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dc.contributor.authorBuzinsky, Nicholas Gregory
dc.contributor.authorFormaggio, Joseph A
dc.contributor.authorSibille, Valerian
dc.date.accessioned2019-09-25T20:40:46Z
dc.date.available2019-09-25T20:40:46Z
dc.date.issued2019-03
dc.date.submitted2018-12
dc.identifier.issn0927-6505
dc.identifier.urihttps://hdl.handle.net/1721.1/122293
dc.description.abstractThe 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 β-particles from tritium β-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. Keywords: Cosmic-ray muon backgrounds; Electrostatic spectrometer; Neutrino massen_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-FG02-97ER41020)en_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-FG02-94ER40818)en_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-SC0004036)en_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-FG02-97ER41033)en_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-FG02-97ER41041)en_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-AC02-05CH11231)en_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-SC0011091)en_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-SC0019304)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1016/j.astropartphys.2019.01.003en_US
dc.rightsCreative Commons Attribution 4.0 International licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceElsevieren_US
dc.titleMuon-induced background in the KATRIN main spectrometeren_US
dc.typeArticleen_US
dc.identifier.citationAltenmüller, K. et al. "Muon-induced background in the KATRIN main spectrometer." Astroparticle Physics 108 (March 2019): 40-49 © 2019 The Authorsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Laboratory for Nuclear Scienceen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Nuclear Science and Engineeringen_US
dc.relation.journalAstroparticle Physicsen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2019-03-21T18:44:23Z
dspace.orderedauthorsAltenmüller, K.; Arenz, M.; Baek, W.-J.; Beck, M.; Beglarian, A.; Behrens, J.; Bergmann, T.; Berlev, A.; Besserer, U.; Blaum, K.; Bobien, S.; Bode, T.; Bornschein, B.; Bornschein, L.; Brunst, T.; Buzinsky, N.; Chilingaryan, S.; Choi, W.Q.; Deffert, M.; Doe, P.J.; Dragoun, O.; Drexlin, G.; Dyba, S.; Edzards, F.; Eitel, K.; Ellinger, E.; Engel, R.; Enomoto, S.; Erhard, M.; Eversheim, D.; Fedkevych, M.; Formaggio, J.A.; Fränkle, F.M.; Franklin, G.B.; Friedel, F.; Fulst, A.; Gil, W.; Glück, F.; Gonzalez Ureña, A.; Grohmann, S.; Grössle, R.; Gumbsheimer, R.; Hackenjos, M.; Hannen, V.; Harms, F.; Haußmann, N.; Heizmann, F.; Helbing, K.; Herz, W.; Hickford, S.; Hilk, D.; Hillesheimer, D.; Howe, M.A.; Huber, A.; Jansen, A.; Kellerer, J.; Kernert, N.; Kippenbrock, L.; Kleesiek, M.; Klein, M.; Kopmann, A.; Korzeczek, M.; Kovalík, A.; Krasch, B.; Kraus, M.; Kuckert, L.; Lasserre, T.; Lebeda, O.; Leiber, B.; Letnev, J.; Linek, J.; Lokhov, A.; Machatschek, M.; Marsteller, A.; Martin, E.L.; Mertens, S.; Mirz, S.; Monreal, B.; Neumann, H.; Niemes, S.; Off, A.; Osipowicz, A.; Otten, E.; Parno, D.S.; Pollithy, A.; Poon, A.W.P.; Priester, F.; Ranitzsch, P.C.-O.; Rest, O.; Rink, R.; Robertson, R.G.H.; Roccati, F.; Rodenbeck, C.; Röllig, M.; Röttele, C.; Rovedo, P.; Ryšavý, M.; Sack, R.; Saenz, A.; Schimpf, L.; Schlösser, K.; Schlösser, M.; Schönung, K.; Schrank, M.; Seitz-Moskaliuk, H.; Sentkerestiová, J.; Sibille, V.; Slezák, M.; Steidl, M.; Steinbrink, N.; Sturm, M.; Suchopar, M.; Suesser, M.; Telle, H.H.; Thorne, L.A.; Thümmler, T.; Titov, N.; Tkachev, I.; Trost, N.; Valerius, K.; Vénos, D.; Vianden, R.; Vizcaya Hernández, A.P.; Wandkowsky, N.; Weber, M.; Weinheimer, C.; Weiss, C.; Welte, S.; Wendel, J.; Wilkerson, J.F.; Wolf, J.; Wüstling, S.; Zadoroghny, S.; Zeller, G.en_US
dspace.embargo.termsNen_US
dspace.date.submission2019-04-04T10:53:30Z
mit.journal.volume108en_US
mit.licensePUBLISHER_CCen_US


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