Low energy analysis techniques for CUORE
Creators
- Alduino, C.1
- Avignone, F.T.1
- Chott, N.1
- Creswick, R.J.1
- Rosenfeld, C.1
- Wilson, J.1
- Alfonso, K.2
- Huang, H.Z.2
- Sakai, M.2
- Schmidt, J.2
- Artusa, D.R.3, 1
- Rusconi, C.3, 1
- Azzolini, O.4
- Camacho, A.4
- Keppel, G.4
- Palmieri, V.4
- Pira, C.4
- Bari, G.5
- Deninno, M.M.5
- Beeman, J.W.6
- Bellini, F.7, 8
- Cosmelli, C.7, 8
- Ferroni, F.7, 8
- Piperno, G.7, 8
- Benato, G.9
- Singh, V.9
- Bersani, A.10
- Caminata, A.10
- Biassoni, M.11, 12
- Brofferio, C.11, 12
- Capelli, S.11, 12
- Carniti, P.11, 12
- Cassina, L.11, 12
- Chiesa, D.11, 12
- Clemenza, M.11, 12
- Faverzani, M.11, 12
- Fiorini, E.11, 12
- Gironi, L.11, 12
- Gotti, C.11, 12
- Maino, M.11, 12
- Nastasi, M.11, 12
- Nucciotti, A.11, 12
- Pavan, M.11, 12
- Pozzi, S.11, 12
- Sisti, M.11, 12
- Terranova, F.11, 12
- Zanotti, L.11, 12
- Branca, A.13
- Taffarello, L.13
- Bucci, C.3
- Cappelli, L.3
- D'Addabbo, A.3
- Gorla, P.3
- Pattavina, L.3
- Pirro, S.3
- Canonica, L.14, 3
- Cao, X.G.15
- Fang, D.Q.15
- Ma, Y.G.15
- Wang, H.W.15
- Zhang, G.Q.15
- Cardani, L.7
- Casali, N.7
- Dafinei, I.7
- Morganti, S.7
- Mosteiro, P.J.7
- Tomei, C.7
- Vignati, M.7
- Copello, S.16, 10
- Di Domizio, S.16, 10
- Marini, L.16, 10
- Pallavicini, M.16, 10
- Cremonesi, O.11
- Ferri, E.11
- Giachero, A.11
- Pessina, G.11
- Previtali, E.11
- Cushman, J.S.17
- Davis, C.J.17
- Heeger, K.M.17
- Lim, K.E.17
- Maruyama, R.H.17
- D'Aguanno, D.18, 3
- Pagliarone, C.E.18, 3
- Dell'Oro, S.19, 3
- Di Vacri, M.L.20, 3
- Santone, D.20, 3
- Drobizhev, A.21, 9
- Hennings-Yeomans, R.21, 9
- Kolomensky, Yu.G.21, 9
- Wagaarachchi, S.L.21, 9
- Franceschi, M.A.22
- Ligi, C.22
- Napolitano, T.22
- Freedman, S.J.21, 9
- Fujikawa, B.K.21
- Mei, Y.21
- Schmidt, B.21
- Smith, A.R.21
- Welliver, B.21
- Giuliani, A.23
- Novati, V.23
- Gladstone, L.14
- Leder, A.14
- Ouellet, J.L.14
- Winslow, L.A.14
- Gutierrez, T.D.24
- Haller, E.E.25, 6
- Han, K.26
- Hansen, E.14, 2
- Kadel, R.27
- Martinez, M.28, 7, 8
- Moggi, N.29, 5
- Zucchelli, S.29, 5
- Nones, C.30
- Norman, E.B.31, 32
- Wang, B.S.31, 32
- O'Donnell, T.33
- Sangiorgio, S.32
- Scielzo, N.D.32
- Wise, T.34, 35
- Woodcraft, A.36
- Zimmermann, S.37
- 1. University of South Carolina, Department of Physics and Astronomy, Columbia, SC (United States)
- 2. University of California, Department of Physics and Astronomy, Los Angeles, CA (United States)
- 3. INFN-Laboratori Nazionali del Gran Sasso, L'Aquila (Italy)
- 4. INFN-Laboratori Nazionali di Legnaro, Padua (Italy)
- 5. INFN-Sezione di Bologna, Bologna (Italy)
- 6. Lawrence Berkeley National Laboratory, Materials Science Division, Berkeley, CA (United States)
- 7. INFN-Sezione di Roma, Rome (Italy)
- 8. Sapienza Universita di Roma, Dipartimento di Fisica, Rome (Italy)
- 9. University of California, Department of Physics, Berkeley, CA (United States)
- 10. INFN-Sezione di Genova, Genoa (Italy)
- 11. INFN-Sezione di Milano Bicocca, Milan (Italy)
- 12. Universita di Milano-Bicocca, Dipartimento di Fisica, Milan (Italy)
- 13. INFN-Sezione di Padova, Padua (Italy)
- 14. Massachusetts Institute of Technology, Cambridge, MA (United States)
- 15. Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai (China)
- 16. Universita di Genova, Dipartimento di Fisica, Genoa (Italy)
- 17. Yale University, Department of Physics, New Haven, CT (United States)
- 18. Universita degli Studi di Cassino e del Lazio Meridionale, Dipartimento di Ingegneria Civile e Meccanica, Cassino (Italy)
- 19. INFN-Gran Sasso Science Institute, L'Aquila (Italy)
- 20. Universita dell'Aquila, Dipartimento di Scienze Fisiche e Chimiche, L'Aquila (Italy)
- 21. Lawrence Berkeley National Laboratory, Nuclear Science Division, Berkeley, CA (United States)
- 22. INFN-Laboratori Nazionali di Frascati, Rome (Italy)
