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The projected background for the CUORE experiment

Authors :
CUORE Collaboration
Alduino, C.
Alfonso, K.
Artusa, D. R.
Avignone, F. T.
Azzolini, O.
Banks, T. I.
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.
Carbone, 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.
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.
Fernandes, G.
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.
Hickerson, K. P.
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.
Pettinacci, V.
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.
Tenconi, M.
Terranova, F.
Tomei, C.
Trentalange, S.
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.
Zhu, B. X.
Zimmermann, S.
Zucchelli, S.
Laubenstein, M.
Alduino, C
Alfonso, K
Artusa, D
Avignone, F
Azzolini, O
Banks, T
Bari, G
Beeman, J
Bellini, F
Benato, G
Bersani, A
Biassoni, M
Branca, A
Brofferio, C
Bucci, C
Camacho, A
Caminata, A
Canonica, L
Cao, X
Capelli, S
Cappelli, L
Carbone, L
Cardani, L
Carniti, P
Casali, N
Cassina, L
Chiesa, D
Chott, N
Clemenza, M
Copello, S
Cosmelli, C
Cremonesi, O
Creswick, R
Cushman, J
D’addabbo, A
Dafinei, I
Davis, C
Dell’oro, S
Deninno, M
Di Domizio, S
Di Vacri, M
Drobizhev, A
Fang, D
Faverzani, M
Fernandes, G
Ferri, E
Ferroni, F
Fiorini, E
Franceschi, M
Freedman, S
Fujikawa, B
Giachero, A
Gironi, L
Giuliani, A
Gladstone, L
Gorla, P
Gotti, C
Gutierrez, T
Haller, E
Han, K
Hansen, E
Heeger, K
Hennings Yeomans, R
Hickerson, K
Huang, H
Kadel, R
Keppel, G
Kolomensky, Y
Leder, A
Ligi, C
Lim, K
Ma, Y
Maino, M
Marini, L
Martinez, M
Maruyama, R
Mei, Y
Moggi, N
Morganti, S
Mosteiro, P
Napolitano, T
Nastasi, M
Nones, C
Norman, E
Novati, V
Nucciotti, A
O’donnell, T
Ouellet, J
Pagliarone, C
Pallavicini, M
Palmieri, V
Pattavina, L
Pavan, M
Pessina, G
Pettinacci, V
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
Singh, V
Sisti, M
Smith, A
Taffarello, L
Tenconi, M
Terranova, F
Tomei, C
Trentalange, S
Vignati, M
Wagaarachchi, S
Wang, B
Wang, H
Welliver, B
Wilson, J
Winslow, L
Wise, T
Woodcraft, A
Zanotti, L
Zhang, G
Zhu, B
Zimmermann, S
Zucchelli, S
Laubenstein, M
Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM)
Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Département de Physique des Particules (ex SPP) (DPP)
Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
CUORE
Département de Physique des Particules (ex SPP) (DPhP)
Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Centre de Sciences Nucléaires et de Sciences de la Matière ( CSNSM )
Université Paris-Sud - Paris 11 ( UP11 ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS )
Département de Physique des Particules (ex SPP) ( DPP )
Institut de Recherches sur les lois Fondamentales de l'Univers ( IRFU )
Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay
Alduino, C.
Alfonso, K.
Artusa, D. R.
Avignone, F. T.
Azzolini, O.
Banks, T. I.
Bari, G.
Beeman, J. W.
Bellini, F.
Benato, G.
Bersani, A.
Biassoni, M.
Branca, A.
Brofferio, C.
Bucci, C.
A., Camacho
Caminata, A.
Canonica, L.
Cao, X. G.
Capelli, S.
Cappelli, L.
Carbone, 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.
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.
G., Fernande
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.
Hickerson, K. P.
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.
Pettinacci, V.
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.
Tenconi, M.
Terranova, F.
Tomei, C.
Trentalange, S.
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.
Zhu, B. X.
S., Zimmermann
Zucchelli, S.
Laubenstein, M.
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
Canonica, Lucia
Gladstone, Laura
Leder, Alexander Friedrich
Ouellet, Jonathan L
Winslow, Lindley
Source :
Eur.Phys.J.C, Eur.Phys.J.C, 2017, 77 (8), pp.543. ⟨10.1140/epjc/s10052-017-5080-6⟩, BASE-Bielefeld Academic Search Engine, European Physical Journal C: Particles and Fields, European Physical Journal C: Particles and Fields, Springer Verlag (Germany), 2017, 77 (8), pp.543. ⟨10.1140/epjc/s10052-017-5080-6⟩, Eur.Phys.J.C, 2017, 77 (8), pp.543. 〈10.1140/epjc/s10052-017-5080-6〉, Zaguán. Repositorio Digital de la Universidad de Zaragoza, instname, TopicHub SCOAP3, European Physical Journal C: Particles and Fields, Vol 77, Iss 8, Pp 1-16 (2017), European Physical Journal C
Publication Year :
2017
Publisher :
Springer New York LLC, 2017.

Abstract

The Cryogenic Underground Observatory for Rare Events (CUORE) is designed to search for neutrinoless double beta decay of ¹³⁰ Te 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 ¹³⁰ Te decay half-life of 9 × 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/year. 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 130 Te is expected.<br />National Science Foundation (U.S.) (Grant NSF-PHY-0605119)<br />National Science Foundation (U.S.) (Grant NSF-PHY-0500337)<br />National Science Foundation (U.S.) (Grant NSF-PHY-0855314)<br />National Science Foundation (U.S.) (Grant NSF-PHY-0902171)<br />National Science Foundation (U.S.) (Grant NSF-PHY-0969852)<br />National Science Foundation (U.S.) (Grant NSF-PHY-1307204)<br />National Science Foundation (U.S.) (Grant NSF-PHY-1314881)<br />National Science Foundation (U.S.) (Grant NSF-PHY-1401832)<br />National Science Foundation (U.S.) (Grant NSF-PHY-1404205)

Details

Language :
English
ISSN :
14346044 and 14346052
Database :
OpenAIRE
Journal :
Eur.Phys.J.C, Eur.Phys.J.C, 2017, 77 (8), pp.543. ⟨10.1140/epjc/s10052-017-5080-6⟩, BASE-Bielefeld Academic Search Engine, European Physical Journal C: Particles and Fields, European Physical Journal C: Particles and Fields, Springer Verlag (Germany), 2017, 77 (8), pp.543. ⟨10.1140/epjc/s10052-017-5080-6⟩, Eur.Phys.J.C, 2017, 77 (8), pp.543. 〈10.1140/epjc/s10052-017-5080-6〉, Zaguán. Repositorio Digital de la Universidad de Zaragoza, instname, TopicHub SCOAP3, European Physical Journal C: Particles and Fields, Vol 77, Iss 8, Pp 1-16 (2017), European Physical Journal C
Accession number :
edsair.doi.dedup.....4cc5804d00da73a4ff081854f58d2211