Journal
EUROPEAN PHYSICAL JOURNAL C
Volume 81, Issue 2, Pages -Publisher
SPRINGER
DOI: 10.1140/epjc/s10052-020-08809-8
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Funding
- Istituto Nazionale di Fisica Nucleare (INFN)
- European Research Council (ERC) under the European Union [H2020/2014-2020]
- ERC [742345 (ERC-2016-ADG), 754496]
- Italian Ministry of University and Research (MIUR) through the grant Progetti di ricerca di Rilevante Interesse Nazionale (PRIN) [2017FJZMCJ]
- US National Science Foundation [NSF-PHY-1401832, NSF-PHY-1614611, NSF-PHY-1913374]
- US Department of Energy (DOE) Office of Science [DE-AC02-05CH11231, DE-AC02-06CH11357]
- DOE Office of Science, Office of Nuclear Physics [DE-FG02-08ER41551, DE-SC0011091, DE-SC0012654, DE-SC0019316, DE-SC0019368, DE-SC0020423]
- Russian Science Foundation [18-12-00003]
- National Research Foundation of Ukraine [2020.02/0011]
- U.S. Department of Energy (DOE) [DE-SC0020423, DE-SC0019368, DE-SC0019316] Funding Source: U.S. Department of Energy (DOE)
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The CUPID Collaboration is developing a background-free detector for double beta decay, with enriched Li2100MoO4 crystals showing potential. Characterization of cubic crystals was conducted, demonstrating energy resolution close to target values. The study validated a Monte Carlo simulation for optimizing detector efficiency.
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 alpha 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 alpha -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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