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1. Progress in the development of a KITWPA for the DARTWARS project

Author

M. Borghesi, C. Barone, S. Capelli, G. Carapella, A.P. Caricato, I. Carusotto, A. Cian, D. Di Gioacchino, E. Enrico, P. Falferi, L. Fasolo, M. Faverzani, E. Ferri, G. Filatrella, C. Gatti, A. Giachero, D. Giubertoni, V. Granata, A. Greco, C. Guarcello, D. Labranca, A. Leo, C. Ligi, G. Maccarrone, F. Mantegazzini, B. Margesin, G. Maruccio, C. Mauro, R. Mezzena, A.G. Monteduro, A. Nucciotti, L. Oberto, L. Origo, S. Pagano, V. Pierro, L. Piersanti, M. Rajteri, A. Rettaroli, S. Rizzato, A. Vinante, M. Zannoni, Borghesi, M, Barone, C, Capelli, S, Carapella, G, Caricato, A, Carusotto, I, Cian, A, Di Gioacchino, D, Enrico, E, Falferi, P, Fasolo, L, Faverzani, M, Ferri, E, Filatrella, G, Gatti, C, Giachero, A, Giubertoni, D, Granata, V, Greco, A, Guarcello, C, Labranca, D, Leo, A, Ligi, C, Maccarrone, G, Mantegazzini, F, Margesin, B, Maruccio, G, Mauro, C, Mezzena, R, Monteduro, A, Nucciotti, A, Oberto, L, Origo, L, Pagano, S, Pierro, V, Piersanti, L, Rajteri, M, Rettaroli, A, Rizzato, S, Vinante, A, and Zannoni, M

Subjects
Superconductivity (cond-mat.supr-con), Nuclear and High Energy Physics, Quantum Physics, KITWPA, Condensed Matter - Superconductivity, Superconducting circuit, Parametric amplifier, Readout, Superconducting circuits, FOS: Physical sciences, Quantum Physics (quant-ph), Instrumentation
Abstract

DARTWARS (Detector Array Readout with Traveling Wave AmplifieRS) is a three years project that aims to develop high-performing innovative Traveling Wave Parametric Amplifiers (TWPAs) for low temperature detectors and qubit readout (C-band). The practical development follows two different promising approaches, one based on the Josephson junctions (TWJPA) and the other one based on the kinetic inductance of a high-resistivity superconductor (KITWPA). This paper presents the advancements made by the DARTWARS collaboration to produce a first working prototype of a KITWPA., 3 pages, 4 figures. Proceeding of Pisa15th Meeting conference

Published
2022

2. Detector Array Readout with Traveling Wave Amplifiers

Author

A. Giachero, C. Barone, M. Borghesi, G. Carapella, A. P. Caricato, I. Carusotto, W. Chang, A. Cian, D. Di Gioacchino, E. Enrico, P. Falferi, L. Fasolo, M. Faverzani, E. Ferri, G. Filatrella, C. Gatti, D. Giubertoni, A. Greco, C. Kutlu, A. Leo, C. Ligi, G. Maccarrone, B. Margesin, G. Maruccio, A. Matlashov, C. Mauro, R. Mezzena, A. G. Monteduro, A. Nucciotti, L. Oberto, S. Pagano, V. Pierro, L. Piersanti, M. Rajteri, S. Rizzato, Y. K. Semertzidis, S. Uchaikin, A. Vinante, Giachero, A., Barone, C., Borghesi, M., Carapella, G., Caricato, A. P., Carusotto, I., Chang, W., Cian, A., Di Gioacchino, D., Enrico, E., Falferi, P., Fasolo, L., Faverzani, M., Ferri, E., Filatrella, G., Gatti, C., Giubertoni, D., Greco, A., Kutlu, C., Leo, A., Ligi, C., Maccarrone, G., Margesin, B., Maruccio, Giuseppe, Matlashov, A., Mauro, C., Mezzena, R., Monteduro, A. G., Nucciotti, A., Oberto, L., Pagano, S., Pierro, V., Piersanti, L., Rajteri, M., Rizzato, S., Semertzidis, Y. K., Uchaikin, S., Vinante, A., Giachero, A, Barone, C, Borghesi, M, Carapella, G, Caricato, A, Carusotto, I, Chang, W, Cian, A, Gioacchino, D, Enrico, E, Falferi, P, Fasolo, L, Faverzani, M, Ferri, E, Filatrella, G, Gatti, C, Giubertoni, D, Greco, A, Kutlu, C, Leo, A, Ligi, C, Maccarrone, G, Margesin, B, Maruccio, G, Matlashov, A, Mauro, C, Mezzena, R, Monteduro, A, Nucciotti, A, Oberto, L, Pagano, S, Pierro, V, Piersanti, L, Rajteri, M, Rizzato, S, Semertzidis, Y, Uchaikin, S, and Vinante, A

