- Main
Sensitivity of the CUPID experiment to 0νββ decay of 100Mo
- Alfonso, K;
- Armatol, A;
- Augier, C;
- Avignone, FT;
- Azzolini, O;
- Barabash, AS;
- Bari, G;
- Barresi, A;
- Baudin, D;
- Bellini, F;
- Benato, G;
- Benussi, L;
- Berest, V;
- Beretta, M;
- Bergé, L;
- Bettelli, M;
- Biassoni, M;
- Billard, J;
- Boffelli, F;
- Boldrini, V;
- Brandani, ED;
- Brofferio, C;
- Bucci, C;
- Buchynska, M;
- Camilleri, J;
- Campani, A;
- Cao, J;
- Capelli, C;
- Capelli, S;
- Caracciolo, V;
- Cardani, L;
- Carniti, P;
- Casali, N;
- Celi, E;
- Chang, C;
- Chapellier, M;
- Chen, H;
- Chiesa, D;
- Cintas, D;
- Clemenza, M;
- Colantoni, I;
- Copello, S;
- Cremonesi, O;
- Creswick, RJ;
- D’Addabbo, A;
- Dafinei, I;
- Danevich, FA;
- De Dominicis, F;
- De Jesus, M;
- de Marcillac, P;
- Dell’Oro, S;
- Di Domizio, S;
- Di Lorenzo, S;
- Dixon, T;
- Drobizhev, A;
- Dumoulin, L;
- Idrissi, M El;
- Faverzani, M;
- Ferri, E;
- Ferri, F;
- Ferroni, F;
- Figueroa-Feliciano, E;
- Formaggio, J;
- Franceschi, A;
- Fu, S;
- Fujikawa, BK;
- Gascon, J;
- Ghislandi, S;
- Giachero, A;
- Girola, M;
- Gironi, L;
- Giuliani, A;
- Gorla, P;
- Gotti, C;
- Grant, C;
- Gras, P;
- Guillaumon, PV;
- Gutierrez, TD;
- Han, K;
- Hansen, EV;
- Heeger, KM;
- Helis, DL;
- Huang, HZ;
- Hurst, MT;
- Imbert, L;
- Johnson, T;
- Juillard, A;
- Karapetrov, G;
- Keppel, G;
- Khalife, H;
- Kobychev, VV;
- Kolomensky, Yu G;
- Kowalski, R;
- Lattaud, H;
- Lefevre, M;
- Lisovenko, M;
- Liu, R;
- Liu, Y;
- Loaiza, P;
- Ma, L;
- Mancarella, F;
- Manenti, N;
- Mariani, A;
- Marini, L;
- Marnieros, S;
- Martinez, M;
- Maruyama, RH;
- Mas, Ph;
- Mayer, D;
- Mazzitelli, G;
- Mazzola, E;
- Mei, Y;
- Moore, MN;
- Morganti, S;
- Napolitano, T;
- Nastasi, M;
- Nikkel, J;
- Nones, C;
- Norman, EB;
- Novosad, V;
- Nutini, I;
- O’Donnell, T;
- Olivieri, E;
- Olmi, M;
- Oregui, BT;
- Pagan, S;
- Pageot, M;
- Pagnanini, L;
- Pasciuto, D;
- Pattavina, L;
- Pavan, M;
- Penek, Ö;
- Peng, H;
- Pessina, G;
- Pettinacci, V;
- Pira, C;
- Pirro, S;
- Pochon, O;
- Poda, DV;
- Polakovic, T;
- Polischuk, OG;
- Pottebaum, EG;
- Pozzi, S;
- Previtali, E;
- Puiu, A;
- Puranam, S;
- Quitadamo, S;
- Rappoldi, A;
- Raselli, GL;
- Ressa, A;
- Rizzoli, R;
- Rosenfeld, C;
- Rosier, P;
- Rossella, M;
- Scarpaci, JA;
- Schmidt, B;
- Serino, R;
- Shaikina, A;
- Shang, K;
- Sharma, V;
- Shlegel, VN;
- Singh, V;
- Sisti, M;
- Slocum, P;
- Speller, D;
- Surukuchi, PT;
- Taffarello, L;
- Tomassini, S;
- Tomei, C;
- Torres, A;
- Torres, JA;
- Tozzi, D;
- Tretyak, VI;
- Trotta, D;
- Velazquez, M;
- Vetter, KJ;
- Wagaarachchi, SL;
- Wang, G;
- Wang, L;
- Wang, R;
- Welliver, B;
- Wilson, J;
- Wilson, K;
- Winslow, LA;
- Xie, F;
- Xue, M;
- Yang, J;
- Yefremenko, V;
- Umatov, VI;
- Zarytskyy, MM;
- Zhu, T;
- Zolotarova, A;
- Zucchelli, S
Published Web Location
https://doi.org/10.1140/epjc/s10052-026-15296-wAbstract
CUPID is a next-generation bolometric experiment to search for neutrinoless double-beta decay (0νββ$$0 u \beta \beta $$) of 100Mo using Li2$$_2$$MoO4$$_4$$ scintillating crystals. It will operate 1596 crystals at ∼$$\sim $$10 mK in the CUORE cryostat at the Laboratori Nazionali del Gran Sasso in Italy. Each crystal will be facing two Ge-based bolometric light detectors for α$$\alpha $$ rejection. We compute the discovery and the exclusion sensitivity of CUPID to 0νββ$$0 u \beta \beta $$ in a Frequentist and a Bayesian framework. This computation is done numerically based on pseudo-experiments. For the CUPID baseline scenario, with a background and an energy resolution of 1.0×10-4$$1.0 \times 10^{-4}$$ counts/keV/kg/yr and 5 keV FWHM at the Q-value, respectively, this results in a Bayesian exclusion sensitivity (90% c.i.) of T^1/2>1.6×1027yr$$\hat{T}_{1/2} > 1.6 \times 10^{27} \ \textrm{yr}$$, corresponding to the effective Majorana neutrino mass of m^ββ<9.6$$\hat{m}_{\beta \beta } < \ 9.6$$–28meV$$28 \ \textrm{meV}$$. The Frequentist discovery sensitivity (3σ$$\sigma $$) is T^1/2=1.0×1027yr$$\hat{T}_{1/2}= 1.0 \times 10^{27} \ \textrm{yr}$$, corresponding to m^ββ=12$$\hat{m}_{\beta \beta }= \ 12$$ – 36meV$$36 \ \textrm{meV}$$.
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