Dark Matter Search with CUORE-0 and CUORE
Clicks: 130
ID: 117781
2015
The Cryogenic Underground Observatory for Rare Events (CUORE) is a ton-scale experiment made of TeO2 bolometers that will probe the neutrinoless double beta decay of 130Te. Excellent energy resolution, low threshold and low background make CUORE sensitive to nuclear recoils, allowing a search for dark matter interactions. With a total mass of 741 kg of TeO2, CUORE can search for an annual modulation of the counting rate at low energies. We present data obtained with CUORE-like detectors and the prospects for a dark matter search in CUORE-0, a 40-kg prototype, and CUORE.
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zucchelli2015physicsdark
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| Authors | C.P. Aguirre,D.R. Artusa,F.T. Avignone,O. Azzolini,M. Balata,T.I. Banks,G. Bari,J. Beeman,F. Bellini,A. Bersani,M. Biassoni,C Brofferio,C Bucci,X.Z. Cai,A. Camacho,L. Canonica,X. Cao,S. Capelli,L. Carbone,L. Cardani,M. Carrettoni,N. Casali,D. Chiesa,N. Chott,Massimiliano Clemenza,C. Cosmelli,O. Cremonesi,R.J. Creswick,I. Dafinei,A. Dally,V. Datskov,A. De Biasi,M.M. DeNinno,S. Di Domizio,M.L. Di Vacri,L. Ejzak,D.Q. Fang,H.A. Farach,M. Faverzani,G. Fernandes,E. Ferri,F. Ferroni,E. Fiorini,M.A. Franceschi,S.J. Freedman,B.K. Fujikawa,Andrea Giachero,Luca Gironi,A. Giuliani,J. Goett,P. Gorla,C. Gotti,T.D. Gutierrez,E.E. Haller,K. Han,K.M. Heeger,R. Hennings-Yeomans,H.Z. Huang,R. Kadel,K. Kazkaz,G. Keppel,Yu.G. Kolomensky,Y.L. Li,C. Ligi,X. Liu,Y.G. Ma,C. Maiano,M. Maino,M. Martinez,R.H. Maruyama,Y. Mei,N. Moggi,S. Morganti,T. Napolitano,S. Nisi,C. Nones,E.B. Norman,A. Nucciotti,T. O’Donnell,F. Orio,D. Orlandi,J.L. Ouellet,M. Pallavicini,V. Palmieri,Luca Pattavina,Maura Pavan,M. Pedretti,G. Pessina,G. Piperno,C. Pira,S. Pirro,E. Previtali,V. Rampazzo,C. Rosenfeld,C. Rusconi,E. Sala,S. Sangiorgio,N.D. Scielzo,M. Sisti,A.R. Smith,L. Taffarello,M. Tenconi,F. Terranova,W.D. Tian,C. Tomei,S. Trentalange,G. Ventura,M. Vignati,B.S. Wang,H.W. Wang,L. Wielgus,J. Wilson,L.A. Winslow,T. Wise,A. Woodcraft,L. Zanotti,C. Zarra,B.X. Zhu,S. Zucchelli;C.P. Aguirre;D.R. Artusa;F.T. Avignone;O. Azzolini;M. Balata;T.I. Banks;G. Bari;J. Beeman;F. Bellini;A. Bersani;M. Biassoni;C Brofferio;C Bucci;X.Z. Cai;A. Camacho;L. Canonica;X. Cao;S. Capelli;L. Carbone;L. Cardani;M. Carrettoni;N. Casali;D. Chiesa;N. Chott;Massimiliano Clemenza;C. Cosmelli;O. Cremonesi;R.J. Creswick;I. Dafinei;A. Dally;V. Datskov;A. De Biasi;M.M. DeNinno;S. Di Domizio;M.L. Di Vacri;L. Ejzak;D.Q. Fang;H.A. Farach;M. Faverzani;G. Fernandes;E. Ferri;F. Ferroni;E. Fiorini;M.A. Franceschi;S.J. Freedman;B.K. Fujikawa;Andrea Giachero;Luca Gironi;A. Giuliani;J. Goett;P. Gorla;C. Gotti;T.D. Gutierrez;E.E. Haller;K. Han;K.M. Heeger;R. Hennings-Yeomans;H.Z. Huang;R. Kadel;K. Kazkaz;G. Keppel;Yu.G. Kolomensky;Y.L. Li;C. Ligi;X. Liu;Y.G. Ma;C. Maiano;M. Maino;M. Martinez;R.H. Maruyama;Y. Mei;N. Moggi;S. Morganti;T. Napolitano;S. Nisi;C. Nones;E.B. Norman;A. Nucciotti;T. O’Donnell;F. Orio;D. Orlandi;J.L. Ouellet;M. Pallavicini;V. Palmieri;Luca Pattavina;Maura Pavan;M. Pedretti;G. Pessina;G. Piperno;C. Pira;S. Pirro;E. Previtali;V. Rampazzo;C. Rosenfeld;C. Rusconi;E. Sala;S. Sangiorgio;N.D. Scielzo;M. Sisti;A.R. Smith;L. Taffarello;M. Tenconi;F. Terranova;W.D. Tian;C. Tomei;S. Trentalange;G. Ventura;M. Vignati;B.S. Wang;H.W. Wang;L. Wielgus;J. Wilson;L.A. Winslow;T. Wise;A. Woodcraft;L. Zanotti;C. Zarra;B.X. Zhu;S. Zucchelli; |
| Journal | physics procedia |
| Year | 2015 |
| DOI | 10.1016/j.phpro.2014.12.005 |
| URL | |
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