Subjects
Quantum Physics, Quantum noise, Parametric amplifer, Traveling wave, Detector array read out, Qubits read out, Physics::Instrumentation and Detectors, Condensed Matter - Superconductivity, FOS: Physical sciences, Condensed Matter Physics, Parametric amplifier, Atomic and Molecular Physics, and Optics, Superconductivity (cond-mat.supr-con), General Materials Science, Quantum Physics (quant-ph), FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
Abstract

Reducing noise to the quantum limit over a large bandwidth is a fundamental requirement for future applications operating at millikelvin temperatures, such as the neutrino mass measurement, the next-generation X-ray observatory, the CMB measurement, the dark matter and axion detection, and the rapid high-fidelity readout of superconducting qubits. The read out sensitivity of arrays of microcalorimeter detectors, resonant axion-detectors, and qubits, is currently limited by the noise temperature and bandwidth of the cryogenic amplifiers. The Detector Array Readout with Traveling Wave Amplifiers project has the goal of developing high-performing innovative traveling wave parametric amplifiers with a high gain, a high saturation power, and a quantum-limited or nearly quantum-limited noise. The practical development follows two different promising approaches, one based on the Josephson junctions and the other one based on the kinetic inductance of a high-resistivity superconductor. In this contribution, we present the aims of the project, the adopted design solutions and preliminary results from simulations and measurements.

Published
2022

3. Ultra low noise readout with traveling wave parametric amplifiers: The DARTWARS project

Author

A. Rettaroli, C. Barone, M. Borghesi, S. Capelli, G. Carapella, A.P. Caricato, I. Carusotto, A. Cian, D. Di Gioacchino, E. Enrico, P. Falferi, L. Fasolo, M. Faverzani, E. Ferri, G. Filatrella, C. Gatti, A. Giachero, D. Giubertoni, V. Granata, A. Greco, C. Guarcello, D. Labranca, A. Leo, C. Ligi, G. Maccarrone, F. Mantegazzini, B. Margesin, G. Maruccio, C. Mauro, R. Mezzena, A.G. Monteduro, A. Nucciotti, L. Oberto, L. Origo, S. Pagano, V. Pierro, L. Piersanti, M. Rajteri, S. Rizzato, A. Vinante, M. Zannoni, Rettaroli, A, Barone, C, Borghesi, M, Capelli, S, Carapella, G, Caricato, A, Carusotto, I, Cian, A, Di Gioacchino, D, Enrico, E, Falferi, P, Fasolo, L, Faverzani, M, Ferri, E, Filatrella, G, Gatti, C, Giachero, A, Giubertoni, D, Granata, V, Greco, A, Guarcello, C, Labranca, D, Leo, A, Ligi, C, Maccarrone, G, Mantegazzini, F, Margesin, B, Maruccio, G, Mauro, C, Mezzena, R, Monteduro, A, Nucciotti, A, Oberto, L, Origo, L, Pagano, S, Pierro, V, Piersanti, L, Rajteri, M, Rizzato, S, Vinante, A, and Zannoni, M

