Korea 610 Representation : Suk Lyun HONG TEL: 02-556-4737 FAX: 02-554-1643 E-mail : webmaster@kps.or.kr Copyright(C) KPS, All rights reserved.
30 May 2022 to 4 June 2022
Virtual Seoul
Asia/Seoul timezone

Particle identification of atmospheric neutrinos in JUNO

Not scheduled
5m
Virtual Seoul

Virtual Seoul

Poster Atmospheric neutrinos Poster

Description

On behalf of the JUNO Collaboration

The Jiangmen Underground Neutrino Observatory (JUNO) with a 20 kton liquid scintillator (LS) detector is a multi-purpose underground experiment. The neutrino mass ordering (NMO) in JUNO can be determined by measuring atmospheric neutrinos with the matter effect (MSW) and measuring the spectrum modification of reactor anti-neutrinos induced by oscillations with ∆M_31^2, respectively. The two independent methods are complementary, and the joint analysis can greatly increase the NMO sensitivity. Considering the signal efficiency and purity, flavor identification is crucial to the NMO sensitivity of atmospheric neutrino. Based on the high detection efficiency of a LS detector for neutrons, Michel electrons compared with the water Cerenkov detector, we can make full use of these particle distribution information for particle identification (PID). The features extracted in the waveform of the photomultiplier tubes are also used to do the PID analysis. The preliminary PID strategy and results of the atmospheric neutrino based on the multiple machine learning methods will be presented in the poster.

Primary author

Presentation materials