CUORE sensitivity to 0 decay

C. Alduino; K. Alfonso; D. R. Artusa; F. T. Avignone; O. Azzolini; T. I. Banks; G. Bari; J. W. Beeman; F. Bellini; G. Benato; A. Bersani; M. Biassoni; A. Branca; C. Brofferio; C. Bucci; A. Camacho; A. Caminata; L. Canonica; X. G. Cao; S. Capelli; L. Cappelli; L. Carbone; L. Cardani; P. Carniti; N. Casali; L. Cassina; D. Chiesa; N. Chott; M. Clemenza; S. Copello; C. Cosmelli; O. Cremonesi; R. J. Creswick; J. S. Cushman; A. D’Addabbo; I. Dafinei; C. J. Davis; S. Dell’Oro; M. M. Deninno; S. Di Domizio; M. L. Di Vacri; A. Drobizhev; D. Q. Fang; M. Faverzani; G. Fernandes; E. Ferri; F. Ferroni; E. Fiorini; M. A. Franceschi; S. J. Freedman; B. K. Fujikawa; A. Giachero; L. Gironi; A. Giuliani; L. Gladstone; P. Gorla; C. Gotti; T. D. Gutierrez; E. E. Haller; K. Han; E. Hansen; K. M. Heeger; R. Hennings-Yeomans; K. P. Hickerson; H. Z. Huang; R. Kadel; G. Keppel; Yu G. Kolomensky; A. Leder; C. Ligi; K. E. Lim; Y. G. Ma; M. Maino; L. Marini; M. Martinez; R. H. Maruyama; Y. Mei; N. Moggi; S. Morganti; P. J. Mosteiro; T. Napolitano; M. Nastasi; C. Nones; E. B. Norman; V. Novati; A. Nucciotti; T. O’Donnell; J. L. Ouellet; C. E. Pagliarone; M. Pallavicini; V. Palmieri; L. Pattavina; M. Pavan; G. Pessina; V. Pettinacci; G. Piperno; C. Pira; S. Pirro; S. Pozzi; E. Previtali; C. Rosenfeld; C. Rusconi; M. Sakai; S. Sangiorgio; D. Santone; B. Schmidt; J. Schmidt; N. D. Scielzo; V. Singh; M. Sisti; A. R. Smith; L. Taffarello; M. Tenconi; F. Terranova; C. Tomei; S. Trentalange; M. Vignati; S. L. Wagaarachchi; B. S. Wang; H. W. Wang; B. Welliver; J. Wilson; L. A. Winslow; T. Wise; A. Woodcraft; L. Zanotti; G. Q. Zhang; B. X. Zhu; S. Zimmermann; S. Zucchelli

doi:10.1140/epjc/s10052-017-5098-9

CUORE sensitivity to 0 decay

C. Alduino, K. Alfonso, D. R. Artusa, F. T. Avignone, O. Azzolini, T. I. Banks, G. Bari, J. W. Beeman, F. Bellini, G. Benato, A. Bersani, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, A. Camacho, A. Caminata, L. Canonica, X. G. Cao, S. CapelliL. Cappelli, L. Carbone, L. Cardani, P. Carniti, N. Casali, L. Cassina, D. Chiesa, N. Chott, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, J. S. Cushman, A. D’Addabbo, I. Dafinei, C. J. Davis, S. Dell’Oro, M. M. Deninno, S. Di Domizio, M. L. Di Vacri, A. Drobizhev, D. Q. Fang, M. Faverzani, G. Fernandes, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, L. Gladstone, P. Gorla, C. Gotti, T. D. Gutierrez, E. E. Haller, K. Han, E. Hansen, K. M. Heeger, R. Hennings-Yeomans, K. P. Hickerson, H. Z. Huang, R. Kadel, G. Keppel, Yu G. Kolomensky, A. Leder, C. Ligi, K. E. Lim, Y. G. Ma, M. Maino, L. Marini, M. Martinez, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, P. J. Mosteiro, T. Napolitano, M. Nastasi, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, T. O’Donnell, J. L. Ouellet, C. E. Pagliarone, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, G. Piperno, C. Pira, S. Pirro, S. Pozzi, E. Previtali, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, D. Santone, B. Schmidt, J. Schmidt, N. D. Scielzo, V. Singh, M. Sisti, A. R. Smith, L. Taffarello, M. Tenconi, F. Terranova, C. Tomei, S. Trentalange, M. Vignati, S. L. Wagaarachchi, B. S. Wang, H. W. Wang, B. Welliver, J. Wilson, L. A. Winslow, T. Wise, A. Woodcraft, L. Zanotti, G. Q. Zhang, B. X. Zhu, S. Zimmermann, S. Zucchelli

