The low energy spectrum of TeO2 bolometers: Results and dark matter perspectives for the CUORE-0 and CUORE experiments

F. Alessandria; R. Ardito; D. R. Artusa; F. T. Avignone; O. Azzolini; M. Balata; T. I. Banks; G. Bari; J. Beeman; F. Bellini; A. Bersani; M. Biassoni; T. Bloxham; C. Brofferio; C. Bucci; X. Z. Cai; L. Canonica; S. Capelli; L. Carbone; L. Cardani; M. Carrettoni; N. Casali; N. Chott; M. Clemenza; C. Cosmelli; O. Cremonesi; R. J. Creswick; I. Dafinei; A. Dally; V. Datskov; A. De Biasi; M. P. Decowski; M. M. Deninno; S. Di Domizio; M. L. Di Vacri; L. Ejzak; R. Faccini; D. Q. Fang; H. A. Farach; E. Ferri; F. Ferroni; E. Fiorini; M. A. Franceschi; S. J. Freedman; B. K. Fujikawa; A. Giachero; L. Gironi; A. Giuliani; J. Goett; P. Gorla; C. Gotti; E. Guardincerri; T. D. Gutierrez; E. E. Haller; K. Han; K. M. Heeger; H. Z. Huang; R. Kadel; K. Kazkaz; G. Keppel; L. Kogler; Yu G. Kolomensky; D. Lenz; Y. L. Li; C. Ligi; X. Liu; Y. G. Ma; C. Maiano; M. Maino; M. Martinez; R. H. Maruyama; N. Moggi; S. Morganti; T. Napolitano; S. Newman; S. Nisi; C. Nones; E. B. Norman; A. Nucciotti; F. Orio; D. Orlandi; J. L. Ouellet; M. Pallavicini; V. Palmieri; L. Pattavina; M. Pavan; M. Pedretti; G. Pessina; S. Pirro; E. Previtali; V. Rampazzo; F. Rimondi; C. Rosenfeld; C. Rusconi; S. Sangiorgio; N. D. Scielzo; M. Sisti; A. R. Smith; F. Stivanello; L. Taffarello; M. Tenconi; W. D. Tian; C. Tomei; S. Trentalange; G. Ventura; M. Vignati; B. S. Wang; H. W. Wang; C. A. Whitten; T. Wise; A. Woodcraft; L. Zanotti; C. Zarra; B. X. Zhu; S. Zucchelli

doi:10.1088/1475-7516/2013/01/038

The low energy spectrum of TeO₂ bolometers: Results and dark matter perspectives for the CUORE-0 and CUORE experiments

F. Alessandria, R. Ardito, D. R. Artusa, F. T. Avignone, O. Azzolini, M. Balata, T. I. Banks, G. Bari, J. Beeman, F. Bellini, A. Bersani, M. Biassoni, T. Bloxham, C. Brofferio, C. Bucci, X. Z. Cai, L. Canonica, S. Capelli, L. Carbone, L. CardaniM. Carrettoni, N. Casali, N. Chott, M. Clemenza, C. Cosmelli, O. Cremonesi, R. J. Creswick, I. Dafinei, A. Dally, V. Datskov, A. De Biasi, M. P. Decowski, M. M. Deninno, S. Di Domizio, M. L. Di Vacri, L. Ejzak, R. Faccini, D. Q. Fang, H. A. Farach, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, J. Goett, P. Gorla, C. Gotti, E. Guardincerri, T. D. Gutierrez, E. E. Haller, K. Han, K. M. Heeger, H. Z. Huang, R. Kadel, K. Kazkaz, G. Keppel, L. Kogler, Yu G. Kolomensky, D. Lenz, Y. L. Li, C. Ligi, X. Liu, Y. G. Ma, C. Maiano, M. Maino, M. Martinez, R. H. Maruyama, N. Moggi, S. Morganti, T. Napolitano, S. Newman, S. Nisi, C. Nones, E. B. Norman, A. Nucciotti, F. Orio, D. Orlandi, J. L. Ouellet, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, M. Pedretti, G. Pessina, S. Pirro, E. Previtali, V. Rampazzo, F. Rimondi, C. Rosenfeld, C. Rusconi, S. Sangiorgio, N. D. Scielzo, M. Sisti, A. R. Smith, F. Stivanello, L. Taffarello, M. Tenconi, W. D. Tian, C. Tomei, S. Trentalange, G. Ventura, M. Vignati, B. S. Wang, H. W. Wang, C. A. Whitten, T. Wise, A. Woodcraft, L. Zanotti, C. Zarra, B. X. Zhu, S. Zucchelli

