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  • C. Augier; A. S. Barabash; F. Bellini; G. Benato; M. Beretta; L. Bergé; J. Billard; Yu. A. Borovlev; L. Cardani; N. Casali; A. Cazes; E. Celi; M. Chapellier; D. Chiesa; I. Dafinei; F. A. Danevich; M. De Jesus; P. de Marcillac; T. Dixon; L. Dumoulin; K. Eitel; F. Ferri; B. K. Fujikawa; J. Gascon; L. Gironi; A. Giuliani; V. D. Grigorieva; M. Gros; D. L. Helis; H. Z. Huang; R. Huang; L. Imbert; J. Johnston; A. Juillard; H. Khalife; M. Kleifges; V. V. Kobychev; Yu. G. Kolomensky; S. I. Konovalov; J. Kotila; P. Loaiza; L. Ma; E. P. Makarov; R. Mariam; L. Marini; S. Marnieros; X.-F. Navick; C. Nones; E. B. Norman; E. Olivieri; J. L. Ouellet; L. Pagnanini; L. Pattavina; B. Paul; M. Pavan; H. Peng; G. Pessina; S. Pirro; D. V. Poda; O. G. Polischuk; S. Pozzi; E. Previtali; Th. Redon; A. Rojas; S. Rozov; V. Sanglard; J. A. Scarpaci; B. Schmidt; Y. Shen; V. N. Shlegel; V. Singh; C. Tomei; V. I. Tretyak; V. I. Umatov; L. Vagneron; M. Velázquez; B. Welliver; L. Winslow; M. Xue; E. Yakushev; M. Zarytskyy; A. S. Zolotarova

    The European physical journal. C, Particles and fields, 07/2023, Letnik: 83, Številka: 7
    Journal Article

    Abstract CUPID-Mo, located in the Laboratoire Souterrain de Modane (France), was a demonstrator for the next generation $$0\nu \beta \beta $$ 0 ν β β decay experiment, CUPID. It consisted of an array of 20 enriched Li $$_{2}$$ 2 $$^{100}$$ 100 MoO $$_4$$ 4 bolometers and 20 Ge light detectors and has demonstrated that the technology of scintillating bolometers with particle identification capabilities is mature. Furthermore, CUPID-Mo can inform and validate the background prediction for CUPID. In this paper, we present a detailed model of the CUPID-Mo backgrounds. This model is able to describe well the features of the experimental data and enables studies of the $$2\nu \beta \beta $$ 2 ν β β decay and other processes with high precision. We also measure the radio-purity of the Li $$_{2}$$ 2 $$^{100}$$ 100 MoO $$_4$$ 4 crystals which are found to be sufficient for the CUPID goals. Finally, we also obtain a background index in the region of interest of 3.7  $$^{+0.9}_{-0.8}$$ - 0.8 + 0.9  (stat) $$^{+1.5}_{-0.7}$$ - 0.7 + 1.5  (syst)  $$\times ~10 ^{-3}$$ × 10 - 3  counts/ $$\Delta E_{\text {FWHM}}/\text {mol}_{\text {iso}}/\text {year},$$ Δ E FWHM / mol iso / year , the lowest in a bolometric $$0\nu \beta \beta $$ 0 ν β β decay experiment.