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47 Scopus citations

Abstract

We report a study of the CUORE sensitivity to neutrinoless double beta (0) decay. We used a Bayesian analysis based on a toy Monte Carlo (MC) approach to extract the exclusion sensitivity to the 0 decay half-life (T1/20ν) at 90 % credibility interval (CI) – i.e. the interval containing the true value of T1/20ν with 90 % probability – and the 3σ discovery sensitivity. We consider various background levels and energy resolutions, and describe the influence of the data division in subsets with different background levels. If the background level and the energy resolution meet the expectation, CUORE will reach a 90 % CI exclusion sensitivity of 2 · 10 ²⁵ year with 3 months, and 9 · 10 ²⁵ year with 5 years of live time. Under the same conditions, the discovery sensitivity after 3 months and 5 years will be 7 · 10 ²⁴ year and 4 · 10 ²⁵ year, respectively.

Original language	English (US)
Article number	532
Journal	European Physical Journal C
Volume	77
Issue number	8
DOIs	https://doi.org/10.1140/epjc/s10052-017-5098-9
State	Published - Aug 1 2017
Externally published	Yes

ASJC Scopus subject areas

Engineering (miscellaneous)
Physics and Astronomy (miscellaneous)

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10.1140/epjc/s10052-017-5098-9

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Alduino, C., Alfonso, K., Artusa, D. R., Avignone, F. T., Azzolini, O., Banks, T. I., Bari, G., Beeman, J. W., Bellini, F., Benato, G., Bersani, A., Biassoni, M., Branca, A., Brofferio, C., Bucci, C., Camacho, A., Caminata, A., Canonica, L., Cao, X. G., ... Zucchelli, S. (2017). CUORE sensitivity to 0 decay. European Physical Journal C, 77(8), Article 532. https://doi.org/10.1140/epjc/s10052-017-5098-9

Alduino, C, Alfonso, K, Artusa, DR, Avignone, FT, Azzolini, O, Banks, TI, Bari, G, Beeman, JW, Bellini, F, Benato, G, 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, 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, Ma, YG, Maino, M, Marini, L, Martinez, M, Maruyama, RH, Mei, Y, Moggi, N, Morganti, S, Mosteiro, PJ, Napolitano, T, Nastasi, M, Nones, C, Norman, EB, Novati, V, Nucciotti, A, O’Donnell, T, 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, Sakai, M, Sangiorgio, S, Santone, D, Schmidt, B, Schmidt, J, 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, Welliver, B, Wilson, J, Winslow, LA, Wise, T, Woodcraft, A, Zanotti, L, Zhang, GQ, Zhu, BX, Zimmermann, S & Zucchelli, S 2017, 'CUORE sensitivity to 0 decay', European Physical Journal C, vol. 77, no. 8, 532. https://doi.org/10.1140/epjc/s10052-017-5098-9

@article{68773be703e24a66b54098380b92d900,

title = "CUORE sensitivity to 0 decay",

abstract = "We report a study of the CUORE sensitivity to neutrinoless double beta (0) decay. We used a Bayesian analysis based on a toy Monte Carlo (MC) approach to extract the exclusion sensitivity to the 0 decay half-life (T1/20ν) at 90 % credibility interval (CI) – i.e. the interval containing the true value of T1/20ν with 90 % probability – and the 3σ discovery sensitivity. We consider various background levels and energy resolutions, and describe the influence of the data division in subsets with different background levels. If the background level and the energy resolution meet the expectation, CUORE will reach a 90 % CI exclusion sensitivity of 2 · 10 25 year with 3 months, and 9 · 10 25 year with 5 years of live time. Under the same conditions, the discovery sensitivity after 3 months and 5 years will be 7 · 10 24 year and 4 · 10 25 year, respectively.",

