Neutrino interaction classification with convolutional neural network in the DUNE far detector
dc.contributor.author | abi, babak | |
dc.contributor.author | Acciarri, Roberto | |
dc.contributor.author | Acero O, Mario A | |
dc.contributor.author | Adamov, G | |
dc.contributor.author | Adams, David | |
dc.contributor.author | Adinolfi, M | |
dc.contributor.author | Ahmad, Z | |
dc.contributor.author | Szczerbinska, Barbara | |
dc.creator.orcid | http://orcid.org/0000-0003-4477-4350 | en_US |
dc.creator.orcid | http://orcid.org/0000-0003-4477-4350 | |
dc.date.accessioned | 2022-10-12T21:02:12Z | |
dc.date.available | 2022-10-12T21:02:12Z | |
dc.date.issued | 2020-09-16 | |
dc.description.abstract | The Deep Underground Neutrino Experiment is a next-generation neutrino oscillation experiment that aims to measure CP-violation in the neutrino sector as part of a wider physics program. A deep learning approach based on a convolutional neural network has been developed to provide highly efficient and pure selections of electron neutrino and muon neutrino charged-current interactions. The electron neutrino (antineutrino) selection efficiency peaks at 90% (94%) and exceeds 85% (90%) for reconstructed neutrino energies between 2–5 GeV. The muon neutrino (antineutrino) event selection is found to have a maximum efficiency of 96% (97%) and exceeds 90% (95%) efficiency for reconstructed neutrino energies above 2 GeV. When considering all electron neutrino and antineutrino interactions as signal, a selection purity of 90% is achieved. These event selections are critical to maximize the sensitivity of the experiment to CP-violating effects. | en_US |
dc.description.sponsorship | This document was prepared by the DUNE Collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, Institute of Particle Physics and NSERC, Canada; CERN; MŠMT, Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; Comunidad de Madrid, Fundación “La Caixa” and MICINN, Spain; State Secretariat for Education, Research and Innovation and SNSF, Switzerland; TÜBİTAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America. | en_US |
dc.identifier.citation | B. Abi, B. Szczerbinska, et al. (DUNE Collaboration) Phys. Rev. D 102 https://doi.org/10.1103/PhysRevD.102.092003 | en_US |
dc.identifier.doi | https://doi.org/10.1103/PhysRevD.102.092003 | |
dc.identifier.uri | https://hdl.handle.net/1969.6/94078 | |
dc.language.iso | en_US | en_US |
dc.rights | Attribution 4.0 International | * |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | * |
dc.subject | dune | en_US |
dc.subject | deep underground neutrino experiment | en_US |
dc.subject | convolutional neural networks | en_US |
dc.subject | neutrino oscillations | en_US |
dc.title | Neutrino interaction classification with convolutional neural network in the DUNE far detector | en_US |
dc.type | Article | en_US |
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