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Journal Articles Journal of Cosmology and Astroparticle Physics Year : 2013

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

F. Alessandria , R. Ardito , D. R. Artusa , F. T. Avignone Iii , 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 , G. Frossati , B. K. Fujikawa , A. Giachero , L. Gironi , A. Giuliani (1) , J. J. Goett , P. Gorla , C. Gotti , E. Guardincerri , T. D. Gutierrez , E. E. Haller , K. Han , K. M. Heeger , H. Z. Huang , R. Kadel , K. Kazkaz , G. Keppel , L. Kogler , Yu. G. Kolomensky , D. Lenz , Y. L. Li , C. Ligi , X. Liu , Y. G. Ma , C. Maiano , M. Maino , M. Martinez , R. H. Maruyama , N. Moggi , S. Morganti , T. Napolitano , S. Newman , S. Nisi , C. Nones (1) , E. B. Norman , A. Nucciotti , F. Orio , D. Orlandi , J. L. Ouellet , M. Pallavicini , V. Palmieri , L. Pattavina , M. Pavan , M. Pedretti , G. Pessina , S. Pirro , E. Previtali , V. Rampazzo , F. Rimondi , C. Rosenfeld , C. Rusconi , S. Sangiorgio , N. D. Scielzo , M. Sisti , A. R. Smith , F. Stivanello , L. Taffarello , M. Tenconi (1) , W. D. Tian , C. Tomei , S. Trentalange , G. Ventura , M. Vignati , B. S. Wang , H. W. Wang , C. A. Whitten Jr. , y T. Wise , A. Woodcraft , L. Zanotti , C. Zarra , B. X. Zhu , S. Zucchelli
F. Alessandria
  • Function : Author
R. Ardito
  • Function : Author
D. R. Artusa
  • Function : Author
F. T. Avignone Iii
  • Function : Author
O. Azzolini
  • Function : Author
M. Balata
  • Function : Author
T. I. Banks
  • Function : Author
G. Bari
  • Function : Author
J. Beeman
  • Function : Author
F. Bellini
  • Function : Author
A. Bersani
  • Function : Author
M. Biassoni
  • Function : Author
T. Bloxham
  • Function : Author
C. Brofferio
  • Function : Author
C. Bucci
  • Function : Author
X. Z. Cai
  • Function : Author
L. Canonica
  • Function : Author
S. Capelli
  • Function : Author
L. Carbone
  • Function : Author
L. Cardani
  • Function : Author
M. Carrettoni
  • Function : Author
N. Casali
  • Function : Author
N. Chott
  • Function : Author
M. Clemenza
  • Function : Author
C. Cosmelli
  • Function : Author
O. Cremonesi
  • Function : Author
R. J. Creswick
  • Function : Author
I. Dafinei
  • Function : Author
A. Dally
  • Function : Author
V. Datskov
  • Function : Author
A. de Biasi
  • Function : Author
M. P. Decowski
  • Function : Author
M. M. Deninno
  • Function : Author
S. Di Domizio
  • Function : Author
M. L. Di Vacri
  • Function : Author
L. Ejzak
  • Function : Author
R. Faccini
  • Function : Author
D. Q. Fang
  • Function : Author
H. A. Farach
  • Function : Author
E. Ferri
  • Function : Author
F. Ferroni
  • Function : Author
E. Fiorini
  • Function : Author
M. A. Franceschi
  • Function : Author
S. J. Freedman
  • Function : Author
G. Frossati
  • Function : Author
B. K. Fujikawa
  • Function : Author
A. Giachero
  • Function : Author
L. Gironi
  • Function : Author
A. Giuliani
  • Function : Author
J. J. Goett
  • Function : Author
P. Gorla
  • Function : Author
C. Gotti
  • Function : Author
E. Guardincerri
  • Function : Author
T. D. Gutierrez
  • Function : Author
E. E. Haller
  • Function : Author
K. Han
  • Function : Author
K. M. Heeger
  • Function : Author
H. Z. Huang
  • Function : Author
R. Kadel
  • Function : Author
K. Kazkaz
  • Function : Author
G. Keppel
  • Function : Author
L. Kogler
  • Function : Author
Yu. G. Kolomensky
  • Function : Author
D. Lenz
  • Function : Author
Y. L. Li
  • Function : Author
C. Ligi
  • Function : Author
X. Liu
Y. G. Ma
  • Function : Author
C. Maiano
  • Function : Author
M. Maino
  • Function : Author
M. Martinez
  • Function : Author
R. H. Maruyama
  • Function : Author
N. Moggi
  • Function : Author
S. Morganti
  • Function : Author
T. Napolitano
  • Function : Author
S. Newman
  • Function : Author
S. Nisi
  • Function : Author
C. Nones
  • Function : Author
E. B. Norman
  • Function : Author
A. Nucciotti
  • Function : Author
F. Orio
  • Function : Author
D. Orlandi
  • Function : Author
J. L. Ouellet
  • Function : Author
M. Pallavicini
V. Palmieri
  • Function : Author
L. Pattavina
  • Function : Author
M. Pavan
  • Function : Author
M. Pedretti
  • Function : Author
G. Pessina
  • Function : Author
S. Pirro
  • Function : Author
E. Previtali
  • Function : Author
V. Rampazzo
  • Function : Author
F. Rimondi
  • Function : Author
C. Rosenfeld
  • Function : Author
C. Rusconi
  • Function : Author
S. Sangiorgio
  • Function : Author
N. D. Scielzo
  • Function : Author
M. Sisti
  • Function : Author
A. R. Smith
  • Function : Author
F. Stivanello
  • Function : Author
L. Taffarello
  • Function : Author
M. Tenconi
  • Function : Author
W. D. Tian
  • Function : Author
C. Tomei
  • Function : Author
S. Trentalange
  • Function : Author
G. Ventura
  • Function : Author
M. Vignati
  • Function : Author
B. S. Wang
  • Function : Author
H. W. Wang
  • Function : Author
C. A. Whitten Jr.
  • Function : Author
y T. Wise
  • Function : Author
A. Woodcraft
  • Function : Author
L. Zanotti
  • Function : Author
C. Zarra
  • Function : Author
B. X. Zhu
  • Function : Author
S. Zucchelli
  • Function : Author

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 CUORE0 (52 bolometers) and CUORE (988 bolometers) experiments to a WIMP annual modulation signal.

Dates and versions

in2p3-00824761 , version 1 (22-05-2013)

Identifiers

Cite

F. Alessandria, R. Ardito, D. R. Artusa, F. T. Avignone Iii, O. Azzolini, et al.. The low energy spectrum of TeO2 bolometers: results and dark matter perspectives for the CUORE-0 and CUORE experiments. Journal of Cosmology and Astroparticle Physics, 2013, pp.038. ⟨10.1088/1475-7516/2013/01/038⟩. ⟨in2p3-00824761⟩
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