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) 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 experiment, and for follow-up studies on detector response and on delayed products induced by cosmic-ray muons.
Zucchelli, S., Zimmermann, S., Zhu, T., Xie, F., Winslow, L., Wilson, K., et al. (2026). Reconstruction of cosmic-ray muon events with CUORE. THE EUROPEAN PHYSICAL JOURNAL. C, PARTICLES AND FIELDS, 86(7) [10.1140/epjc/s10052-026-15737-6].
Reconstruction of cosmic-ray muon events with CUORE
Sisti M.;Quitadamo S.;Previtali E.;Pavan M.;Pattavina L.;Nucciotti A.;Nastasi M.;Gotti C.;Gironi L.;Giachero A.;Faverzani M.;Chiesa D.;Capelli S.;Brofferio C.;Branca A.;
2026
Abstract
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) 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 experiment, and for follow-up studies on detector response and on delayed products induced by cosmic-ray muons.| File | Dimensione | Formato | |
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