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dc.contributor.authorGladstone, Laura
dc.contributor.authorWinslow, Lindley
dc.contributor.authorHansen, E.
dc.contributor.authorLeder, Alexander Friedrich
dc.contributor.authorCononica, Lucia
dc.date.accessioned2018-11-14T15:20:17Z
dc.date.available2018-11-14T15:20:17Z
dc.date.issued2018-09
dc.date.submitted2018-09
dc.identifier.issn1434-6044
dc.identifier.issn1434-6052
dc.identifier.urihttp://hdl.handle.net/1721.1/118999
dc.description.abstractCUORE is a tonne-scale cryogenic detector operating at the Laboratori Nazionali del Gran Sasso (LNGS) that uses tellurium dioxide bolometers to search for neutrinoless double-beta decay of130Te. CUORE is also suitable to search for low energy rare events such as solar axions or WIMP scattering, thanks to its ultra-low background and large target mass. However, to conduct such sensitive searches requires improving the energy threshold to 10 keV. In this paper, we describe the analysis techniques developed for the low energy analysis of CUORE-like detectors, using the data acquired from November 2013 to March 2015 by CUORE-0, a single-tower prototype designed to validate the assembly procedure and new cleaning techniques of CUORE. We explain the energy threshold optimization, continuous monitoring of the trigger efficiency, data and event selection, and energy calibration at low energies in detail. We also present the low energy background spectrum of CUORE-0 below 60keV. Finally, we report the sensitivity of CUORE to WIMP annual modulation using the CUORE-0 energy threshold and background, as well as an estimate of the uncertainty on the nuclear quenching factor from nuclear recoils inCUORE-0.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant NSFPHY-0605119)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant NSF-PHY-0500337)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant NSF-PHY-0855314)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant NSF-PHY0902171)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant NSF-PHY-0969852)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant NSF-PHY-1307204)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant NSF-PHY1404205)en_US
dc.description.sponsorshipAlfred P. Sloan Foundationen_US
dc.description.sponsorshipUniversity of Wisconsin Foundationen_US
dc.description.sponsorshipYale Universityen_US
dc.publisherSpringer Natureen_US
dc.relation.isversionofhttp://dx.doi.org/10.1140/EPJC/S10052-017-5433-1en_US
dc.rightsCreative Commons Attribution 4.0 International Licenseen_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.sourceSpringeren_US
dc.titleLow energy analysis techniques for CUOREen_US
dc.typeArticleen_US
dc.identifier.citationAlduino, C., et al. “Low Energy Analysis Techniques for CUORE.” The European Physical Journal C, vol. 77, no. 12, Dec. 2017. © 2017 The Authorsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.mitauthorGladstone, Laura
dc.contributor.mitauthorWinslow, Lindley
dc.contributor.mitauthorHansen, E.
dc.contributor.mitauthorLeder, Alexander Friedrich
dc.contributor.mitauthorCononica, Lucia
dc.relation.journalThe European Physical Journal Cen_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.updated2018-10-11T16:38:41Z
dspace.orderedauthorsAlduino, C.; Alfonso, K.; Artusa, D. R.; Avignone, F. T.; Azzolini, O.; Bari, G.; Beeman, J. W.; Bellini, F.; Benato, G.; Bersani, A.; Biassoni, M.; Branca, A.; Brofferio, C.; Bucci, C.; Camacho, A.; Caminata, A.; Canonica, L.; Cao, X. G.; Capelli, S.; Cappelli, L.; Cardani, L.; Carniti, P.; Casali, N.; Cassina, L.; Chiesa, D.; Chott, N.; Clemenza, M.; Copello, S.; Cosmelli, C.; Cremonesi, O.; Creswick, R. J.; Cushman, J. S.; D’Addabbo, A.; D’Aguanno, D.; Dafinei, I.; Davis, C. J.; Dell’Oro, S.; Deninno, M. M.; Di Domizio, S.; Di Vacri, M. L.; Drobizhev, A.; Fang, D. Q.; Faverzani, M.; Ferri, E.; Ferroni, F.; Fiorini, E.; Franceschi, M. A.; Freedman, S. J.; Fujikawa, B. K.; Giachero, A.; Gironi, L.; Giuliani, A.; Gladstone, L.; Gorla, P.; Gotti, C.; Gutierrez, T. D.; Haller, E. E.; Han, K.; Hansen, E.; Heeger, K. M.; Hennings-Yeomans, R.; Huang, H. Z.; Kadel, R.; Keppel, G.; Kolomensky, Yu. G.; Leder, A.; Ligi, C.; Lim, K. E.; Ma, Y. G.; Maino, M.; Marini, L.; Martinez, M.; Maruyama, R. H.; Mei, Y.; Moggi, N.; Morganti, S.; Mosteiro, P. J.; Napolitano, T.; Nastasi, M.; Nones, C.; Norman, E. B.; Novati, V.; Nucciotti, A.; O’Donnell, T.; Ouellet, J. L.; Pagliarone, C. E.; Pallavicini, M.; Palmieri, V.; Pattavina, L.; Pavan, M.; Pessina, G.; Piperno, G.; Pira, C.; Pirro, S.; Pozzi, S.; Previtali, E.; Rosenfeld, C.; Rusconi, C.; Sakai, M.; Sangiorgio, S.; Santone, D.; Schmidt, B.; Schmidt, J.; Scielzo, N. D.; Singh, V.; Sisti, M.; Smith, A. R.; Taffarello, L.; Terranova, F.; Tomei, C.; Vignati, M.; Wagaarachchi, S. L.; Wang, B. S.; Wang, H. W.; Welliver, B.; Wilson, J.; Winslow, L. A.; Wise, T.; Woodcraft, A.; Zanotti, L.; Zhang, G. Q.; Zimmermann, S.; Zucchelli, S.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-0195-2295
dc.identifier.orcidhttps://orcid.org/0000-0002-9970-108X
dc.identifier.orcidhttps://orcid.org/0000-0003-1429-1104
mit.licensePUBLISHER_CCen_US


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