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CUPID-0: the first array of enriched scintillating bolometers for 0νββ decay investigations

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arxiv 1802.06562 v3 pith:K3IYUNRQ submitted 2018-02-19 physics.ins-det

CUPID-0: the first array of enriched scintillating bolometers for 0νββ decay investigations

O. Azzolini , M.T. Barrera , J. W. Beeman , F. Bellini , M. Beretta , M. Biassoni , C. Brofferio , C. Bucci
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L. Canonica S. Capelli L. Cardani P. Carniti N. Casali L. Cassina M. Clemenza O. Cremonesi A. Cruciani A. D'Addabbo I. Dafinei S. Di Domizio F. Ferroni L. Gironi A. Giuliani P. Gorla C. Gotti G. Keppel M. Martinez S. Morganti S. Nagorny M. Nastasi S. Nisi C. Nones D. Orlandi L. Pagnanini M. Pallavicini V. Palmieri L. Pattavina M. Pavan G. Pessina V. Pettinacci S. Pirro S. Pozzi E. Previtali A. Puiu F. Reindl C. Rusconi K. Schaeffner C. Tomei M. Vignati A. Zolotarova
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classification physics.ins-det
keywords betadetectorconstructioncupid-0arraybackgroundcryogenicdecay
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The CUPID-0 detector hosted at the Laboratori Nazionali del Gran Sasso, Italy, is the first large array of enriched scintillating cryogenic detectors for the investigation of $^{82}$Se neutrinoless double-beta decay (0$\nu\beta\beta$). CUPID-0 aims at measuring a background index in the region of interest (RoI) for 0$\nu\beta\beta$ at the level of 10$^{-3}$ c/keV/kg/y, the lowest value ever measured using cryogenic detectors. This result can be achieved by a state of the art technology for background suppression and thorough protocols and procedures for detector preparation and construction. In this paper, the different phases of the detector design and construction will be presented, from the material selection (for the absorber production) to the new and innovative detector structure. The successful construction of the detector lead to promising detector performance which are here preliminarily discussed

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Cited by 2 Pith papers

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  1. Probing large mass-splitting inelastic Dark Matter with RES-NOVA

    astro-ph.CO 2026-07 conditional novelty 6.0

    A 32.4 g·d PbWO4 cryogenic detector reports the first direct limits on inelastic dark matter at mass splittings up to ~510 keV (SHM) and ~780 keV (LMC).

  2. CUPID pre-CDR

    physics.ins-det 2019-07 unverdicted novelty 4.0

    CUPID proposes a large bolometric detector array with alpha/beta discrimination to achieve a background-free search for 0νββ decay in 100Mo and probe the inverted neutrino mass hierarchy.