- 23. Universite Paris-Saclay, CSNSM, Univ. Paris-Sud, CNRS/IN2P3, Orsay (France)
- 24. California Polytechnic State University, Physics Department, San Luis Obispo, CA (United States)
- 25. University of California, Department of Materials Science and Engineering, Berkeley, CA (United States)
- 26. Shanghai Jiao Tong University, Department of Physics and Astronomy, Shanghai (China)
- 27. Lawrence Berkeley National Laboratory, Physics Division, Berkeley, CA (United States)
- 28. Universidad de Zaragoza, Laboratorio de Fisica Nuclear y Astroparticulas, Saragossa (Spain)
- 29. Universita di Bologna - Alma Mater Studiorum, Dipartimento di Fisica e Astronomia, Bologna (IT)
- 30. CEA/Saclay, Service de Physique des Particules, Gif-sur-Yvette (FR)
- 31. University of California, Department of Nuclear Engineering, Berkeley, CA (US)
- 32. Lawrence Livermore National Laboratory, Livermore, CA (US)
- 33. Virginia Polytechnic Institute and State University, Center for Neutrino Physics, Blacksburg, VA (US)
- 34. University of Wisconsin, Department of Physics, Madison, WI (US)
- 35. Yale University, Department of Physics, New Haven, CT (US)
- 36. University of Edinburgh, SUPA, Institute for Astronomy, Edinburgh (GB)
- 37. Lawrence Berkeley National Laboratory, Engineering Division, Berkeley, CA (US)
Description
CUORE is a tonne-scale cryogenic detector operating at the Laboratori Nazionali del Gran Sasso (LNGS) that uses tellurium dioxide bolometers to search for neutrinoless double-beta decay of 130Te. CUORE is also suitable to search for low energy rare events such as solar axions or WIMP scattering, thanks to its ultra-low background and large target mass. However, to conduct such sensitive searches requires improving the energy threshold to 10 keV. In this paper, we describe the analysis techniques developed for the low energy analysis of CUORE-like detectors, using the data acquired from November 2013 to March 2015 by CUORE-0, a single-tower prototype designed to validate the assembly procedure and new cleaning techniques of CUORE. We explain the energy threshold optimization, continuous monitoring of the trigger efficiency, data and event selection, and energy calibration at low energies in detail. We also present the low energy background spectrum of CUORE-0 below 60 keV. Finally, we report the sensitivity of CUORE to WIMP annual modulation using the CUORE-0 energy threshold and background, as well as an estimate of the uncertainty on the nuclear quenching factor from nuclear recoils in CUORE-0. (orig.)
Availability note (English)
Available from: http://dx.doi.org/10.1140/epjc/s10052-017-5433-1Additional details
Identifiers
Publishing Information
- Journal Title
- European Physical Journal. C, Particles and Fields (Online)
- Journal Volume
- 77
- Journal Issue
- 12
- Journal Page Range
- p. 1-11
- ISSN
- 1434-6052
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- Germany
- INIS RN
- 49021032
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Descriptors DEI
- ANNUAL VARIATIONS; BACKGROUND RADIATION; BETA DETECTION; BOLOMETERS; CALIBRATION; CRYOGENICS; DATA PROCESSING; EFFICIENCY; ENERGY SPECTRA; KEV RANGE 10-100; LOW LEVEL COUNTERS; MONITORING; NEUTRINOLESS DOUBLE BETA DECAY; OPTIMIZATION; PARTICLE DISCRIMINATION; SENSITIVITY; TELLURIUM 130; TELLURIUM OXIDES; UNDERGROUND; WIMPS
- Descriptors DEC
- BETA DECAY; BETA-MINUS DECAY; CHALCOGENIDES; CHARGED PARTICLE DETECTION; DECAY; DETECTION; DOUBLE BETA DECAY; ELEMENTARY PARTICLES; ENERGY RANGE; EVEN-EVEN NUCLEI; INTERMEDIATE MASS NUCLEI; ISOTOPES; KEV RANGE; LEVELS; MEASURING INSTRUMENTS; NUCLEAR DECAY; NUCLEI; OXIDES; OXYGEN COMPOUNDS; PARTICLE IDENTIFICATION; POSTULATED PARTICLES; PROCESSING; RADIATION DETECTION; RADIATION DETECTORS; RADIATIONS; SPECTRA; STABLE ISOTOPES; TELLURIUM COMPOUNDS; TELLURIUM ISOTOPES; VARIATIONS