Subjects
Quantum Physics, Nuclear and High Energy Physics, Josephson junctions, Microwaves, Low noise, Parametric amplification, Detector arrays, Superconductors, FOS: Physical sciences, Detector array, Josephson junction, Superconductor, Quantum Physics (quant-ph), Microwave, Instrumentation
Abstract

The DARTWARS project has the goal of developing high-performing innovative travelling wave parametric amplifiers with high gain, large bandwidth, high saturation power, and nearly quantum-limited noise. The target frequency region for its applications is 5 - 10 GHz, with an expected noise temperature of about 600 mK. The development follows two different approaches, one based on Josephson junctions and one based on kinetic inductance of superconductors. This contribution mainly focuses on the Josephson travelling wave parametric amplifier, presenting its design, preliminary measurements and the test of homogeneity of arrays of Josephson junctions., 4 pages, 5 figures. Proceeding of Pisa15th Meeting conference. arXiv admin note: text overlap with arXiv:2111.03409

Published
2023

4. Search for Majorana neutrinos exploiting millikelvin cryogenics with CUORE

Author

Adams, D. Q., Alduino, C., Alfonso, K., Avignone, F. T., Azzolini, O., Bari, G., Bellini, F., Benato, G., Beretta, M., Biassoni, M., Branca, A., Brofferio, C., Bucci, C., Camilleri, J., Caminata, A., Campani, A., Canonica, L., Cao, X. G., Capelli, S., Cappelli, L., Cardani, L., Carniti, P., Casali, N., Celi, E., Chiesa, D., Clemenza, M., Copello, S., Cremonesi, O., Creswick, R. J., D'Addabbo, A., Dafinei, I., Dell'Oro, S., Di Domizio, S., Dompe', V., Fang, D. Q., Fantini, G., Faverzani, M., Ferri, E., Ferroni, F., Fiorini, E., Franceschi, M. A., Freedman, S. J., Fu, S. H., Fujikawa, B. K., Giachero, A., Gironi, L., Giuliani, A., Gorla, P., Gotti, C., Gutierrez, T. D., Han, K., Hansen, E. V., Heeger, K. M., Huang, R. G., Huang, H. Z., Johnston, J., Keppel, G., Kolomensky, Yu. G., Ligi, C., Liu, R., Ma, L., Ma, Y. G., Marini, L., Maruyama, R. H., Mayer, D., Mei, Y., Moggi, N., Morganti, S., Napolitano, T., Nastasi, M., Nikkel, J., Nones, C., Norman, E. B., Nucciotti, A., Nutini, I., O'Donnell, T., Ouellet, J. L., Pagan, S., Pagliarone, C. E., Pagnanini, L., Pallavicini, M., Pattavina, L., Pavan, M., Pessina, G., Pettinacci, V., Pira, C., Pirro, S., Pozzi, S., Previtali, E., Puiu, A., Rosenfeld, C., Rusconi, C., Sakai, M., Sangiorgio, S., Schmidt, B., Scielzo, N. D., Sharma, V., Singh, V., Sisti, M., Speller, D., Surukuchi, P. T., Taffarello, L., Terranova, F., Tomei, C., Vetter, K. J., Vignati, M., Wagaarachchi, S. L., Wang, B. S., Welliver, B., Wilson, J., Wilson, K., Winslow, L. A., Zimmermann, S., Zucchelli, S., D. Q. Adam, C. Alduino, K. Alfonso, F. T. Avignone, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Beretta, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, L. Canonica, X. G. Cao, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, E. Celi, D. Chiesa, M. Clemenza, S. Copello, O. Cremonesi, R. J. Creswick, A. D???Addabbo, I. Dafinei, S. Dell???Oro, S. Di Domizio, V. Domp??, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, S. H. Fu, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, E. V. Hansen, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, R. Liu, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, D. Mayer, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. None, E. B. Norman, A. Nucciotti, I. Nutini, T. O???Donnell, J. L. Ouellet, S. Pagan, C. E. Pagliarone, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rosenfeld, C. Rusconi, M. Sakai, S. Sangiorgio, B. Schmidt, N. D. Scielzo, V. Sharma, V. Singh, M. Sisti, D. Speller, P. T. Surukuchi, L. Taffarello, F. Terranova, C. Tomei, K. J. Vetter, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, S. Zimmermann, S. Zucchelli, Adams, D, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Beretta, M, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Celi, E, Chiesa, D, Clemenza, M, Copello, S, Cremonesi, O, Creswick, R, D'Addabbo, A, Dafinei, I, Dell'Oro, S, Di Domizio, S, Dompe, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fu, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Hansen, E, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Liu, R, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mayer, D, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagan, S, Pagliarone, C, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rosenfeld, C, Rusconi, C, Sakai, M, Sangiorgio, S, Schmidt, B, Scielzo, N, Sharma, V, Singh, V, Sisti, M, Speller, D, Surukuchi, P, Taffarello, L, Terranova, F, Tomei, C, Vetter, K, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zimmermann, S, Zucchelli, S, Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, and CUORE

