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Muon-induced background in the KATRIN main spectrometer

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    SYSNO ASEP0503183
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleMuon-induced background in the KATRIN main spectrometer
    Author(s) Altenmuller, K. (DE)
    Arenz, M. (DE)
    Baek, W. -J. (DE)
    Beck, M. (DE)
    Beglarian, A. (DE)
    Behrens, J. (DE)
    Bergmann, T. (DE)
    Berlev, A. I. (RU)
    Dragoun, Otokar (UJF-V) RID, SAI
    Kovalík, Alojz (UJF-V) RID, ORCID, SAI
    Lebeda, Ondřej (UJF-V) RID, ORCID, SAI
    Ryšavý, Miloš (UJF-V) RID, ORCID, SAI
    Sentkerestiová, Jana (UJF-V) SAI
    Suchopár, Martin (UJF-V)
    Vénos, Drahoslav (UJF-V) RID, SAI, ORCID
    Number of authors134
    Source TitleAstroparticle Physics. - : Elsevier - ISSN 0927-6505
    Roč. 108, č. 3 (2019), s. 40-49
    Number of pages10 s.
    Publication formPrint - P
    Languageeng - English
    CountryNL - Netherlands
    Keywordscosmic ray muon backgrounds ; electrostatic spectrometer ; neutrino mass
    Subject RIVBF - Elementary Particles and High Energy Physics
    OECD categoryParticles and field physics
    R&D ProjectsLTT18021 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    LM2015056 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    LTT19005 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    Method of publishingOpen access
    Institutional supportUJF-V - RVO:61389005
    UT WOS000459520800003
    EID SCOPUS85059838543
    DOI10.1016/j.astropartphys.2019.01.003
    AnnotationThe KArlsruhe TRItium Neutrino (KATRIN) experiment aims to make a model-independent determination of the effective electron antineutrino mass with a sensitivity of 0.2 eV/c(2). It investigates the kinematics of beta-particles from tritium beta-decay close to the endpoint of the energy spectrum. Because the KATRIN main spectrometer (MS) is located above ground, muon-induced backgrounds are of particular concern. Coincidence measurements with the MS and a scintillator-based muon detector system confirmed the model of secondary electron production by cosmic-ray muons inside the MS. Correlation measurements with the same setup showed that about 12% of secondary electrons emitted from the inner surface are induced by cosmic-ray muons, with approximately one secondary electron produced for every 17 muon crossings. However, the magnetic and electrostatic shielding of the MS is able to efficiently suppress these electrons, and we find that muons are responsible for less than 17% (90% confidence level) of the overall MS background.
    WorkplaceNuclear Physics Institute
    ContactMarkéta Sommerová, sommerova@ujf.cas.cz, Tel.: 266 173 228
    Year of Publishing2020
    Electronic addresshttps://doi.org/10.1016/j.astropartphys.2019.01.003
Number of the records: 1  

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