1. The CUORE Detector and Results
- Author
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James R. Wilson, C. Rosenfeld, S. Morganti, N. D. Scielzo, Carlo Ligi, V. Dompè, A. D'Addabbo, A. Campani, P. Gorla, F. Ferroni, C. Tomei, Monica Sisti, S. Copello, S. L. Wagaarachchi, J. Nikkel, L. Zanotti, Paolo Carniti, C. Pira, M. Faverzani, N. Casali, N. Chott, Simone Capelli, C. J. Davis, Giovanni Benato, H. Z. Huang, G. Keppel, L. Gironi, Ettore Fiorini, F. Terranova, G. Fantini, C. Nones, A. Puiu, S. Zucchelli, V. Novati, Andrea Giachero, Massimiliano Clemenza, Carlo Cosmelli, F. T. Avignone, Irene Nutini, Yu. G. Kolomensky, Massimiliano Nastasi, L. Canonica, L. Marini, V. Pettinacci, K. Wilson, Eric B. Norman, T. O'Donnell, D. Q. Adams, Vasundhara Singh, Jonathan Ouellet, K. Alfonso, S. Di Domizio, J. Johnston, Claudio Gotti, G. Bari, Y. Mei, D. D'Aguanno, T. Napolitano, Evelyn Ferri, Laura Cardani, L. Taffarello, Stefano Dell'Oro, B. K. Fujikawa, Stefano Pozzi, F. Bellini, B. Schmidt, Y. G. Ma, Oliviero Cremonesi, M. Biassoni, Danielle Speller, B. S. Wang, Xi-Guang Cao, C. Brofferio, M. Vignati, M. Pavan, L. Pagnanini, K. M. Heeger, Davide Chiesa, O. Azzolini, N. Moggi, Marco Pallavicini, C. Rusconi, C. Bucci, T. D. Gutierrez, R. J. Creswick, Samuele Sangiorgio, Lindley Winslow, A. Giuliani, Ke Han, Reina H. Maruyama, I. Dafinei, M. Sakai, G. Pessina, Stuart J. Freedman, L. Pattavina, A. Nucciotti, C. Alduino, S. Zimmermann, S. Pirro, L. Ma, D. Q. Fang, A. Branca, M. A. Franceschi, R. G. Huang, L. Cappelli, C. Pagliarone, A. Caminata, Ezio Previtali, B. Welliver, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Nutini, I, Adams, D, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D’Addabbo, A, D’Aguanno, D, Dafinei, I, Davis, C, Dell’Oro, S, Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, Y, Ma, L, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, O’Donnell, T, Ouellet, J, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, Nutini I., Adams D.Q., Alduino C., Alfonso K., Avignone F.T., Azzolini O., Bari G., Bellini F., Benato G., Biassoni M., Branca A., Brofferio C., Bucci C., Caminata A., Campani A., Canonica L., Cao X.G., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Chiesa D., Chott N., Clemenza M., Copello S., Cosmelli C., Cremonesi O., Creswick R.J., D'Addabbo A., D'Aguanno D., Dafinei I., Davis C.J., Dell'Oro S., Domizio S.D., Dompe V., Fang D.Q., Fantini G., Faverzani M., Ferri E., Ferroni F., Fiorini E., Franceschi M.A., Freedman S.J., Fujikawa B.K., Giachero A., Gironi L., Giuliani A., Gorla P., Gotti C., Gutierrez T.D., Han K., Heeger K.M., Huang R.G., Huang H.Z., Johnston J., Keppel G., Kolomensky Y.G., Ligi C., Ma Y.G., Ma L., Marini L., Maruyama R.H., Mei Y., Moggi N., Morganti S., Napolitano T., Nastasi M., Nikkel J., Nones C., Norman E.B., Novati V., Nucciotti A., O'Donnell T., Ouellet J.L., Pagliarone C.E., Pagnanini L., Pallavicini M., Pattavina L., Pavan M., Pessina G., Pettinacci V., Pira C., Pirro S., Pozzi S., Previtali E., Puiu A., Rosenfeld C., Rusconi C., Sakai M., Sangiorgio S., Schmidt B., Scielzo N.D., Singh V., Sisti M., Speller D., Taffarello L., Terranova F., Tomei C., Vignati M., Wagaarachchi S.L., Wang B.S., Welliver B., Wilson J., Wilson K., Winslow L.A., Zanotti L., Zimmermann S., Zucchelli S., and Département de Physique des Particules (ex SPP) (DPhP)
- Subjects
Particle physics ,0 νββ ,Cryogenics ,CUORE ,Macro-calorimeters ,Neutrinos ,Physics::Instrumentation and Detectors ,Cryogenic ,01 natural sciences ,tellurium: oxygen ,010305 fluids & plasmas ,crystal ,double-beta decay: (0neutrino) ,Double beta decay ,0103 physical sciences ,Neutrino ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,General Materials Science ,Beta (velocity) ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,010306 general physics ,activity report ,detector: design ,Physics ,0νββ ,0 nu beta beta ,Detector ,Astrophysics::Instrumentation and Methods for Astrophysics ,Condensed Matter Physics ,Atomic and Molecular Physics, and Optics ,High Energy Physics::Experiment ,tellurium: nuclide ,Macro-calorimeter ,experimental results - Abstract
The cryogenic underground observatory for rare events (CUORE) is a cryogenic experiment searching for neutrinoless double beta decay ($$0\nu \beta \beta$$0νββ) of $${^{130}\hbox {Te}}$$130Te. The detector consists of an array of $$988\,{\hbox {TeO}_{2}}$$988TeO2 crystals arranged in a compact cylindrical structure of 19 towers. We report the CUORE initial operations and optimization campaigns. We then present the CUORE results on $$0\nu \beta \beta$$0νββ and $$2\nu \beta \beta$$2νββ decay of $${^{130}\hbox {Te}}$$130Te obtained from the analysis of the physics data acquired in 2017.
- Published
- 2019