1. Lowering the CUORE energy threshold
- Author
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M. Faverzani, Yu. G. Kolomensky, Luigi Cappelli, Jeremy S. Cushman, Massimiliano Clemenza, Carlo Cosmelli, L. Gladstone, N. Casali, E. V. Hansen, A. Woodcraft, Lorenzo Cassina, Ke Han, A. Branca, Reina H. Maruyama, F. Terranova, Stuart J. Freedman, R. J. Creswick, L. Carbone, C. Pagliarone, Y. Mei, I. Dafinei, T. Wise, N. Moggi, V. Palmieri, C. Brofferio, P. J. Mosteiro, S. L. Wagaarachchi, K. M. Heeger, L. Gironi, Samuele Sangiorgio, A. Drobizhev, C. Rosenfeld, S. Zucchelli, A. Nucciotti, Eric B. Norman, Guimin Zhang, C. Alduino, Stefano Dell'Oro, S. Pirro, Simone Capelli, R. W. Kadel, T. Napolitano, Oliviero Cremonesi, A. Caminata, M. A. Franceschi, S. Zimmermann, P. Gorla, F. Ferroni, Marco Pallavicini, C. Rusconi, Jonathan Ouellet, M. M. Deninno, H. Z. Huang, C. Pira, M. Tenconi, C. Tomei, F. Orio, A. Giuliani, G. Pessina, Emanuele Ferri, Eugene E. Haller, T. I. Banks, M. Biassoni, G. Bari, X. Liu, L. Pattavina, S. Morganti, Avignone, F. T., Iii., B. S. Wang, S. Trentalange, G. Piperno, A. Camacho, S. Di Domizio, F. Bellini, O. Azzolini, Ettore Fiorini, B. K. Fujikawa, C. Nones, Stefano Pozzi, C. Bucci, T. D. Gutierrez, M. Pavan, M. Maino, Miriam Lucio Martinez, V. Pettinacci, R. Hennings-Yeomans, H. W. Wang, A. D'Addabbo, M. Vignati, T. O'Donnell, L. Cardani, Carlo Ligi, A. Giachero, A. R. Smith, X. G. Cao, James R. Wilson, L. Taffarello, K. Alfonso, G. Fernandes, G. Keppel, D. R. Artusa, Virendra Singh, M. L. Di Vacri, B. X. Zhu, Monica Sisti, D. Q. Fang, N. Chott, C. J. Davis, Yu-Gang Ma, S. Copello, Paolo Carniti, Lindley Winslow, Claudio Gotti, Davide Chiesa, K. E. Lim, Jeffrey W. Beeman, A. Bersani, L. Zanotti, A. Leder, D. Santone, N. D. Scielzo, E. Previtali, L. Canonica, L. Marini, Kevin Hickerson, Copello, S, Alduino, C, Alfonso, K, Artusa, D, Avignone, F, Azzolini, O, Banks, T, Bari, G, Beeman, J, Bellini, F, Bersani, A, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Camacho, A, Caminata, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Carbone, L, Cardani, L, Carniti, P, Casali, N, Cassina, L, Chiesa, D, Chott, N, Clemenza, M, Cosmelli, C, Cremonesi, O, Creswick, R, Cushman, J, D'Addabbo, A, Dafinei, I, Davis, C, Dell'Oro, S, Deninno, M, Di Domizio, S, Di Vacri, M, Drobizhev, A, Fang, D, Faverzani, M, Fernandes, G, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gladstone, L, Gorla, P, Gotti, C, Gutierrez, T, Haller, E, Han, K, Hansen, E, Heeger, K, Hennings-Yeomans, R, Hickerson, K, Huang, H, Kadel, R, Keppel, G, Kolomensky, Y, Leder, A, Ligi, C, Lim, K, Liu, X, Ma, Y, Maino, M, Marini, L, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Mosteiro, P, Napolitano, T, Nones, C, Norman, E, Nucciotti, A, O'Donnell, T, Orio, F, Ouellet, J, Pagliarone, C, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Piperno, G, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Rosenfeld, C, Rusconi, C, Sangiorgio, S, Santone, D, Scielzo, N, Singh, V, Sisti, M, Smith, A, Taffarello, L, Tenconi, M, Terranova, F, Tomei, C, Trentalange, S, Vignati, M, Wagaarachchi, S, Wang, B, Wang, H, Wilson, J, Winslow, L, Wise, T, Woodcraft, A, Zanotti, L, Zhang, G, Zhu, B, Zimmermann, S, Zucchelli, S, 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, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Département de Physique des Particules (ex SPP) (DPhP), Copello, S., Alduino, C., Alfonso, K., Artusa, D. R., Avignone, F. T., Azzolini, O., Banks, T. I., Bari, G., Beeman, J. W., Bellini, F., Bersani, A., Biassoni, M., Branca, A., Brofferio, C., Bucci, C., A., Camacho, Caminata, A., Canonica, L., Cao, X. G., Capelli, S., Cappelli, L., Carbone, L., Cardani, L., Carniti, P., Casali, N., Cassina, L., Chiesa, D., Chott, N., Clemenza, M., Cosmelli, C., Cremonesi, O., Creswick, R. J., Cushman, J. S., D'Addabbo, A., Dafinei, I., Davis, C. J., Dell'Oro, S., Deninno, M. M., Di Domizio, S., Di