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Recent progresses on BSM and Dark Matter searches with CUORE

by CUORE Collaboration: D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, G. Benuzzi, M. Beretta, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, L. Canonica, X. G. Cao, S. Capelli, C. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, E. Celi, D. Chiesa, M. Clemenza, S. Copello, O. Cremonesi, R. J. Creswick, A. D'Addabbo, I. Dafinei, F. Del Corso, S. Dell'Oro, S. Di Domizio, S. Di Lorenzo, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, S.H. Fu, B. K. Fujikawa, S. Ghislandi, A. Giachero, A. Gianvecchio, M. Girola, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, P.V. Guillaumon, T. D. Gutierrez, K. Han, E. V. Hansen, K. M. Heeger, R. G. Huang, H. Z. Huang, G. Keppel, Yu. G. Kolomensky, R. Kowalski, R. Liu, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, D. Mayer, Y. Mei, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, A. Nucciotti, I. Nutini, T. O'Donnell, M. Olmi, J. L. Ouellet, S. Pagan, C. E. Pagliarone, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, I. Ponce, S. Pozzi, E. Previtali, A. Puiu, S. Quitadamo, A. Ressa, C. Rosenfeld, B. Schmidt, V. Sharma, V. Singh, M. Sisti, D. Speller, P.T. Surukuchi, L. Taffarello, F. Terranova, C. Tomei, J.A Torres, K. J. Vetter, M. Vignati, S. L. Wagaarachchi, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, S. Zimmermann, S. Zucchelli

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Submission summary

Authors (as registered SciPost users): Antonio Branca
Submission information
Preprint Link: scipost_202210_00043v1  (pdf)
Date accepted: 2023-04-28
Date submitted: 2022-10-05 11:01
Submitted by: Branca, Antonio
Submitted to: SciPost Physics Proceedings
Proceedings issue: 14th International Conference on Identification of Dark Matter (IDM2022)
Ontological classification
Academic field: Physics
  • Nuclear Physics - Experiment
Approach: Experimental


The Cryogenic Underground Observatory for Rare Events (CUORE) is the first bolometric $0\nu\beta\beta$ experiment to reach the one-tonne mass scale. The detector, located underground at the Laboratori Nazionali del Gran Sasso in Italy, consists of 988 TeO$_2$ crystals arranged in a compact cylindrical structure of 19 towers, operating at a base temperature of about 10~mK. After beginning its first physics data run in 2017, CUORE has since collected the largest amount of data ever acquired with a solid state detector and provided the most sensitive measurement of $0\nu\beta\beta$ decay in $^{130}$Te ever conducted. The large exposure, sharp energy resolution, segmented structure and radio-pure environment make CUORE an ideal instrument for a wide array of searches for rare events and symmetry violations. New searches for low mass dark matter, solar axions, CPT and Lorenz violations, and refined measurements of the $2\nu\beta\beta$ spectrum in CUORE have the potential to provide new insight and constraints on extensions to the standard model complementary to other particle physics searches. In this contribution, the recent progress on BSM and dark matter searches in CUORE are discussed.

Published as SciPost Phys. Proc. 12, 054 (2023)

Reports on this Submission

Anonymous Report 1 on 2022-11-7 (Invited Report)

  • Cite as: Anonymous, Report on arXiv:scipost_202210_00043v1, delivered 2022-11-07, doi: 10.21468/SciPost.Report.6079


The data received in the experiment will be used outside of it is original goal, extending possible physics results.


Missing some visual illustrations.


Author describes very wide range of efforts taken by collaboration to perform searches Beyond Standard Model. A lot of tools developed for this and work is on going. A new approach to reduce the background is presented. As well experiment claims to exclude DAMA positive signal region.

  • validity: -
  • significance: high
  • originality: high
  • clarity: high
  • formatting: excellent
  • grammar: excellent

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