CAS OpenIR  > 中科院上海应用物理研究所2011-2019年
Status and prospects for CUORE
Canonica, L; 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; Cao, XG; Capelli, S; Cappelli, L; Carbone, L; Cardani, L; Carniti, P; Casali, N; Cassina, L; Chiesa, D; Chott, N; Clemenza, M; Copello, S; 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; Novati, V; 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; 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 Name27th International Conference on Neutrino Physics and Astrophysics (Neutrino)
Source PublicationXXVII INTERNATIONAL CONFERENCE ON NEUTRINO PHYSICS AND ASTROPHYSICS (NEUTRINO2016)
Issue
Conference DateJUL 04-09, 2016
Conference PlaceRoyal Geog Soc, London, ENGLAND
AbstractCUORE is a cryogenic detector consisting of 988 TeO2 crystals, 750 g each, and will be operated at a temperature of similar to 10 mK, to search for neutrinoless double beta decay (0 nu beta beta) of Te-130. The detector, in the final stages of construction at the Laboratori Nazionali del Gran Sasso (Italy), will start its operations in 2016. CUORE-0, its pilot experiment, has proven the feasibility of CUORE, demonstrating that the target background of 0.01 counts/keV/kg/y and the energy resolution of 5 keV are within reach. CUORE-0 also made the most precise measurement of the 2 nu beta beta decay. The expected sensitivity of CUORE to the 0 nu beta beta Te-130 half-life is 9 . 10(25) y, for 5 years of data taking. Here, we report the most recent results of CUORE-0, their implications for CUORE, and the current status of the CUORE experiment.
ISSN1742-6588
Subtype会议论文
DOI10.1088/1742-6596/888/1/012034
Indexed BySCI
Language英语
Citation statistics
Document Type会议论文
Identifierhttp://ir.sinap.ac.cn/handle/331007/31934
Collection中科院上海应用物理研究所2011-2019年
Affiliation1.Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67010 Laquila, Italy
2.Univ South Carolina, Dept Phys & Astron, Columbia, SC 29208 USA
3.Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
4.Ist Nazl Fis Nucl, Lab Nazl Legnaro, I-35020 Padua, Italy
5.Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
6.Lawrence Berkeley Natl Lab, Div Nucl Sci, Berkeley, CA 94720 USA
7.Ist Nazl Fis Nucl, Sez Bologna, I-40127 Bologna, Italy
8.Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA
9.Sapienza Univ Roma, Dipartimento Fis, I-00185 Rome, Italy
10.Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy
11.Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy
12.Univ Milano Bicocca, Dipartimento Fis, I-20126 Milan, Italy
13.Ist Nazl Fis Nucl, Sez Milano Bicocca, I-20126 Milan, Italy
14.Chinese Acad Sci, Shanghai Inst Appl Phys, Shanghai 201800, Peoples R China
15.Univ Cassino & Lazio Merid, Dipartimento Ingn Civile & Meccan, I-03043 Cassino, Italy
16.Univ Genoa, Dipartimento Fis, I-16146 Genoa, Italy
17.Yale Univ, Dept Phys, New Haven, CT 06520 USA
18.Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA
19.Ist Nazl Fis Nucl, Gran Sasso Sci Inst, I-67100 Laquila, Italy
20.Univ Aquila, Dipartimento Sci Fis & Chim, I-67100 Laquila, Italy
21.Univ Paris Saclay, CSNSM, Univ Paris Sud, CNRS,IN2P3, F-91405 Orsay, France
22.MIT, 77 Massachusetts Ave, Cambridge, MA 02139 USA
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.Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA
26.Univ Zaragoza, Lab Fis Nucl & Astroparticulas, E-50009 Zaragoza, Spain
27.Univ Bologna, Dipartimento Sci Qualita Vita, Alma Mater Studiorum, I-47921 Bologna, Italy
28.CEA Saclay, Serv Phys Particules, F-91191 Gif Sur Yvette, France
29.Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
30.Univ Calif Berkeley, Dept Nucl Engn, Berkeley, CA 94720 USA
31.Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy
32.Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Rome, Italy
33.Ist Nazl Fis Nucl, Sez Firenze, I-50125 Florence, Italy
34.Lawrence Berkeley Natl Lab, Div Engn, Berkeley, CA 94720 USA
35.Univ Bologna, Dipartimento Fis & Astron, Alma Mater Studiorum, I-40127 Bologna, Italy
36.Virginia Polytech Inst & State Univ, Ctr Neutrino Phys, Blacksburg, VA 24061 USA
37.Univ Edinburgh, SUPA, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
Recommended Citation
GB/T 7714
Canonica, L,Alduino, C,Alfonso, K,et al. Status and prospects for CUORE[C],2017.
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