Vacri, M. L., Drobizhev, A., Fang, D. Q., Faverzani, M., G., Fernande, Ferri, E., Ferroni, F., Fiorini, E., Franceschi, M. A., Freedman, S. J., Fujikawa, B. K., Giachero, A., Gironi, L., Giuliani, A., Gladstone, L., Gorla, P., Gotti, C., Gutierrez, T. D., Haller, E. E., Han, K., Hansen, E., Heeger, K. M., Hennings-Yeomans, R., Hickerson, K. P., Huang, H. Z., Kadel, R., Keppel, G., Kolomensky, Yu. G., Leder, A., Ligi, C., Lim, K. E., Liu, X., Ma, Y. G., Maino, M., Marini, L., Martinez, M., Maruyama, R. H., Mei, Y., Moggi, N., Morganti, S., Mosteiro, P. J., Napolitano, T., Nones, C., Norman, E. B., Nucciotti, A., O'Donnell, T., Orio, F., Ouellet, J. L., Pagliarone, C. E., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pessina, G., Pettinacci, V., Piperno, G., Pira, C. C., Pirro, S., Pozzi, S., Previtali, E., Rosenfeld, C., Rusconi, C., Sangiorgio, S., Santone, D., Scielzo, N. D., Singh, V., Sisti, M., Smith, A. R., Taffarello, L., Tenconi, M., Terranova, F., Tomei, C., Trentalange, S., Vignati, M., Wagaarachchi, S. L., Wang, B. S., Wang, H. W., Wilson, J., Winslow, L. A., Wise, T., Woodcraft, A., Zanotti, L., Zhang, G. Q., Zhu, B. X., S., Zimmermann, and Zucchelli, S.
- Subjects
History ,Particle physics ,Physics::Instrumentation and Detectors ,dark matter: direct detection ,[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex] ,01 natural sciences ,Education ,Physics and Astronomy (all) ,energy: threshold ,Low energy ,CUORE ,double-beta decay: (0neutrino) ,bolometer ,Double beta decay ,0103 physical sciences ,semiconductor counter ,010306 general physics ,detector: design ,energy: low ,Physics ,010308 nuclear & particles physics ,Astrophysics::Instrumentation and Methods for Astrophysics ,Energy: threshold | trigger: efficiency | dark matter: direct detection | axion: solar | energy: low | CUORE | double-beta decay | Gran Sasso | bolometer | observatory | calibration | sensitivity | performance | background | cryogenics ,calibration ,Gran Sasso ,Computer Science Applications ,Continuous data ,cryogenics ,trigger: efficiency ,electronics: readout ,axion: solar ,National laboratory ,tellurium compounds ,Tellurium compounds ,Data selection - Abstract
Author(s): Copello, S; Alduino, C; Alfonso, K; Artusa, DR; Avignone, FT; Azzolini, O; Banks, TI; Bari, G; Beeman, JW; Bellini, F; Bersani, A; Biassoni, M; Branca, A; Brofferio, C; Bucci, C; Camacho, A; Caminata, A; Canonica, L; Cao, XG; Capelli, S; Cappelli, L; Carbone, L; Cardani, L; Carniti, P; Casali, N; Cassina, L; Chiesa, D; Chott, N; Clemenza, M; Cosmelli, C; Cremonesi, O; Creswick, RJ; Cushman, JS; D'Addabbo, A; Dafinei, I; Davis, CJ; Dell'Oro, S; Deninno, MM; Di Domizio, S; Di Vacri, ML; Drobizhev, A; Fang, DQ; Faverzani, M; Fernandes, G; Ferri, E; Ferroni, F; Fiorini, E; Franceschi, MA; Freedman, SJ; Fujikawa, BK; Giachero, A; Gironi, L; Giuliani, A; Gladstone, L; Gorla, P; Gotti, C; Gutierrez, TD; Haller, EE; Han, K; Hansen, E; Heeger, KM; Hennings-Yeomans, R; Hickerson, KP; Huang, HZ; Kadel, R; Keppel, G; Kolomensky, YG; Leder, A; Ligi, C; Lim, KE; Liu, X; Ma, YG; Maino, M; Marini, L; Martinez, M; Maruyama, RH; Mei, Y; Moggi, N; Morganti, S; Mosteiro, PJ; Napolitano, T; Nones, C; Norman, EB; Nucciotti, A; O'Donnell, T | Abstract: The Cryogenic Underground Observatory for Rare Events (CUORE) is a ton-scale double beta decay experiment based on TeO2 cryogenic bolometers and is currently in the last construction stage at the Gran Sasso National Laboratory (LNGS). Its primary goal is to observe neutrino-less double beta decay of 130Te, however thanks to the ultra-low background and large projected exposure it could also be suitable for other rare event searches, as the detection of solar axions, neutrinos from type II supernovae or direct detection of dark matter. The sensitivity for these searches will depend on the performance achieved at the low energy threshold. For this reason a trigger algorithm based on continuous data filtering has been developed which will allow lowering the threshold down to the few keV region. The new trigger has been tested in CUORE-0, a single-tower CUORE prototype consisting of 52 TeO2 bolometers and recently concluded, and here we present the results in terms of trigger efficiency, data selection and low-energy calibration.
- Published
- 2017
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