A cryogenic underground observatory for rare events: CUORE, an update |
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Authors: | A Alessandrello C Arnaboldi F T Avignone III J Beeman M Barucci M Balata C Brofferio C Bucci S Cebrian R J Creswick S Capelli L Carbone O Cremonesi A de Ward E Fiorini H A Farach G Frossati A Giuliani D Giugni E E Haller I G Irastorza R J McDonald A Morales E B Norman P Negri A Nucciotti M Pedretti C Pobes V Palmieri M Pavan G Pessina S Pirro E Previtali C Rosenfeld A R Smith M Sisti G Ventura M Vanzini L Zanotti |
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Institution: | (1) Department of Physics and Astronomy, University of South Carolina, Columbia, SC 29208, USA;(2) Lawrence Berkeley National Laboratory, California, USA;(3) Department of Materials Science and Mineral Engineering, University of California, Berkeley, CA 94720, USA;(4) Dipartimento di Fisica dell'Università di Firenze e Sezione di Firenze dell'INFN, Italy;(5) Laboratori Nazionali del Gran Sasso, Assergi (L'Aquila), Italy;(6) Laboratorio de Física Nuclear y Altas Energías, Universidad de Zaragoza, Spain;(7) Kamerling Onnes Laboratory, Leiden University, The Netherlands;(8) Dipartimento di Scienze Chimiche, Fisiche e Matematiche dell'Università dell'Insubria e Sezione di Milano dell'INFN, Como, Italy;(9) Laboratori Nazionali de Legnaro, Padova, Italy;(10) Dipartimento di Fisica dell'Università di Milano-Bicocca e Sezione di Milano dell'INFN, Italy |
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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 750 g. The array consists of 25 vertical towers, arranged in a square of 5 towers by 5 towers, each containing ten 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 of various sizes (MIBETA) 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. |
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