The low energy spectrum of TeO2 bolometers: results and dark matter perspectives for the CUORE-0 and CUORE experiments

Authors
  • The CUORE collaboration
  • F. Alessandria
  • R. Ardito
  • D. R. Artusa
  • F. T. Avignone
  • O. Azzolini
  • M. Balata
  • T.I. Banks
  • G. Bari
  • J. Beeman
  • F. Bellini
  • A. Bersani
  • M. Biassoni
  • T. Bloxham
  • C. Brofferio
  • C. Bucci
  • X. Z. Cai
  • L. Canonica
  • S. Capelli
  • L. Carbone
  • L. Cardani
  • M. Carrettoni
  • N. Casali
  • N. Chott
  • M. Clemenza
  • C. Cosmelli
  • O. Cremonesi
  • R. J. Creswick
  • I. Dafinei
  • A. Dally
  • V. Datskov
  • A. De Biasi
  • M. P. Decowski
  • M. M. Deninno
  • S. Di Domizio
  • M. L. Di Vacri
  • L. Ejzak
  • R. Faccini
  • D. Q. Fang
  • H. A. Farach
  • E. Ferri
  • F. Ferroni
  • E. Fiorini
  • M. A. Franceschi
  • S.J. Freedman
  • B.K. Fujikawa
  • A. Giachero
  • L. Gironi
  • A. Giuliani
  • J. Goett
  • P. Gorla
Publication date 01-2013
Journal Journal of Cosmology and Astroparticle Physics
Volume | Issue number 2013 | 1
Number of pages 15
Organisations
  • Faculty of Science (FNWI) - Institute of Physics (IoP) - Institute for Theoretical Physics Amsterdam (ITFA)
  • Faculty of Science (FNWI)
  • Faculty of Science (FNWI) - Institute of Physics (IoP) - Institute for High Energy Physics (IHEF)
  • Faculty of Science (FNWI) - Institute of Physics (IoP)
Abstract

We collected 19.4 days of data from four 750 g TeO2 bolometers, and in three of them we were able to set the energy threshold around 3 keV using a new analysis technique. We found a background rate ranging from 25 cpd/keV/kg at 3 keV to 2 cpd/keV/kg at 25 keV, and a peak at 4.7 keV. The origin of this peak is presently unknown, but its presence is confirmed by a reanalysis of 62.7 kg·days of data from the finished CUORICINO experiment. Finally, we report the expected sensitivities of the CUORE-0 (52 bolometers) and CUORE (988 bolometers) experiments to a WIMP annual modulation signal.

Document type Article
Language English
Published at https://doi.org/10.1088/1475-7516/2013/01/038
Other links https://www.scopus.com/pages/publications/84873648220
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