- Main
Reconstruction of cosmic-ray muon events with CUORE
- Adams, DQ;
- Alduino, C;
- Alfonso, K;
- Armatol, A;
- Avignone, FT;
- Azzolini, O;
- Bari, G;
- Bellini, F;
- Benato, G;
- Beretta, M;
- Biassoni, M;
- Branca, A;
- Brandani, ED;
- Brofferio, C;
- Bucci, C;
- Camilleri, J;
- Caminata, A;
- Campani, A;
- Cao, J;
- Capelli, S;
- Cappelli, L;
- Cardani, L;
- Carniti, P;
- Casali, N;
- Chiesa, D;
- Chu, Y;
- Clemenza, M;
- Copello, S;
- Cremonesi, O;
- Creswick, RJ;
- D’Addabbo, A;
- Dafinei, I;
- Dell’Oro, S;
- Di Domizio, S;
- Di Lorenzo, S;
- Fang, DQ;
- Faverzani, M;
- Ferri, E;
- Ferroni, F;
- Fiorini, E;
- Franceschi, MA;
- Freedman, SJ;
- Fu, SH;
- Fujikawa, BK;
- Ghislandi, S;
- Giachero, A;
- Girola, M;
- Gironi, L;
- Giuliani, A;
- Gorla, P;
- Gotti, C;
- Guillaumon, PV;
- Gutierrez, TD;
- Han, K;
- Hansen, EV;
- Heeger, KM;
- Helis, DL;
- Huang, HZ;
- Hurst, MT;
- Keppel, G;
- Kolomensky, Yu G;
- Kowalski, R;
- Liu, R;
- Ma, L;
- G., Y;
- Marini, L;
- Maruyama, RH;
- Mayer, D;
- Moore, MN;
- Napolitano, T;
- Nastasi, M;
- Nones, C;
- Norman, EB;
- Nucciotti, A;
- Nutini, I;
- O’Donnell, T;
- Olmi, M;
- Pagan, S;
- Pagliarone, CE;
- Pagnanini, L;
- Pallavicini, M;
- Pattavina, L;
- Pavan, M;
- Pessina, G;
- Pettinacci, V;
- Pira, C;
- Pirro, S;
- Pottebaum, EG;
- Pozzi, S;
- Previtali, E;
- Puiu, A;
- Quitadamo, S;
- Ressa, A;
- Rosenfeld, C;
- Schmidt, B;
- Serino, R;
- Shaikina, A;
- Sharma, V;
- Singh, V;
- Sisti, M;
- Speller, D;
- Surukuchi, PT;
- Taffarello, L;
- Tomei, C;
- Torres, A;
- Torres, JA;
- Vetter, KJ;
- Vignati, M;
- Wagaarachchi, SL;
- Wang, R;
- Welliver, B;
- Wilson, J;
- Wilson, K;
- Winslow, LA;
- Xie, F;
- Zhu, T;
- Zimmermann, S;
- Zucchelli, S
Published Web Location
https://doi.org/10.1140/epjc/s10052-026-15737-6Abstract
We report the in-situ 3D reconstruction of through-going muons in the CUORE experiment, a cryogenic calorimeter array searching for neutrinoless double beta (0νββ$$0 u \beta \beta $$) decay, leveraging the segmentation of the detector. Due to the slow time response of the detector, time-of-flight estimation is not feasible. Therefore, the track reconstruction is performed using a multi-objective optimization algorithm that relies on geometrical information from the detector as a whole. We measure the integral flux of cosmic-ray muons underground at the Laboratori Nazionali del Gran Sasso, and find our value to be in good agreement with other experiments that have performed a similar measurement. To our knowledge, this work represents the first demonstration of 3D particle tracking and reconstruction of through-going muons with per-event angular determination in a millikelvin cryogenic detector array. The analysis performed for this work will be critical for validating the muon-related background in CUPID, a next-generation 0νββ$$0 u \beta \beta $$ experiment, and for follow-up studies on detector response and on delayed products induced by cosmic-ray muons.
Many UC-authored scholarly publications are freely available on this site because of the UC's open access policies. Let us know how this access is important for you.