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Abstract

We collected 19.4 days of data from four 750 g TeO₂ bolometers, and in three of them we were able to set the energy threshold around 3 keV using a new analysis technique. We found a background rate ranging from 25 cpd/keV/kg at 3 keV to 2 cpd/keV/kg at 25 keV, and a peak at 4.7 keV. The origin of this peak is presently unknown, but its presence is confirmed by a reanalysis of 62.7 kg·days of data from the finished CUORICINO experiment. Finally, we report the expected sensitivities of the CUORE-0 (52 bolometers) and CUORE (988 bolometers) experiments to a WIMP annual modulation signal.

Original language	English (US)
Article number	038
Journal	Journal of Cosmology and Astroparticle Physics
Volume	2013
Issue number	1
DOIs	https://doi.org/10.1088/1475-7516/2013/01/038
State	Published - Jan 2013
Externally published	Yes

ASJC Scopus subject areas

Astronomy and Astrophysics

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10.1088/1475-7516/2013/01/038

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Alessandria, F., Ardito, R., Artusa, D. R., Avignone, F. T., Azzolini, O., Balata, M., Banks, T. I., Bari, G., Beeman, J., Bellini, F., Bersani, A., Biassoni, M., Bloxham, T., Brofferio, C., Bucci, C., Cai, X. Z., Canonica, L., Capelli, S., Carbone, L., ... Zucchelli, S. (2013). The low energy spectrum of TeO₂ bolometers: Results and dark matter perspectives for the CUORE-0 and CUORE experiments. Journal of Cosmology and Astroparticle Physics, 2013(1), Article 038. https://doi.org/10.1088/1475-7516/2013/01/038

Alessandria, F, Ardito, R, Artusa, DR, Avignone, FT, Azzolini, O, Balata, M, Banks, TI, Bari, G, Beeman, J, Bellini, F, Bersani, A, Biassoni, M, Bloxham, T, Brofferio, C, Bucci, C, Cai, XZ, Canonica, L, Capelli, S, Carbone, L, Cardani, L, Carrettoni, M, Casali, N, Chott, N, Clemenza, M, Cosmelli, C, Cremonesi, O, Creswick, RJ, Dafinei, I, Dally, A, Datskov, V, De Biasi, A, Decowski, MP, Deninno, MM, Di Domizio, S, Di Vacri, ML, Ejzak, L, Faccini, R, Fang, DQ, Farach, HA, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, MA, Freedman, SJ, Fujikawa, BK, Giachero, A, Gironi, L, Giuliani, A, Goett, J, Gorla, P, Gotti, C, Guardincerri, E, Gutierrez, TD, Haller, EE, Han, K, Heeger, KM, Huang, HZ, Kadel, R, Kazkaz, K, Keppel, G, Kogler, L, Kolomensky, YG, Lenz, D, Li, YL, Ligi, C, Liu, X, Ma, YG, Maiano, C, Maino, M, Martinez, M, Maruyama, RH, Moggi, N, Morganti, S, Napolitano, T, Newman, S, Nisi, S, Nones, C, Norman, EB, Nucciotti, A, Orio, F, Orlandi, D, Ouellet, JL, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pedretti, M, Pessina, G, Pirro, S, Previtali, E, Rampazzo, V, Rimondi, F, Rosenfeld, C, Rusconi, C, Sangiorgio, S, Scielzo, ND, Sisti, M, Smith, AR, Stivanello, F, Taffarello, L, Tenconi, M, Tian, WD, Tomei, C, Trentalange, S, Ventura, G, Vignati, M, Wang, BS, Wang, HW, Whitten, CA, Wise, T, Woodcraft, A, Zanotti, L, Zarra, C, Zhu, BX & Zucchelli, S 2013, 'The low energy spectrum of TeO₂ bolometers: Results and dark matter perspectives for the CUORE-0 and CUORE experiments', Journal of Cosmology and Astroparticle Physics, vol. 2013, no. 1, 038. https://doi.org/10.1088/1475-7516/2013/01/038

