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Title: Dark matter search with CUORE-0 and CUORE

Abstract

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.

Authors:
 [1];  [2];  [1];  [3];  [4];  [5];  [6];  [7];  [8];  [9];  [10];  [10];  [4];  [11];  [3];  [4];  [11];  [10];  [12];  [13] more »;  [10];  [4];  [10];  [1];  [10];  [13];  [12];  [1];  [14];  [15];  [12];  [3];  [6];  [16];  [4];  [15];  [11];  [1];  [10];  [16];  [10];  [10];  [10];  [17];  [18];  [7];  [10];  [10];  [19];  [4];  [4];  [10];  [20];  [21];  [7];  [22];  [23];  [24];  [7];  [25];  [3];  [26];  [11];  [17];  [11];  [11];  [10];  [10];  [27];  [22];  [7];  [6];  [14];  [17];  [4];  [28];  [29];  [10];  [23];  [14];  [4];  [26];  [16];  [3];  [4];  [10];  [25];  [12];  [13];  [3];  [4];  [12];  [3];  [1];  [12];  [10];  [25];  [25];  [10];  [7];  [30];  [19];  [12];  [31];  [14];  [24];  [32];  [14];  [29];  [33];  [15];  [1];  [24];  [34];  [35];  [36];  [4];  [24];  [37] « less
  1. Univ. of South Carolina, Columbia, SC (United States)
  2. Univ. of South Carolina, Columbia, SC (United States); INF - Lab. Nazionali del Gran Sasso, Assergi (Italy)
  3. INFN - Lab. Nazionali di Lagnaro, Legnaro (Italy)
  4. INF - Lab. Nazionali del Gran Sasso, Assergi (Italy)
  5. Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab.. Berkeley, CA (United States); INF - Lab. Nazionali del Gran Sasso, Assergi (Italy)
  6. INFN - Sezione di Bologna, Bologna (Italy)
  7. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  8. Sapienza Univ. of Rome (Italy); INFN - Sezione di Roma, Roma (Italy)
  9. INFN - Sezione di Genova, Genova (Italy)
  10. Univ. di Milano-Bicocca, Milano (Italy); INFN - Sezione di Milano Bicocca, Milano (Italy)
  11. Shanghai Insitute of Applied Physics (Chinese Acadmy of Science), Shanghai (China)
  12. INFN - Sezione di Milano Bicocca, Milano (Italy)
  13. Sapienza Univ. di Roma, Roma (Italy); INFN - Sezione di Roma, Roma (Italy)
  14. INFN - Sezione di Roma, Roma (Italy)
  15. Univ. of Wisconsin, Madison, WI (United States)
  16. Univ. di Genova, Genova (Italy); INFN - Sezione di Genova, Genova (Italy)
  17. INFN - Lab. Nazionali di Frascati, Frascati (Italy)
  18. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States); INFN - Sezione di Milano Biocca, Milano (Italy)
  19. Centre de Spectrometrie Nucleaire et de Spectrometrie de Masse, Orsay Campus (France)
  20. California Polytechnic State Univ. (CalPoly), San Luis Obispo, CA (United States)
  21. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of California, Berkeley, CA (United States)
  22. Yale Univ., New Haven, CT (United States)
  23. Univ. of California, Berkeley, CA (United States)
  24. Univ. of California, Los Angeles, CA (United States)
  25. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  26. Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  27. Univ. de Zaragoza, Zaragoza (Spain)
  28. Servuce de Physique des Particules, CEA, Gif-sur-Yvette (France)
  29. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States); Univ. of California, Berkeley, CA (United States)
  30. INFN - Sezione di Paova, Padova (Italy)
  31. Shangahia Institute of Applied Physics (Chinese Academy of Sciences), Shanghai (China)
  32. Univ. di Firenze, Firenze (Italy); INFN - Sezione di Firenze, Firenze (Italy)
  33. Shanghai Institute of Applied Physics (Chinese Academy of Sciences), Shanghai (China)
  34. Yale Univ., New Haven, CT (United States); Univ. of Wisconsin, Madison, WI (United States)
  35. Univ. of Edinburgh, Edinburgh (United Kingdom)
  36. Univ. di Milano-Biocca, Milano (Italy); INFN - Sezione di Milano Biocca, Milano (Italy)
  37. Univ. di Bologna, Bologna (Italy); INFN - Sezione di Bologna, Bologna (Italy)
Publication Date:
Research Org.:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE
OSTI Identifier:
1201706
Grant/Contract Number:  
AC02-05CH11231
Resource Type:
Journal Article: Accepted Manuscript
Journal Name:
Physics Procedia
Additional Journal Information:
Journal Volume: 61; Journal Issue: C; Journal ID: ISSN 1875-3892
Publisher:
Elsevier
Country of Publication:
United States
Language:
English
Subject:
46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; 79 ASTRONOMY AND ASTROPHYSICS; dark matter; tellurium; CUORE; low threshold

