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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; 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; 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, 11/2022, Letnik: 82, Številka: 11
    Journal Article

    Abstract The CUPID-Mo experiment to search for 0 $$\nu \beta \beta $$ ν β β decay in $$^{100}$$ 100 Mo has been recently completed after about 1.5 years of operation at Laboratoire Souterrain de Modane (France). It served as a demonstrator for CUPID, a next generation 0 $$\nu \beta \beta $$ ν β β decay experiment. CUPID-Mo was comprised of 20 enriched $$\hbox {Li}_{{2}}$$ Li 2 $$^{100}$$ 100 $$\hbox {MoO}_4$$ MoO 4 scintillating calorimeters, each with a mass of $$\sim 0.2$$ ∼ 0.2  kg, operated at $$\sim 20$$ ∼ 20  mK. We present here the final analysis with the full exposure of CUPID-Mo ( $$^{100}$$ 100 Mo exposure of 1.47 $$\hbox {kg} \times \hbox {year}$$ kg × year ) used to search for lepton number violation via 0 $$\nu \beta \beta $$ ν β β decay. We report on various analysis improvements since the previous result on a subset of data, reprocessing all data with these new techniques. We observe zero events in the region of interest and set a new limit on the $$^{100}$$ 100 Mo 0 $$\nu \beta \beta $$ ν β β decay half-life of $$T_{1/2}^{0\nu }$$ T 1 / 2 0 ν $$> {1.8}\times 10^{24}$$ > 1.8 × 10 24  year (stat. + syst.) at 90% CI. Under the light Majorana neutrino exchange mechanism this corresponds to an effective Majorana neutrino mass of $$\left<m_{\beta \beta }\right>$$ m β β   $$<~{(0.28{-}0.49)} $$ < ( 0.28 - 0.49 )  eV, dependent upon the nuclear matrix element utilized.