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

  1. 1.
    SYSNO ASEP0574847
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleIdentification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector
    Author(s) Abed Abud, A. (CH)
    Abi, B. (GB)
    Acciarri, R. (US)
    Filip, Peter (FZU-D) ORCID
    Kvasnička, Jiří (FZU-D) RID, ORCID
    Lokajíček, Miloš (FZU-D) RID, ORCID
    Pěč, Viktor (FZU-D) ORCID
    Zálešák, Jaroslav (FZU-D) RID, ORCID
    Zuklín, Josef (FZU-D) ORCID
    Number of authors1260
    Article number092012
    Source TitlePhysical Review D. - : American Physical Society - ISSN 2470-0010
    Roč. 107, č. 9 (2023)
    Number of pages22 s.
    Languageeng - English
    CountryUS - United States
    Keywordsnumerical calculations: Monte Carlo ; threshold: effect ; electronics: readout
    Subject RIVBF - Elementary Particles and High Energy Physics
    OECD categoryParticles and field physics
    Research InfrastructureCERN-CZ III - 90240 - Fyzikální ústav AV ČR, v. v. i.
    Method of publishingOpen access
    Institutional supportFZU-D - RVO:68378271
    UT WOS001010953400003
    EID SCOPUS85162211963
    DOI10.1103/PhysRevD.107.092012
    AnnotationMeasurements 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.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2024
    Electronic addresshttps://hdl.handle.net/11104/0350511
Number of the records: 1  

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