author = "C. Alduino and K. Alfonso and Artusa, {D. R.} and Avignone, {F. T.} and O. Azzolini and Banks, {T. I.} and G. Bari and Beeman, {J. W.} and F. Bellini and G. Benato and A. Bersani and M. Biassoni and A. Branca and C. Brofferio and C. Bucci and A. Camacho and A. Caminata and L. Canonica and Cao, {X. G.} and S. Capelli and L. Cappelli and L. Carbone and L. Cardani and P. Carniti and N. Casali and L. Cassina and D. Chiesa and N. Chott and M. Clemenza and S. Copello and C. Cosmelli and O. Cremonesi and Creswick, {R. J.} and Cushman, {J. S.} and A. D{\textquoteright}Addabbo and I. Dafinei and Davis, {C. J.} and S. Dell{\textquoteright}Oro and Deninno, {M. M.} and {Di Domizio}, S. and {Di Vacri}, {M. L.} and A. Drobizhev and Fang, {D. Q.} and M. Faverzani and G. Fernandes and E. Ferri and F. Ferroni and E. Fiorini and Franceschi, {M. A.} and Freedman, {S. J.} and Fujikawa, {B. K.} and A. Giachero and L. Gironi and A. Giuliani and L. Gladstone and P. Gorla and C. Gotti and Gutierrez, {T. D.} and Haller, {E. E.} and K. Han and E. Hansen and Heeger, {K. M.} and R. Hennings-Yeomans and Hickerson, {K. P.} and Huang, {H. Z.} and R. Kadel and G. Keppel and Kolomensky, {Yu G.} and A. Leder and C. Ligi and Lim, {K. E.} and Ma, {Y. G.} and M. Maino and L. Marini and M. Martinez and Maruyama, {R. H.} and Y. Mei and N. Moggi and S. Morganti and Mosteiro, {P. J.} and T. Napolitano and M. Nastasi and C. Nones and Norman, {E. B.} and V. Novati and A. Nucciotti and T. O{\textquoteright}Donnell and Ouellet, {J. L.} and Pagliarone, {C. E.} and M. Pallavicini and V. Palmieri and L. Pattavina and M. Pavan and G. Pessina and V. Pettinacci and G. Piperno and C. Pira and S. Pirro and S. Pozzi and E. Previtali and C. Rosenfeld and C. Rusconi and M. Sakai and S. Sangiorgio and D. Santone and B. Schmidt and J. Schmidt and Scielzo, {N. D.} and V. Singh and M. Sisti and Smith, {A. R.} and L. Taffarello and M. Tenconi and F. Terranova and C. Tomei and S. Trentalange and M. Vignati and Wagaarachchi, {S. L.} and Wang, {B. S.} and Wang, {H. W.} and B. Welliver and J. Wilson and Winslow, {L. A.} and T. Wise and A. Woodcraft and L. Zanotti and Zhang, {G. Q.} and Zhu, {B. X.} and S. Zimmermann and S. Zucchelli",

note = "Publisher Copyright: {\textcopyright} 2017, The Author(s).",

year = "2017",

month = aug,

day = "1",

doi = "10.1140/epjc/s10052-017-5098-9",

language = "English (US)",

volume = "77",

journal = "European Physical Journal C",

issn = "1434-6044",

publisher = "Springer New York",

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TY - JOUR

T1 - CUORE sensitivity to 0 decay

AU - Alduino, C.

AU - Alfonso, K.

AU - Artusa, D. R.

AU - Avignone, F. T.

AU - Azzolini, O.

AU - Banks, T. I.

AU - Bari, G.

AU - Beeman, J. W.

AU - Bellini, F.

AU - Benato, G.

AU - Bersani, A.

AU - Biassoni, M.

AU - Branca, A.

AU - Brofferio, C.

AU - Bucci, C.

AU - Camacho, A.

AU - Caminata, A.

AU - Canonica, L.

AU - Cao, X. G.

AU - Capelli, S.

AU - Cappelli, L.

AU - Carbone, L.

AU - Cardani, L.

AU - Carniti, P.

AU - Casali, N.

AU - Cassina, L.

AU - Chiesa, D.

AU - Chott, N.

AU - Clemenza, M.

AU - Copello, S.

AU - Cosmelli, C.

AU - Cremonesi, O.

AU - Creswick, R. J.

AU - Cushman, J. S.

AU - D’Addabbo, A.

AU - Dafinei, I.

AU - Davis, C. J.

AU - Dell’Oro, S.

AU - Deninno, M. M.

AU - Di Domizio, S.

AU - Di Vacri, M. L.

AU - Drobizhev, A.

AU - Fang, D. Q.

AU - Faverzani, M.

AU - Fernandes, G.

AU - Ferri, E.

AU - Ferroni, F.

AU - Fiorini, E.

AU - Franceschi, M. A.

AU - Freedman, S. J.

AU - Fujikawa, B. K.

AU - Giachero, A.

AU - Gironi, L.

AU - Giuliani, A.