Subjects
tonne scale, cosmological model, data analysis method, LNGS, solid-state counter, neutrino-less double beta decay, Majorana neutrino, millikelvin, cryogenics, FOS: Physical sciences, double beta decay, Dirac Neutrino, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], nucl-ex, Neutrinoless Double Beta Decay, computer: quantum, dark matter, CUORE, Neutrinoless Double Beta Decay, LNGS, Neutrino, Majorana Neutrino, Dirac Neutrino, Particle Physics, energy: transition, double-beta decay: (0neutrino), bolometer, Neutrino, calorimeter, detector: calibration, Nuclear Physics - Experiment, Nuclear Experiment (nucl-ex), Particle Physics, Nuclear Experiment, neutrinoless, antimatter: asymmetry, leptogenesis, CUORE, Multidisciplinary, Neutrino physiscs. Majorana neutrino. Neutrinoless double beta decay. Cryogenic innovation and performance. CUORE experiment, particle: Majorana, double-beta decay, temperature, stability, tellurium: nuclide, matter: antimatter, Majorana
Abstract

The CUORE experiment finds no evidence for neutrinoless double beta decay after operating a large cryogenic TeO$_{2}$ calorimeter stably for several years in an extreme low-radiation environment at a temperature of 10 millikelvin. AbstractThe possibility that neutrinos may be their own antiparticles, unique among the known fundamental particles, arises from the symmetric theory of fermions proposed by Ettore Majorana in 19371. Given the profound consequences of such Majorana neutrinos, among which is a potential explanation for the matter–antimatter asymmetry of the universe via leptogenesis2, the Majorana nature of neutrinos commands intense experimental scrutiny globally; one of the primary experimental probes is neutrinoless double beta (0νββ) decay. Here we show results from the search for 0νββ decay of 130Te, using the latest advanced cryogenic calorimeters with the CUORE experiment3. CUORE, operating just 10 millikelvin above absolute zero, has pushed the state of the art on three frontiers: the sheer mass held at such ultralow temperatures, operational longevity, and the low levels of ionizing radiation emanating from the cryogenic infrastructure. We find no evidence for 0νββ decay and set a lower bound of the process half-life as 2.2 × 1025 years at a 90 per cent credibility interval. We discuss potential applications of the advances made with CUORE to other fields such as direct dark matter, neutrino and nuclear physics searches and large-scale quantum computing, which can benefit from sustained operation of large payloads in a low-radioactivity, ultralow-temperature cryogenic environment. The possibility that neutrinos may be their own antiparticles, unique among the known fundamental particles, arises from the symmetric theory of fermions proposed by Ettore Majorana in 1937. Given the profound consequences of such Majorana neutrinos, among which is a potential explanation for the matter-antimatter asymmetry of the universe via leptogenesis, the Majorana nature of neutrinos commands intense experimental scrutiny globally; one of the primary experimental probes is neutrinoless double beta ($0 \nu \beta \beta$) decay. Here we show results from the search for $0 \nu \beta \beta$ decay of $^{130}$Te, using the latest advanced cryogenic calorimeters with the CUORE experiment. CUORE, operating just 10 millikelvin above absolute zero, has pushed the state of the art on three frontiers: the sheer mass held at such ultra-low temperatures, operational longevity, and the low levels of ionising radiation emanating from the cryogenic infrastructure. We find no evidence for $0 \nu \beta \beta$ decay and set a lower bound of $T_{1/2}^{0 \nu} > 2.2 \times 10^{25}$ years at a 90% credibility interval. We discuss potential applications of the advances made with CUORE to other fields such as direct dark matter, neutrino and nuclear physics searches and large-scale quantum computing, which can benefit from sustained operation of large payloads in a low-radioactivity, ultra-low temperature cryogenic environment.

