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. © 2013 IOP Publishing Ltd and Sissa Medialab srl.
Alessandria, F., Ardito, R., Artusa, D., Avignone, F., Azzolini, O., Balata, M., et al. (2013). 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(1) [10.1088/1475-7516/2013/01/038].
The low energy spectrum of TeO2 bolometers: results and dark matter perspectives for the CUORE-0 and CUORE experiments
BIASSONI, MATTEO;BROFFERIO, CHIARA;Canonica, L;CAPELLI, SILVIA;CLEMENZA, MASSIMILIANO;Cremonesi, O;FERRI, ELENA;FIORINI, ETTORE;GIACHERO, ANDREA;GIRONI, LUCA;GOTTI, CLAUDIO;MAINO, MATTEO;NUCCIOTTI, ANGELO ENRICO LODOVICO;Pattavina, L;PAVAN, MAURA;Pessina, G;Previtali, E;SISTI, MONICA;ZANOTTI, LUIGI ERNESTO;
2013
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. © 2013 IOP Publishing Ltd and Sissa Medialab srl.File | Dimensione | Formato | |
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