Citation Formats

Aguirre, C. P., Artusa, D. R., Avignone, F. T., Azzolini, O., Balata, M., Banks, T. I., Bari, G., Beeman, J., Bellini, F., Bersani, A., Biassoni, M., Brofferio, C., Bucci, C., Cai, X. Z., Camacho, A., Canonica, L., Cao, X., Capelli, S., Carbone, L., Cardani, L., Carrettoni, M., Casali, N., Chiesa, D., Chott, N., Clemenza, M., Cosmelli, C., Cremonesi, O., Creswick, R. J., Dafinei, I., Dally, A., Datskov, V., De Biasi, A., Deninno, M. M., Di Domizio, S., di Vacri, M. L., Ejzak, L., Fang, D. Q., Farach, H. A., Faverzani, M., Fernandes, G., Ferri, E., Ferroni, F., Fiorini, E., Franceschi, M. A., Freedman, S. J., Fujikawa, B. K., Giachero, A., Gironi, L., Giuliani, A., Goett, J., Gorla, P., Gotti, C., Gutierrez, T. D., Haller, E. E., Han, K., Heeger, K. M., Hennings-Yeomans, R., Huang, H. Z., Kadel, R., Kazkaz, K., Keppel, G., Kolomensky, Yu. G., Li, Y. L., Ligi, C., Liu, X., Ma, Y. G., Maiano, C., Maino, M., Martinez, M., Maruyama, R. H., Mei, Y., Moggi, N., Morganti, S., Napolitano, T., Nisi, S., Nones, C., Norman, E. B., Nucciotti, A., O’Donnell, T., Orio, F., Orlandi, D., Ouellet, J. L., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pedretti, M., Pessina, G., Piperno, G., Pira, C., Pirro, S., Previtali, E., Rampazzo, V., Rosenfeld, C., Rusconi, C., Sala, E., Sangiorgio, S., Scielzo, N. D., Sisti, M., Smith, A. R., Taffarello, L., Tenconi, M., Terranova, F., Tian, W. D., Tomei, C., Trentalange, S., Ventura, G., Vignati, M., Wang, B. S., Wang, H. W., Wielgus, L., Wilson, J., Winslow, L. A., Wise, T., Woodcraft, A., Zanotti, L., Zarra, C., Zhu, B. X., and Zucchelli, S.. Dark matter search with CUORE-0 and CUORE. United States: N. p., 2015. Web. doi:10.1016/j.phpro.2014.12.005.
Aguirre, C. P., Artusa, D. R., Avignone, F. T., Azzolini, O., Balata, M., Banks, T. I., Bari, G., Beeman, J., Bellini, F., Bersani, A., Biassoni, M., Brofferio, C., Bucci, C., Cai, X. Z., Camacho, A., Canonica, L., Cao, X., Capelli, S., Carbone, L., Cardani, L., Carrettoni, M., Casali, N., Chiesa, D., Chott, N., Clemenza, M., Cosmelli, C., Cremonesi, O., Creswick, R. J., Dafinei, I., Dally, A., Datskov, V., De Biasi, A., Deninno, M. M., Di Domizio, S., di Vacri, M. L., Ejzak, L., Fang, D. Q., Farach, H. A., Faverzani, M., Fernandes, G., Ferri, E., Ferroni, F., Fiorini, E., Franceschi, M. A., Freedman, S. J., Fujikawa, B. K., Giachero, A., Gironi, L., Giuliani, A., Goett, J., Gorla, P., Gotti, C., Gutierrez, T. D., Haller, E. E., Han, K., Heeger, K. M., Hennings-Yeomans, R., Huang, H. Z., Kadel, R., Kazkaz, K., Keppel, G., Kolomensky, Yu. G., Li, Y. L., Ligi, C., Liu, X., Ma, Y. G., Maiano, C., Maino, M., Martinez, M., Maruyama, R. H., Mei, Y., Moggi, N., Morganti, S., Napolitano, T., Nisi, S., Nones, C., Norman, E. B., Nucciotti, A., O’Donnell, T., Orio, F., Orlandi, D., Ouellet, J. L., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pedretti, M., Pessina, G., Piperno, G., Pira, C., Pirro, S., Previtali, E., Rampazzo, V., Rosenfeld, C., Rusconi, C., Sala, E., Sangiorgio, S., Scielzo, N. D., Sisti, M., Smith, A. R., Taffarello, L., Tenconi, M., Terranova, F., Tian, W. D., Tomei, C., Trentalange, S., Ventura, G., Vignati, M., Wang, B. S., Wang, H. W., Wielgus, L., Wilson, J., Winslow, L. A., Wise, T., Woodcraft, A., Zanotti, L., Zarra, C., Zhu, B. X., & Zucchelli, S.. Dark matter search with CUORE-0 and CUORE. United States. doi:10.1016/j.phpro.2014.12.005.
