TY - JOUR
T1 - Characterization of cubic Li 2100 MoO 4 crystals for the CUPID experiment
AU - The CUPID Collaboration
AU - Armatol, A.
AU - Armengaud, E.
AU - Armstrong, W.
AU - Augier, C.
AU - Avignone, F. T.
AU - Azzolini, O.
AU - Barabash, A.
AU - Bari, G.
AU - Barresi, A.
AU - Baudin, D.
AU - Bellini, F.
AU - Benato, G.
AU - Beretta, M.
AU - Bergé, L.
AU - Biassoni, M.
AU - Billard, J.
AU - Boldrini, V.
AU - Branca, A.
AU - Brofferio, C.
AU - Bucci, C.
AU - Camilleri, J.
AU - Capelli, S.
AU - Cappelli, L.
AU - Cardani, L.
AU - Carniti, P.
AU - Casali, N.
AU - Cazes, A.
AU - Celi, E.
AU - Chang, C.
AU - Chapellier, M.
AU - Charrier, A.
AU - Chiesa, D.
AU - Clemenza, M.
AU - Colantoni, I.
AU - Collamati, F.
AU - Copello, S.
AU - Cremonesi, O.
AU - J. Creswick, R.
AU - Cruciani, A.
AU - D’Addabbo, A.
AU - D’Imperio, G.
AU - Dafinei, I.
AU - A. Danevich, F.
AU - de Combarieu, M.
AU - De Jesus, M.
AU - de Marcillac, P.
AU - Dell’Oro, S.
AU - Di Domizio, S.
AU - Dompè, V.
AU - Figueroa-Feliciano, E.
N1 - Funding Information:
The CUPID Collaboration thanks the directors and staff of the Laboratori Nazionali del Gran Sasso and the technical staff of our laboratories. This work was supported by the Istituto Nazionale di Fisica Nucleare (INFN); by the European Research Council (ERC) under the European Union Horizon 2020 program (H2020/2014-2020) with the ERC Advanced Grant No. 742345 (ERC-2016-ADG, project CROSS) and the Marie Sklodowska-Curie Grant Agreement No. 754496; by the Italian Ministry of University and Research (MIUR) through the grant Progetti di ricerca di Rilevante Interesse Nazionale (PRIN 2017, Grant No. 2017FJZMCJ); by the US National Science Foundation under Grant Nos. NSF-PHY-1401832, NSF-PHY-1614611, and NSF-PHY-1913374. This material is also based upon work supported by the US Department of Energy (DOE) Office of Science under Contract Nos. DE-AC02-05CH11231 and DE-AC02-06CH11357; and by the DOE Office of Science, Office of Nuclear Physics under Contract Nos. DE-FG02-08ER41551, DE-SC0011091, DE-SC0012654, DE-SC0019316, DE-SC0019368, and DE-SC0020423. This work was also supported by the Russian Science Foundation under Grant No. 18-12-00003 and the National Research Foundation of Ukraine under Grant No. 2020.02/0011. This research used resources of the National Energy Research Scientific Computing Center (NERSC). This work makes use of both the DIANA data analysis and APOLLO data acquisition software packages, which were developed by the CUORICINO, CUORE, LUCIFER and CUPID-0 Collaborations.
Publisher Copyright:
© 2021, The Author(s).
PY - 2021/2
Y1 - 2021/2
N2 - The CUPID Collaboration is designing a tonne-scale, background-free detector to search for double beta decay with sufficient sensitivity to fully explore the parameter space corresponding to the inverted neutrino mass hierarchy scenario. One of the CUPID demonstrators, CUPID-Mo, has proved the potential of enriched Li2100MoO4 crystals as suitable detectors for neutrinoless double beta decay search. In this work, we characterised cubic crystals that, compared to the cylindrical crystals used by CUPID-Mo, are more appealing for the construction of tightly packed arrays. We measured an average energy resolution of (6.7 ± 0.6) keV FWHM in the region of interest, approaching the CUPID target of 5 keV FWHM. We assessed the identification of α particles with and without a reflecting foil that enhances the scintillation light collection efficiency, proving that the baseline design of CUPID already ensures a complete suppression of this α-induced background contribution. We also used the collected data to validate a Monte Carlo simulation modelling the light collection efficiency, which will enable further optimisations of the detector.
AB - The CUPID Collaboration is designing a tonne-scale, background-free detector to search for double beta decay with sufficient sensitivity to fully explore the parameter space corresponding to the inverted neutrino mass hierarchy scenario. One of the CUPID demonstrators, CUPID-Mo, has proved the potential of enriched Li2100MoO4 crystals as suitable detectors for neutrinoless double beta decay search. In this work, we characterised cubic crystals that, compared to the cylindrical crystals used by CUPID-Mo, are more appealing for the construction of tightly packed arrays. We measured an average energy resolution of (6.7 ± 0.6) keV FWHM in the region of interest, approaching the CUPID target of 5 keV FWHM. We assessed the identification of α particles with and without a reflecting foil that enhances the scintillation light collection efficiency, proving that the baseline design of CUPID already ensures a complete suppression of this α-induced background contribution. We also used the collected data to validate a Monte Carlo simulation modelling the light collection efficiency, which will enable further optimisations of the detector.
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U2 - 10.1140/epjc/s10052-020-08809-8
DO - 10.1140/epjc/s10052-020-08809-8
M3 - Article
AN - SCOPUS:85100264580
SN - 1434-6044
VL - 81
JO - European Physical Journal C
JF - European Physical Journal C
IS - 2
M1 - 104
ER -