Published
2022

5. Exploring the neutrinoless double beta decay in the inverted neutrino hierarchy with bolometric detectors

Author

Oliviero Cremonesi, Carlo Ligi, J. Goett, T. I. Banks, M. Balata, M. Carrettoni, S. Trentalange, J. W. Beeman, Nicholas Scielzo, Ettore Fiorini, S. Zucchelli, Davide Chiesa, Massimiliano Clemenza, Marisa Pedretti, N. Casali, Andrea Giachero, N. Chott, P. Gorla, F. Ferroni, L. Wielgus, W. D. Tian, G. Piperno, Emanuele Ferri, Eugene E. Haller, L. Canonica, Xiangyu Cao, M. Pavan, Alan R. Smith, Ke Han, Reina H. Maruyama, Stuart J. Freedman, N. Moggi, Jonathan Ouellet, G. Bari, B. S. Wang, M. L. Di Vacri, L. Carbone, L. Pattavina, L. Taffarello, C. Pira, L. Zanotti, A. Bersani, T. Wise, A. De Biasi, Silvia Capelli, F. Orio, L. Gironi, Elena Sala, Y. Mei, X. Liu, F. T. Avignone, Claudio Gotti, M. Maino, V. Rampazzo, Eric B. Norman, Lindley Winslow, Yu G. Kolomensky, Ezio Previtali, H. Z. Huang, R. Hennings-Yeomans, G. Ventura, O. Azzolini, S. Pirro, Larissa M. Ejzak, B. X. Zhu, C. Cosmelli, I. Dafinei, M. Biassoni, S. Di Domizio, C. Zarra, K. M. Heeger, A. Woodcraft, C. Nones, T. O'Donnell, B. K. Fujikawa, M. I. Martínez, M. Tenconi, K. Kazkaz, M. M. Deninno, V. Palmieri, S. Morganti, R. W. Kadel, Francesca Bellini, S. Nisi, James R. Wilson, R. J. Creswick, T. D. Gutierrez, F. Terranova, M. Vignati, Yong-Ping Li, C. Rusconi, M. Faverzani, H. A. Farach, G. Keppel, D. R. Artusa, T. Napolitano, V. Pettinacci, A. Giuliani, C. Maiano, G. Fernandes, Monica Sisti, Hongwei Wang, L. Cardani, Vladimir Datskov, A. Dally, Yu-Gang Ma, C. Bucci, Deqing Fang, X. Z. Cai, Marco Pallavicini, Claudia Tomei, G. Pessina, C. Rosenfeld, C. Brofferio, Alejandro E. Camacho, Samuele Sangiorgio, A. Nucciotti, D. Orlandi, M. A. Franceschi, Artusa, D, Avignone, F, Azzolini, O, Balata, M, Banks, T, Bari, G, Beeman, J, Bellini, F, Bersani, A, Biassoni, M, Brofferio, C, Bucci, C, Cai, X, 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, Dafinei, I, Dally, A, Datskov, V, De Biasi, A, Deninno, M, Di Domizio, S, Di Vacri, M, Ejzak, L, Fang, D, Farach, H, Faverzani, M, Fernandes, G, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Goett, J, Gorla, P, Gotti, C, Gutierrez, T, Haller, E, Han, K, Heeger, K, Hennings Yeomans, R, Huang, H, Kadel, R, Kazkaz, K, Keppel, G, Kolomensky, Y, Li, Y, Ligi, C, Liu, X, Ma, Y, Maiano, C, Maino, M, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nisi, S, Nones, C, Norman, E, Nucciotti, A, O’Donnell, T, Orio, F, Orlandi, D, Ouellet, J, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pedretti, M, Pessina, G, Pettinacci, V, Piperno, G, Pira, C, Pirro, S, Previtali, E, Rampazzo, V, Rosenfeld, C, Rusconi, C, Sala, E, Sangiorgio, S, Scielzo, N, Sisti, M, Smith, A, Taffarello, L, Tenconi, M, Terranova, F, Tian, W, Tomei, C, Trentalange, S, Ventura, G, Vignati, M, Wang, B, Wang, H, Wielgus, L, Wilson, J, Winslow, L, Wise, T, Woodcraft, A, Zanotti, L, Zarra, C, Zhu, B, Zucchelli, S, D. R. Artusa, F. T. Avignone, O. Azzolini, M. Balata, T. I. Bank, 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, M. Clemenza, 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. Fernande, 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, T. D. Gutierrez, E. E. Haller, K. Han, K. M. Heeger, R. Hennings-Yeoman, 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. None, E. B. Norman, A. Nucciotti, T. O’Donnell, F. Orio, D. Orlandi, J. L. Ouellet, M. Pallavicini, V. Palmieri, L. Pattavina, M. 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. Wielgu, J. Wilson, L. A. Winslow, T. Wise, A. Woodcraft, L. Zanotti, C. Zarra, B. X. Zhu, and S. Zucchelli

