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Lowering the CUORE energy threshold | |
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; Orio, F; Ouellet, JL; Pagliarone, CE; 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, ND; Singh, V; Sisti, M; Smith, AR; Taffarello, L; Tenconi, M; Terranova, F; Tomei, C; Trentalange, S; Vignati, M; Wagaarachchi, SL; Wang, BS; Wang, HW; Wilson, J; Winslow, LA; Wise, T; Woodcraft, A; Zanotti, L; Zhang, GQ; Zhu, BX; Zimmermann, S; Zucchelli, S | |
2017 | |
Conference Name | 27th International Conference on Neutrino Physics and Astrophysics (Neutrino) |
Source Publication | XXVII INTERNATIONAL CONFERENCE ON NEUTRINO PHYSICS AND ASTROPHYSICS (NEUTRINO2016) |
Issue | — |
Conference Date | JUL 04-09, 2016 |
Conference Place | Royal Geog Soc, London, ENGLAND |
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 Te-130, 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. |
ISSN | 1742-6588 |
Subtype | 会议论文 |
DOI | 10.1088/1742-6596/888/1/012047 |
Indexed By | SCI |
Language | 英语 |
Citation statistics | |
Document Type | 会议论文 |
Identifier | http://ir.sinap.ac.cn/handle/331007/31928 |
Collection | 中科院上海应用物理研究所2011-2020年 |
Affiliation | 1.Univ Genoa, Dipartimento Fis, I-16146 Genoa, Italy 2.INFN, Sez Genova, I-16146 Genoa, Italy 3.Univ South Carolina, Dept Phys & Astron, Columbia, SC 29208 USA 4.Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA 5.INFN, Lab Nazl Gran Sasso, I-67010 Laquila, Italy 6.INFN, Lab Nazl Legnaro, I-35020 Padua, Italy 7.Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA 8.Lawrence Berkeley Natl Lab, Div Nucl Sci, Berkeley, CA 94720 USA 9.INFN, Sez Bologna, I-40127 Bologna, Italy 10.Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA 11.Sapienza Univ Roma, Dipartimento Fis, I-00185 Rome, Italy 12.INFN, Sez Roma, I-00185 Rome, Italy 13.Univ Milano Bicocca, Dipartimento Fis, I-20126 Milan, Italy 14.INFN, Sez Milano Bicocca, I-20126 Milan, Italy 15.INFN, Sez Padova, I-35131 Padua, Italy 16.MIT, 77 Massachusetts Ave, Cambridge, MA 02139 USA 17.Chinese Acad Sci, Shanghai Inst Appl Phys, Shanghai 201800, Peoples R China 18.Yale Univ, Dept Phys, New Haven, CT 06520 USA 19.INFN, Gran Sasso Sci Inst, I-67100 Laquila, Italy 20.Univ Aquila, Dipartimento Sci Fis & Chim, I-67100 Laquila, Italy 21.INFN, Nazl Frascati Lab, I-00044 Rome, Italy 22.Univ Paris Saclay, Univ Paris Sud, IN2P3, CSNSM,CNRS, F-91405 Orsay, France 23.Calif Polytech State Univ San Luis Obispo, Dept Phys, San Luis Obispo, CA 93407 USA 24.Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA 25.Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai 200240, Peoples R China 26.Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA 27.Univ Zaragoza, Lab Fis Nucl & Astroparticulas, E-50009 Zaragoza, Spain 28.Univ Bologna, Alma Mater Studiorum, Dipartimento Sci Qual Vita, I-47921 Bologna, Italy 29.CEA Saclay, Serv Phys Particules, F-91191 Gif Sur Yvette, France 30.Lawrence Livermore Natl Lab, Livermore, CA 94550 USA 31.Univ Calif Berkeley, Dept Nucl Engn, Berkeley, CA 94720 USA 32.Virginia Polytech Inst & State Univ, Ctr Neutrino Phys, Blacksburg, VA 24061 USA 33.Univ Cassino & Lazio Merid, Dipartimento Ingn Civile & Meccan, I-03043 Cassino, Italy 34.Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA 35.Univ Edinburgh, Inst Astron, SUPA, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland 36.Lawrence Berkeley Natl Lab, Div Engn, Berkeley, CA 94720 USA 37.Univ Bologna, Alma Mater Studiorum, Dipartimento Fis & Astron, I-40127 Bologna, Italy |
Recommended Citation GB/T 7714 | Copello, S,Alduino, C,Alfonso, K,et al. Lowering the CUORE energy threshold[C],2017. |
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