Dark Matter Search with CUORE-0 and CUORE

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;

doi:10.1016/j.phpro.2014.12.005

Dark Matter Search with CUORE-0 and CUORE

Clicks: 268

ID: 117781

2015

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Abstract

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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.

Reference Key	zucchelli2015physicsdark Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
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 Searching for DOI...
URL	https://sciprofiles.com/publication/view/9b214639e0c48da60d42d66a228c2938 https://doi.org/10.1016/j.phpro.2014.12.005
Keywords	cuore dark matter tellurium low threshold

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