Subjects
Particle physics, J.2, Physics - Instrumentation and Detectors, Experimental Physics, Physics and Astronomy (miscellaneous), Physics beyond the Standard Model, FOS: Physical sciences, 01 natural sciences, law.invention, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), CUORE, law, Double beta decay, 0103 physical sciences, Physics and Astronomy, Beta (velocity), neutrinole, Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment, Engineering (miscellaneous), Physics, 010308 nuclear & particles physics, Bolometer, bolometry, Instrumentation and Detectors (physics.ins-det), Beta decay, MAJORANA, DOUBLE-BETA DECAY, Neutrino
Abstract

Neutrinoless double beta decay (0nubb) is one of the most sensitive probes for physics beyond the Standard Model, providing unique information on the nature of neutrinos. In this paper we review the status and outlook for bolometric 0nubb decay searches. We summarize recent advances in background suppression demonstrated using bolometers with simultaneous readout of heat and light signals. We simulate several configurations of a future CUORE-like bolometer array which would utilize these improvements and present the sensitivity reach of a hypothetical next-generation bolometric 0nubb experiment. We demonstrate that a bolometric experiment with the isotope mass of about 1 ton is capable of reaching the sensitivity to the effective Majorana neutrino mass (|mee|) of order 10-20 meV, thus completely exploring the so-called inverted neutrino mass hierarchy region. We highlight the main challenges and identify priorities for an R&D program addressing them., 22 pages, 15 figures, submitted to EPJC

