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Muon-induced background in the KATRIN main spectrometer
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SYSNO ASEP 0503183 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Muon-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, ORCIDNumber of authors 134 Source Title Astroparticle Physics. - : Elsevier - ISSN 0927-6505
Roč. 108, č. 3 (2019), s. 40-49Number of pages 10 s. Publication form Print - P Language eng - English Country NL - Netherlands Keywords cosmic ray muon backgrounds ; electrostatic spectrometer ; neutrino mass Subject RIV BF - Elementary Particles and High Energy Physics OECD category Particles and field physics R&D Projects LTT18021 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 publishing Open access Institutional support UJF-V - RVO:61389005 UT WOS 000459520800003 EID SCOPUS 85059838543 DOI 10.1016/j.astropartphys.2019.01.003 Annotation The 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. Workplace Nuclear Physics Institute Contact Markéta Sommerová, sommerova@ujf.cas.cz, Tel.: 266 173 228 Year of Publishing 2020 Electronic address https://doi.org/10.1016/j.astropartphys.2019.01.003
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