1. CUORE: a cryogenic underground observatory for rare events
- Author
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Arnaboldi, C, Avignone, F, Beemanc, J, Barucci, M, Balata, M, Brofferio, C, Buccie, C, Cebrian, S, Creswick, R, Capelli, S, Carbone, L, Cremonesi, O, de Ward, A, Fiorini, E, Farach, H, Frossati, G, Giuliani, A, Giugni, D, Gorla, P, Haller, E, Irastorza, I, Mcdonald, R, Morales, A, Norman, E, Negri, P, Nucciotti, A, Pedretti, M, Pobes, C, Palmieri, V, Pavan, M, Pessina, G, Pirro, S, Previtali, E, Rosenfeld, C, Smith, A, Sisti, M, Ventura, G, Vanzini, M, Zanotti, L, For the CUORE, C, ARNABOLDI, CLAUDIO, BROFFERIO, CHIARA, CAPELLI, SILVIA, FIORINI, ETTORE, GIULIANI, ANDREA, GORLA, PAOLO, NUCCIOTTI, ANGELO ENRICO LODOVICO, PAVAN, MAURA, SISTI, MONICA, ZANOTTI, LUIGI ERNESTO, Avignone, FT, Creswick, RJ, Farach, HA, Haller, EE, Irastorza, IJ, McDonald, RJ, Norman, EB, Smith, AR, For the CUORE Collaboration, Arnaboldi, C, Avignone, F, Beemanc, J, Barucci, M, Balata, M, Brofferio, C, Buccie, C, Cebrian, S, Creswick, R, Capelli, S, Carbone, L, Cremonesi, O, de Ward, A, Fiorini, E, Farach, H, Frossati, G, Giuliani, A, Giugni, D, Gorla, P, Haller, E, Irastorza, I, Mcdonald, R, Morales, A, Norman, E, Negri, P, Nucciotti, A, Pedretti, M, Pobes, C, Palmieri, V, Pavan, M, Pessina, G, Pirro, S, Previtali, E, Rosenfeld, C, Smith, A, Sisti, M, Ventura, G, Vanzini, M, Zanotti, L, For the CUORE, C, ARNABOLDI, CLAUDIO, BROFFERIO, CHIARA, CAPELLI, SILVIA, FIORINI, ETTORE, GIULIANI, ANDREA, GORLA, PAOLO, NUCCIOTTI, ANGELO ENRICO LODOVICO, PAVAN, MAURA, SISTI, MONICA, ZANOTTI, LUIGI ERNESTO, Avignone, FT, Creswick, RJ, Farach, HA, Haller, EE, Irastorza, IJ, McDonald, RJ, Norman, EB, Smith, AR, and For the CUORE Collaboration
- Abstract
CUORE is a proposed tightly packed array of 1000 TeO2 bolometers, each being a cube 5 cm on a side with a mass of 760 g. The array consists of 25 vertical towers, arranged in a square of 5 towers×5 towers, each containing 10 layers of four crystals. The design of the detector is optimized for ultralow-background searches: for neutrinoless double-beta decay of 130Te (33.8% abundance), cold dark matter, solar axions, and rare nuclear decays. A preliminary experiment involving 20 crystals 3×3×6 cm3 of 340 g has been completed, and a single CUORE tower is being constructed as a smaller-scale experiment called CUORICINO. The expected performance and sensitivity, based on Monte Carlo simulations and extrapolations of present results, are reported. © 2003 Elsevier B.V. All rights reserved.
- Published
- 2004