AU - Gladstone, L.

AU - Gorla, P.

AU - Gotti, C.

AU - Gutierrez, T. D.

AU - Haller, E. E.

AU - Han, K.

AU - Hansen, E.

AU - Heeger, K. M.

AU - Hennings-Yeomans, R.

AU - Hickerson, K. P.

AU - Huang, H. Z.

AU - Kadel, R.

AU - Keppel, G.

AU - Kolomensky, Yu G.

AU - Leder, A.

AU - Ligi, C.

AU - Lim, K. E.

AU - Ma, Y. G.

AU - Maino, M.

AU - Marini, L.

AU - Martinez, M.

AU - Maruyama, R. H.

AU - Mei, Y.

AU - Moggi, N.

AU - Morganti, S.

AU - Mosteiro, P. J.

AU - Napolitano, T.

AU - Nastasi, M.

AU - Nones, C.

AU - Norman, E. B.

AU - Novati, V.

AU - Nucciotti, A.

AU - O’Donnell, T.

AU - Ouellet, J. L.

AU - Pagliarone, C. E.

AU - Pallavicini, M.

AU - Palmieri, V.

AU - Pattavina, L.

AU - Pavan, M.

AU - Pessina, G.

AU - Pettinacci, V.

AU - Piperno, G.

AU - Pira, C.

AU - Pirro, S.

AU - Pozzi, S.

AU - Previtali, E.

AU - Rosenfeld, C.

AU - Rusconi, C.

AU - Sakai, M.

AU - Sangiorgio, S.

AU - Santone, D.

AU - Schmidt, B.

AU - Schmidt, J.

AU - Scielzo, N. D.

AU - Singh, V.

AU - Sisti, M.

AU - Smith, A. R.

AU - Taffarello, L.

AU - Tenconi, M.

AU - Terranova, F.

AU - Tomei, C.

AU - Trentalange, S.

AU - Vignati, M.

AU - Wagaarachchi, S. L.

AU - Wang, B. S.

AU - Wang, H. W.

AU - Welliver, B.

AU - Wilson, J.

AU - Winslow, L. A.

AU - Wise, T.

AU - Woodcraft, A.

AU - Zanotti, L.

AU - Zhang, G. Q.

AU - Zhu, B. X.

AU - Zimmermann, S.

AU - Zucchelli, S.

PY - 2017/8/1

Y1 - 2017/8/1

N2 - We report a study of the CUORE sensitivity to neutrinoless double beta (0) decay. We used a Bayesian analysis based on a toy Monte Carlo (MC) approach to extract the exclusion sensitivity to the 0 decay half-life (T1/20ν) at 90 % credibility interval (CI) – i.e. the interval containing the true value of T1/20ν with 90 % probability – and the 3σ discovery sensitivity. We consider various background levels and energy resolutions, and describe the influence of the data division in subsets with different background levels. If the background level and the energy resolution meet the expectation, CUORE will reach a 90 % CI exclusion sensitivity of 2 · 10 25 year with 3 months, and 9 · 10 25 year with 5 years of live time. Under the same conditions, the discovery sensitivity after 3 months and 5 years will be 7 · 10 24 year and 4 · 10 25 year, respectively.

AB - We report a study of the CUORE sensitivity to neutrinoless double beta (0) decay. We used a Bayesian analysis based on a toy Monte Carlo (MC) approach to extract the exclusion sensitivity to the 0 decay half-life (T1/20ν) at 90 % credibility interval (CI) – i.e. the interval containing the true value of T1/20ν with 90 % probability – and the 3σ discovery sensitivity. We consider various background levels and energy resolutions, and describe the influence of the data division in subsets with different background levels. If the background level and the energy resolution meet the expectation, CUORE will reach a 90 % CI exclusion sensitivity of 2 · 10 25 year with 3 months, and 9 · 10 25 year with 5 years of live time. Under the same conditions, the discovery sensitivity after 3 months and 5 years will be 7 · 10 24 year and 4 · 10 25 year, respectively.

UR - http://www.scopus.com/inward/record.url?scp=85027148501&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85027148501&partnerID=8YFLogxK

U2 - 10.1140/epjc/s10052-017-5098-9

DO - 10.1140/epjc/s10052-017-5098-9

M3 - Article

AN - SCOPUS:85027148501

SN - 1434-6044

VL - 77

JO - European Physical Journal C

JF - European Physical Journal C

IS - 8

M1 - 532

ER -

CUORE sensitivity to 0 decay

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