Aguirre, C. P., Artusa, D. R., Avignone, F. T., Azzolini, O., Balata, M., Banks, T. I., Bari, G., Beeman, J., Bellini, F., Bersani, A., Biassoni, M., Brofferio, C., Bucci, C., Cai, X. Z., Camacho, A., Canonica, L., Cao, X., Capelli, S., Carbone, L., Cardani, L., Carrettoni, M., Casali, N., Chiesa, D., Chott, N., Clemenza, M., Cosmelli, C., Cremonesi, O., Creswick, R. J., Dafinei, I., Dally, A., Datskov, V., De Biasi, A., Deninno, M. M., Di Domizio, S., di Vacri, M. L., Ejzak, L., Fang, D. Q., Farach, H. A., Faverzani, M., Fernandes, G., Ferri, E., Ferroni, F., Fiorini, E., Franceschi, M. A., Freedman, S. J., Fujikawa, B. K., Giachero, A., Gironi, L., Giuliani, A., Goett, J., Gorla, P., Gotti, C., Gutierrez, T. D., Haller, E. E., Han, K., Heeger, K. M., Hennings-Yeomans, R., Huang, H. Z., Kadel, R., Kazkaz, K., Keppel, G., Kolomensky, Yu. G., Li, Y. L., Ligi, C., Liu, X., Ma, Y. G., Maiano, C., Maino, M., Martinez, M., Maruyama, R. H., Mei, Y., Moggi, N., Morganti, S., Napolitano, T., Nisi, S., Nones, C., Norman, E. B., Nucciotti, A., O’Donnell, T., Orio, F., Orlandi, D., Ouellet, J. L., Pallavicini, M., Palmieri, V., Pattavina, L., Pavan, M., Pedretti, M., Pessina, G., Piperno, G., Pira, C., Pirro, S., Previtali, E., Rampazzo, V., Rosenfeld, C., Rusconi, C., Sala, E., Sangiorgio, S., Scielzo, N. D., Sisti, M., Smith, A. R., Taffarello, L., Tenconi, M., Terranova, F., Tian, W. D., Tomei, C., Trentalange, S., Ventura, G., Vignati, M., Wang, B. S., Wang, H. W., Wielgus, L., Wilson, J., Winslow, L. A., Wise, T., Woodcraft, A., Zanotti, L., Zarra, C., Zhu, B. X., and Zucchelli, S.. Thu . "Dark matter search with CUORE-0 and CUORE". United States. doi:10.1016/j.phpro.2014.12.005. https://www.osti.gov/servlets/purl/1201706.
@article{osti_1201706,
title = {Dark matter search with CUORE-0 and CUORE},
author = {Aguirre, C. P. and Artusa, D. R. and Avignone, F. T. and Azzolini, O. and Balata, M. and Banks, T. I. and Bari, G. and Beeman, J. and Bellini, F. and Bersani, A. and Biassoni, M. and Brofferio, C. and Bucci, C. and Cai, X. Z. and Camacho, A. and Canonica, L. and Cao, X. and Capelli, S. and Carbone, L. and Cardani, L. and Carrettoni, M. and Casali, N. and Chiesa, D. and Chott, N. and Clemenza, M. and Cosmelli, C. and Cremonesi, O. and Creswick, R. J. and Dafinei, I. and Dally, A. and Datskov, V. and De Biasi, A. and Deninno, M. M. and Di Domizio, S. and di Vacri, M. L. and Ejzak, L. and Fang, D. Q. and Farach, H. A. and Faverzani, M. and Fernandes, G. and Ferri, E. and Ferroni, F. and Fiorini, E. and Franceschi, M. A. and Freedman, S. J. and Fujikawa, B. K. and Giachero, A. and Gironi, L. and Giuliani, A. and Goett, J. and Gorla, P. and Gotti, C. and Gutierrez, T. D. and Haller, E. E. and Han, K. and Heeger, K. M. and Hennings-Yeomans, R. and Huang, H. Z. and Kadel, R. and Kazkaz, K. and Keppel, G. and Kolomensky, Yu. G. and Li, Y. L. and Ligi, C. and Liu, X. and Ma, Y. G. and Maiano, C. and Maino, M. and Martinez, M. and Maruyama, R. H. and Mei, Y. and Moggi, N. and Morganti, S. and Napolitano, T. and Nisi, S. and Nones, C. and Norman, E. B. and Nucciotti, A. and O’Donnell, T. and Orio, F. and Orlandi, D. and Ouellet, J. L. and Pallavicini, M. and Palmieri, V. and Pattavina, L. and Pavan, M. and Pedretti, M. and Pessina, G. and Piperno, G. and Pira, C. and Pirro, S. and Previtali, E. and Rampazzo, V. and Rosenfeld, C. and Rusconi, C. and Sala, E. and Sangiorgio, S. and Scielzo, N. D. and Sisti, M. and Smith, A. R. and Taffarello, L. and Tenconi, M. and Terranova, F. and Tian, W. D. and Tomei, C. and Trentalange, S. and Ventura, G. and Vignati, M. and Wang, B. S. and Wang, H. W. and Wielgus, L. and Wilson, J. and Winslow, L. A. and Wise, T. and Woodcraft, A. and Zanotti, L. and Zarra, C. and Zhu, B. X. and Zucchelli, S.},
abstractNote = {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.},
doi = {10.1016/j.phpro.2014.12.005},
journal = {Physics Procedia},
number = C,
volume = 61,
place = {United States},
year = {Thu Jan 01 00:00:00 EST 2015},
month = {Thu Jan 01 00:00:00 EST 2015}
}

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