CUORE and Beyond: Bolometric Techniques to Explore Inverted Neutrino Mass Hierarchy

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.G. Cao,S. Capelli,L. Carbone,L. Cardani,M. Carrettoni,N. Casali,D. Chiesa,N. Chott,Massimiliano Clemenza,S. Copello,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,V. Pettinacci,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; 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.G. Cao; S. Capelli; L. Carbone; L. Cardani; M. Carrettoni; N. Casali; D. Chiesa; N. Chott; Massimiliano Clemenza; S. Copello; 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; V. Pettinacci; 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

CUORE and Beyond: Bolometric Techniques to Explore Inverted Neutrino Mass Hierarchy

Clicks: 181

ID: 120211

2015

The CUORE (Cryogenic Underground Observatory for Rare Events) experiment will search for neutrinoless double beta decay of 130Te. With 741 kg of TeO2 crystals and an excellent energy resolution of 5 keV (0.2%) at the region of interest, CUORE will be one of the most competitive neutrinoless double beta decay experiments on the horizon. With five years of live time, CUORE projected neutrinoless double beta decay half-life sensitivity is 1.6 × 1026 y at 1σ (9.5 × 1025 y at the 90% confidence level), which corresponds to an upper limit on the effective Majorana mass in the range 40–100 meV (50–130 meV). Further background rejection with auxiliary light detector can significantly improve the search sensitivity and competitiveness of bolometric detectors to fully explore the inverted neutrino mass hierarchy with 130Te and possibly other double beta decay candidate nuclei.

Reference Key	zucchelli2015physicscuore Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors	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.G. Cao,S. Capelli,L. Carbone,L. Cardani,M. Carrettoni,N. Casali,D. Chiesa,N. Chott,Massimiliano Clemenza,S. Copello,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,V. Pettinacci,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;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.G. Cao;S. Capelli;L. Carbone;L. Cardani;M. Carrettoni;N. Casali;D. Chiesa;N. Chott;Massimiliano Clemenza;S. Copello;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;V. Pettinacci;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.2014.12.039
URL	https://sciprofiles.com/publication/view/8e9b660b79e6df3212e5e8b62aea19c4 https://doi.org/10.1016/j.phpro.2014.12.039
Keywords	neutrino mass cuore inverted neutrino explore inverted bolometric techniques mass hierarchy

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