Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector

Measurements of electrons from νe interactions are crucial for the Deep Underground Neutrino Experiment (DUNE) neutrino oscillation program, as well as searches for physics beyond the standard model, supernova neutrino detection, and solar neutrino measurements. This article describes the selection...

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Autores: Abud, A. Abed, Amedo, P., Antonova, M., Barenboim, Gabriela, Cervera Villanueva, Anselmo, De Romeri, V., García-Peris, M.A., Martín-Albo, Justo, Martínez-Miravé, Pablo, Mena, Olga, Molina Bueno, Laura, Novella, Pau, Pompa, Federica, Rocabado Rocha, J.L., Sorel, Michel, Tórtola, Mariam, Valle, J.W.F., DUNE Collaboration
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2023
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/364025
Acesso em linha:http://hdl.handle.net/10261/364025
Access Level:acceso abierto
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spelling Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detectorAbud, A. AbedAmedo, P.Antonova, M.Barenboim, GabrielaCervera Villanueva, AnselmoDe Romeri, V.García-Peris, M.A.Martín-Albo, JustoMartínez-Miravé, PabloMena, OlgaMolina Bueno, LauraNovella, PauPompa, FedericaRocabado Rocha, J.L.Sorel, MichelTórtola, MariamValle, J.W.F.DUNE CollaborationMeasurements of electrons from νe interactions are crucial for the Deep Underground Neutrino Experiment (DUNE) neutrino oscillation program, as well as searches for physics beyond the standard model, supernova neutrino detection, and solar neutrino measurements. This article describes the selection and reconstruction of low-energy (Michel) electrons in the ProtoDUNE-SP detector. ProtoDUNE-SP is one of the prototypes for the DUNE far detector, built and operated at CERN as a charged particle test beam experiment. A sample of low-energy electrons produced by the decay of cosmic muons is selected with a purity of 95%. This sample is used to calibrate the low-energy electron energy scale with two techniques. An electron energy calibration based on a cosmic ray muon sample uses calibration constants derived from measured and simulated cosmic ray muon events. Another calibration technique makes use of the theoretically well-understood Michel electron energy spectrum to convert reconstructed charge to electron energy. In addition, the effects of detector response to low-energy electron energy scale and its resolution including readout electronics threshold effects are quantified. Finally, the relation between the theoretical and reconstructed low-energy electron energy spectra is derived, and the energy resolution is characterized. The low-energy electron selection presented here accounts for about 75% of the total electron deposited energy. After the addition of lost energy using a Monte Carlo simulation, the energy resolution improves from about 40% to 25% at 50 MeV. These results are used to validate the expected capabilities of the DUNE far detector to reconstruct low-energy electrons.Peer reviewedAmerican Physical SocietyEuropean CommissionMinisterio de Ciencia e Innovación (España)Generalitat ValencianaAgencia Estatal de Investigación (España)Junta de AndalucíaConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2024202420232024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/364025reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/EC/H2020/754496info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C41info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C42info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C43info:eu-repo/grantAgreement/EC/H2020/101025085http://dx.doi.org/10.1103/PhysRevD.107.092012Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/3640252026-05-22T06:33:51Z
dc.title.none.fl_str_mv Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector
title Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector
spellingShingle Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector
Abud, A. Abed
title_short Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector
title_full Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector
title_fullStr Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector
title_full_unstemmed Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector
title_sort Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector
dc.creator.none.fl_str_mv Abud, A. Abed
Amedo, P.
Antonova, M.
Barenboim, Gabriela
Cervera Villanueva, Anselmo
De Romeri, V.
García-Peris, M.A.
Martín-Albo, Justo
Martínez-Miravé, Pablo
Mena, Olga
Molina Bueno, Laura
Novella, Pau
Pompa, Federica
Rocabado Rocha, J.L.
Sorel, Michel
Tórtola, Mariam
Valle, J.W.F.
DUNE Collaboration
author Abud, A. Abed
author_facet Abud, A. Abed
Amedo, P.
Antonova, M.
Barenboim, Gabriela
Cervera Villanueva, Anselmo
De Romeri, V.
García-Peris, M.A.
Martín-Albo, Justo
Martínez-Miravé, Pablo
Mena, Olga
Molina Bueno, Laura
Novella, Pau
Pompa, Federica
Rocabado Rocha, J.L.
Sorel, Michel
Tórtola, Mariam
Valle, J.W.F.
DUNE Collaboration
author_role author
author2 Amedo, P.
Antonova, M.
Barenboim, Gabriela
Cervera Villanueva, Anselmo
De Romeri, V.
García-Peris, M.A.
Martín-Albo, Justo
Martínez-Miravé, Pablo
Mena, Olga
Molina Bueno, Laura
Novella, Pau
Pompa, Federica
Rocabado Rocha, J.L.
Sorel, Michel
Tórtola, Mariam
Valle, J.W.F.
DUNE Collaboration
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv European Commission
Ministerio de Ciencia e Innovación (España)
Generalitat Valenciana
Agencia Estatal de Investigación (España)
Junta de Andalucía
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
description Measurements of electrons from νe interactions are crucial for the Deep Underground Neutrino Experiment (DUNE) neutrino oscillation program, as well as searches for physics beyond the standard model, supernova neutrino detection, and solar neutrino measurements. This article describes the selection and reconstruction of low-energy (Michel) electrons in the ProtoDUNE-SP detector. ProtoDUNE-SP is one of the prototypes for the DUNE far detector, built and operated at CERN as a charged particle test beam experiment. A sample of low-energy electrons produced by the decay of cosmic muons is selected with a purity of 95%. This sample is used to calibrate the low-energy electron energy scale with two techniques. An electron energy calibration based on a cosmic ray muon sample uses calibration constants derived from measured and simulated cosmic ray muon events. Another calibration technique makes use of the theoretically well-understood Michel electron energy spectrum to convert reconstructed charge to electron energy. In addition, the effects of detector response to low-energy electron energy scale and its resolution including readout electronics threshold effects are quantified. Finally, the relation between the theoretical and reconstructed low-energy electron energy spectra is derived, and the energy resolution is characterized. The low-energy electron selection presented here accounts for about 75% of the total electron deposited energy. After the addition of lost energy using a Monte Carlo simulation, the energy resolution improves from about 40% to 25% at 50 MeV. These results are used to validate the expected capabilities of the DUNE far detector to reconstruct low-energy electrons.
publishDate 2023
dc.date.none.fl_str_mv 2023
2024
2024
2024
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
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status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/364025
url http://hdl.handle.net/10261/364025
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
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info:eu-repo/grantAgreement/EC/H2020/754496
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C41
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C42
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C43
info:eu-repo/grantAgreement/EC/H2020/101025085
http://dx.doi.org/10.1103/PhysRevD.107.092012

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dc.publisher.none.fl_str_mv American Physical Society
publisher.none.fl_str_mv American Physical Society
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