The projected background for the CUORE experiment
Creators: name: CUORE Collaboration
name: Alduino, C.
name: Alfonso, K.
name: Artusa, D. R.
name: Avignone, F. T.
name: Azzolini, O.
name: Banks, T. I.
name: Bari, G.
name: Beeman, J. W.
name: Bellini, F.
name: Benato, G.
name: Bersani, A.
name: Biassoni, M.
name: Branca, A.
name: Brofferio, C.
name: Bucci, C.
name: Camacho, A.
name: Caminata, A.
name: Canonica, L.
name: Cao, X. G.
name: Capelli, S.
name: Cappelli, L.
name: Carbone, L.
name: Cardani, L.
name: Carniti, P.
name: Casali, N.
name: Cassina, L.
name: Chiesa, D.
name: Chott, N.
name: Clemenza, M.
name: Copello, S.
name: Cosmelli, C.
name: Cremonesi, O.
name: Creswick, R. J.
name: Cushman, J. S.
name: D'Addabbo, A.
name: Dafinei, I.
name: Davis, C. J.
name: Dell'Oro, S.
name: Deninno, M. M.
name: Di Domizio, S.
name: Di Vacri, M. L.
name: Drobizhev, A.
name: Fang, D. Q.
name: Faverzani, M.
name: Fernandes, G.
name: Ferri, E.
name: Ferroni, F.
name: Fiorini, E.
name: Franceschi, M. A.
name: Freedman, S. J.
name: Fujikawa, B. K.
name: Giachero, A.
name: Gironi, L.
name: Giuliani, A.
name: Gladstone, L.
name: Gorla, P.
name: Gotti, C.
name: Gutierrez, T. D.
name: Haller, E. E.
name: Han, K.
name: Hansen, E.
name: Heeger, K. M.
name: Hennings-Yeomans, R.
name: Hickerson, K. P.
name: Huang, H. Z.
name: Kadel, R.
name: Keppel, G.
name: Kolomensky, Yu. G.
name: Leder, A.
name: Ligi, C.
name: Lim, K. E.
name: Ma, Y. G.
name: Maino, M.
name: Marini, L.
name: Martinez, M.
name: Maruyama, R. H.
name: Mei, Y.
name: Moggi, N.
name: Morganti, S.
name: Mosteiro, P. J.
name: Napolitano, T.
name: Nastasi, M.
name: Nones, C.
name: Norman, E. B.
name: Novati, V.
name: Nucciotti, A.
name: O'Donnell, T.
name: Ouellet, J. L.
name: Pagliarone, C. E.
name: Pallavicini, M.
name: Palmieri, V.
name: Pattavina, L.
name: Pavan, M.
name: Pessina, G.
name: Pettinacci, V.
name: Piperno, G.
name: Pira, C.
name: Pirro, S.
name: Pozzi, S.
name: Previtali, E.
name: Rosenfeld, C.
name: Rusconi, C.
name: Sakai, M.
name: Sangiorgio, S.
name: Santone, D.
name: Schmidt, B.
name: Schmidt, J.
name: Scielzo, N. D.
name: Singh, V.
name: Sisti, M.
name: Smith, A. R.
name: Taffarello, L.
name: Tenconi, M.
name: Terranova, F.
name: Tomei, C.
name: Trentalange, S.
name: Vignati, M.
name: Wagaarachchi, S. L.
name: Wang, B. S.
name: Wang, H. W.
name: Welliver, B.
name: Wilson, J.
name: Winslow, L. A.
name: Wise, T.
name: Woodcraft, A.
name: Zanotti, L.
name: Zhang, G. Q.
name: Zhu, B. X.
name: Zimmermann, S.
name: Zucchelli, S.
name: Laubenstein, M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: The Cryogenic Underground Observatory for Rare Events (CUORE) is designed to search for neutrinoless double beta decay of 130Te with an array of 988 TeO2 bolometers operating at temperatures around 10 mK. The experiment is currently being commissioned in Hall A of Laboratori Nazionali del Gran Sasso, Italy. The goal of CUORE is to reach a 90\% C.L. exclusion sensitivity on the \tect decay half-life of 9$\times$10$^{25}$ years after 5\,years of data taking. The main issue to be addressed to accomplish this aim is the rate of background events in the region of interest, which must not be higher than 10$^{-2}$\,counts/keV/kg/y. We developed a detailed Monte Carlo simulation, based on results from a campaign of material screening, radioassays, and bolometric measurements, to evaluate the expected background. This was used over the years to guide the construction strategies of the experiment and we use it here to project a background model for CUORE. In this paper we report the results of our study and our expectations for the background rate in the energy region where the peak signature of neutrinoless double beta decay of 130Te is expected.
description: 17 pages, 7 figures, matches published version