Issue |
EPJ Web Conf.
Volume 209, 2019
RICAP18, 7th Roma International Conference on Astroparticle Physics
|
|
---|---|---|
Article Number | 01011 | |
Number of page(s) | 4 | |
DOI | https://doi.org/10.1051/epjconf/201920901011 | |
Published online | 13 May 2019 |
https://doi.org/10.1051/epjconf/201920901011
e- discrimination at high energy in the JUNO detector
1 Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre, Via della Vasca Navale 84, 00146 Rome, Italy
2 INFN Sezione di Roma Tre, Via della Vasca Navale 84, 00146 Rome, Italy
a e-mail: giulio.settanta@uniroma3.it
Published online: 13 May 2019
Cosmic Ray and neutrino oscillation physics can be studied by using atmospheric neutrinos. JUNO (Jiangmen Underground Neutrino Observatory) is a large liquid scintillator detector with low energy detection threshold and excellent energy resolution. The detector performances allow the atmospheric neutrino oscillation measurements. In this work, a discrimination algorithm for different reaction channels of neutrino-nucleon interactions in the JUNO liquid scintillator, in the GeV/sub-GeV energy region, is presented. The atmospheric neutrino flux is taken as reference, considering and
. The different temporal behaviour of the classes of events have been exploited to build a timeprofile-based discrimination algorithm. The results show a good selection power for
CC events, while the
CC component suffers of an important contamination from NC events at low energy, which is under study. Preliminary results are presented.
© The Authors, published by EDP Sciences, 2019
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