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title = "The low energy spectrum of TeO2 bolometers: Results and dark matter perspectives for the CUORE-0 and CUORE experiments",

abstract = "We collected 19.4 days of data from four 750 g TeO2 bolometers, and in three of them we were able to set the energy threshold around 3 keV using a new analysis technique. We found a background rate ranging from 25 cpd/keV/kg at 3 keV to 2 cpd/keV/kg at 25 keV, and a peak at 4.7 keV. The origin of this peak is presently unknown, but its presence is confirmed by a reanalysis of 62.7 kg·days of data from the finished CUORICINO experiment. Finally, we report the expected sensitivities of the CUORE-0 (52 bolometers) and CUORE (988 bolometers) experiments to a WIMP annual modulation signal.",

author = "F. Alessandria and R. Ardito and Artusa, {D. R.} and Avignone, {F. T.} and O. Azzolini and M. Balata and Banks, {T. I.} and G. Bari and J. Beeman and F. Bellini and A. Bersani and M. Biassoni and T. Bloxham and C. Brofferio and C. Bucci and Cai, {X. Z.} and L. Canonica and S. Capelli and L. Carbone and L. Cardani and M. Carrettoni and N. Casali and N. Chott and M. Clemenza and C. Cosmelli and O. Cremonesi and Creswick, {R. J.} and I. Dafinei and A. Dally and V. Datskov and {De Biasi}, A. and Decowski, {M. P.} and Deninno, {M. M.} and {Di Domizio}, S. and {Di Vacri}, {M. L.} and L. Ejzak and R. Faccini and Fang, {D. Q.} and Farach, {H. A.} 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 J. Goett and P. Gorla and C. Gotti and E. Guardincerri and Gutierrez, {T. D.} and Haller, {E. E.} and K. Han and Heeger, {K. M.} and Huang, {H. Z.} and R. Kadel and K. Kazkaz and G. Keppel and L. Kogler and Kolomensky, {Yu G.} and D. Lenz and Li, {Y. L.} and C. Ligi and X. Liu and Ma, {Y. G.} and C. Maiano and M. Maino and M. Martinez and Maruyama, {R. H.} and N. Moggi and S. Morganti and T. Napolitano and S. Newman and S. Nisi and C. Nones and Norman, {E. B.} and A. Nucciotti and F. Orio and D. Orlandi and Ouellet, {J. L.} and M. Pallavicini and V. Palmieri and L. Pattavina and M. Pavan and M. Pedretti and G. Pessina and S. Pirro and E. Previtali and V. Rampazzo and F. Rimondi and C. Rosenfeld and C. Rusconi and S. Sangiorgio and Scielzo, {N. D.} and M. Sisti and Smith, {A. R.} and F. Stivanello and L. Taffarello and M. Tenconi and Tian, {W. D.} and C. Tomei and S. Trentalange and G. Ventura and M. Vignati and Wang, {B. S.} and Wang, {H. W.} and Whitten, {C. A.} and T. Wise and A. Woodcraft and L. Zanotti and C. Zarra and Zhu, {B. X.} and S. Zucchelli",

year = "2013",

month = jan,

doi = "10.1088/1475-7516/2013/01/038",

language = "English (US)",

volume = "2013",

journal = "Journal of Cosmology and Astroparticle Physics",

issn = "1475-7516",

publisher = "IOP Publishing Ltd.",

number = "1",

}

TY - JOUR

T1 - The low energy spectrum of TeO2 bolometers

T2 - Results and dark matter perspectives for the CUORE-0 and CUORE experiments

AU - Alessandria, F.

AU - Ardito, R.

AU - Artusa, D. R.

AU - Avignone, F. T.

AU - Azzolini, O.

AU - Balata, M.

AU - Banks, T. I.

AU - Bari, G.

AU - Beeman, J.

AU - Bellini, F.

AU - Bersani, A.

AU - Biassoni, M.

AU - Bloxham, T.

AU - Brofferio, C.

AU - Bucci, C.

AU - Cai, X. Z.

AU - Canonica, L.

AU - Capelli, S.

AU - Carbone, L.

AU - Cardani, L.

AU - Carrettoni, M.

AU - Casali, N.

AU - Chott, N.

AU - Clemenza, M.

AU - Cosmelli, C.

AU - Cremonesi, O.

AU - Creswick, R. J.

AU - Dafinei, I.

AU - Dally, A.

AU - Datskov, V.

AU - De Biasi, A.

AU - Decowski, M. P.

AU - Deninno, M. M.

AU - Di Domizio, S.

AU - Di Vacri, M. L.

AU - Ejzak, L.

AU - Faccini, R.

AU - Fang, D. Q.

AU - Farach, H. A.

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 - Goett, J.

AU - Gorla, P.

AU - Gotti, C.

AU - Guardincerri, E.

AU - Gutierrez, T. D.

AU - Haller, E. E.

AU - Han, K.

AU - Heeger, K. M.

AU - Huang, H. Z.

AU - Kadel, R.

AU - Kazkaz, K.

AU - Keppel, G.

AU - Kogler, L.

AU - Kolomensky, Yu G.

AU - Lenz, D.

AU - Li, Y. L.

AU - Ligi, C.

AU - Liu, X.

AU - Ma, Y. G.

AU - Maiano, C.

AU - Maino, M.

AU - Martinez, M.

AU - Maruyama, R. H.

AU - Moggi, N.

AU - Morganti, S.

AU - Napolitano, T.

AU - Newman, S.

AU - Nisi, S.

AU - Nones, C.

AU - Norman, E. B.

AU - Nucciotti, A.

AU - Orio, F.

AU - Orlandi, D.

AU - Ouellet, J. L.

AU - Pallavicini, M.

AU - Palmieri, V.

AU - Pattavina, L.

AU - Pavan, M.

AU - Pedretti, M.

AU - Pessina, G.

AU - Pirro, S.

AU - Previtali, E.

AU - Rampazzo, V.

AU - Rimondi, F.

AU - Rosenfeld, C.

AU - Rusconi, C.

AU - Sangiorgio, S.

AU - Scielzo, N. D.

AU - Sisti, M.

AU - Smith, A. R.

AU - Stivanello, F.

AU - Taffarello, L.

AU - Tenconi, M.

AU - Tian, W. D.

AU - Tomei, C.

AU - Trentalange, S.

AU - Ventura, G.

AU - Vignati, M.

AU - Wang, B. S.

AU - Wang, H. W.

AU - Whitten, C. A.

AU - Wise, T.

AU - Woodcraft, A.

AU - Zanotti, L.

AU - Zarra, C.

AU - Zhu, B. X.

AU - Zucchelli, S.

PY - 2013/1

Y1 - 2013/1

N2 - We collected 19.4 days of data from four 750 g TeO2 bolometers, and in three of them we were able to set the energy threshold around 3 keV using a new analysis technique. We found a background rate ranging from 25 cpd/keV/kg at 3 keV to 2 cpd/keV/kg at 25 keV, and a peak at 4.7 keV. The origin of this peak is presently unknown, but its presence is confirmed by a reanalysis of 62.7 kg·days of data from the finished CUORICINO experiment. Finally, we report the expected sensitivities of the CUORE-0 (52 bolometers) and CUORE (988 bolometers) experiments to a WIMP annual modulation signal.

AB - We collected 19.4 days of data from four 750 g TeO2 bolometers, and in three of them we were able to set the energy threshold around 3 keV using a new analysis technique. We found a background rate ranging from 25 cpd/keV/kg at 3 keV to 2 cpd/keV/kg at 25 keV, and a peak at 4.7 keV. The origin of this peak is presently unknown, but its presence is confirmed by a reanalysis of 62.7 kg·days of data from the finished CUORICINO experiment. Finally, we report the expected sensitivities of the CUORE-0 (52 bolometers) and CUORE (988 bolometers) experiments to a WIMP annual modulation signal.

UR - http://www.scopus.com/inward/record.url?scp=84873648220&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84873648220&partnerID=8YFLogxK

U2 - 10.1088/1475-7516/2013/01/038

DO - 10.1088/1475-7516/2013/01/038

M3 - Article

AN - SCOPUS:84873648220

SN - 1475-7516

VL - 2013

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

IS - 1

M1 - 038

ER -

The low energy spectrum of TeO₂ bolometers: Results and dark matter perspectives for the CUORE-0 and CUORE experiments

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