Published
2014

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

Author

V. Palmieri, F. Orio, K. M. Heeger, Kareem Kazkaz, B. X. Zhu, Eric B. Norman, Silvio Morganti, C. Maiano, Ettore Fiorini, T. Napolitano, B. S. Wang, T. I. Banks, L. Gironi, H. Z. Huang, O. Azzolini, C. Rosenfeld, C. Nones, Massimiliano Clemenza, Carlo Cosmelli, S. Zucchelli, D. Orlandi, P. Gorla, F. Ferroni, F. Rimondi, F. T. Avignone, Emanuele Ferri, W. D. Tian, Eugene E. Haller, M. P. Decowski, A. Bersani, M. Biassoni, M. L. Di Vacri, L. Kogler, M. A. Franceschi, R. Faccini, M. Maino, Claudio Gotti, T. Bloxham, Alan R. Smith, G. Bari, H. W. Wang, C. Brofferio, C. Bucci, T. D. Gutierrez, N. Chott, F. Alessandria, Oliviero Cremonesi, J. Goett, J. L. Ouellet, M. I. Martínez, M. Tenconi, S. Di Domizio, Larissa M. Ejzak, T. Wise, A. Dally, Marco Pallavicini, A. Giachero, C. Zarra, G. Pessina, X. Liu, Nicholas Scielzo, S. Newman, C. A. Whitten, M. Balata, F. Stivanello, L. Taffarello, V. Rampazzo, B. K. Fujikawa, L. Zanotti, N. Casali, L. Pattavina, Jeffrey W. Beeman, M. M. Deninno, N. Moggi, H. A. Farach, Lucia Canonica, Raffaele Ardito, Samuele Sangiorgio, Stefano Nisi, A. Nucciotti, F. Bellini, Ezio Previtali, M. Vignati, L. Carbone, Ioan Dafinei, R. J. Creswick, G. Ventura, Simone Capelli, R. W. Kadel, Yu. G. Kolomensky, Yong-Ping Li, Marisa Pedretti, G. Keppel, A. Woodcraft, M. Carrettoni, Ke Han, Reina H. Maruyama, Stuart J. Freedman, C. Rusconi, D. Lenz, Carlo Ligi, L. Cardani, Stefano Pirro, Vladimir Datskov, Yu-Gang Ma, A. De Biasi, Deqing Fang, X. Z. Cai, E. Guardincerri, A. Giuliani, S. Trentalange, M. Pavan, Claudia Tomei, D. R. Artusa, Monica Sisti, Alessandria, F, Ardito, R, Artusa, D, Avignone, F, Azzolini, O, Balata, M, Banks, T, Bari, G, Beeman, J, Bellini, F, Bersani, A, Biassoni, M, Bloxham, T, Brofferio, C, Bucci, C, Cai, X, Canonica, L, Capelli, S, Carbone, L, Cardani, L, Carrettoni, M, Casali, N, Chott, N, Clemenza, M, Cosmelli, C, Cremonesi, O, Creswick, R, Dafinei, I, Dally, A, Datskov, V, Biasi, A, Decowski, M, Deninno, M, Domizio, S, Vacri, M, Ejzak, L, Faccini, R, Fang, D, Farach, H, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Goett, J, Gorla, P, Gotti, C, Guardincerri, E, Gutierrez, T, Haller, E, Han, K, Heeger, K, Huang, H, Kadel, R, Kazkaz, K, Keppel, G, Kogler, L, Kolomensky, Y, Lenz, D, Li, Y, Ligi, C, Liu, X, Ma, Y, Maiano, C, Maino, M, Martinez, M, Maruyama, R, Moggi, N, Morganti, S, Napolitano, T, Newman, S, Nisi, S, Nones, C, Norman, E, Nucciotti, A, Orio, F, Orlandi, D, Ouellet, J, 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, N, Sisti, M, Smith, A, Stivanello, F, Taffarello, L, Tenconi, M, Tian, W, Tomei, C, Trentalange, S, Ventura, G, Vignati, M, Wang, B, Wang, H, Whitten, C, Wise, T, Woodcraft, A, Zanotti, L, Zarra, C, Zhu, B, Zucchelli, S, F Alessandria, R Ardito, D.R Artusa, F.T Avignone, O Azzolini, M Balata, T.I Bank, 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 None, 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, CSNSM PS1, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), GRAPPA (ITFA, IoP, FNWI), Faculty of Science, Other Research IHEF (IoP, FNWI), Gravitation and Astroparticle Physics Amsterdam, and IoP (FNWI)

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics - Instrumentation and Detectors, Dark matter, FOS: Physical sciences, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 01 natural sciences, RESPONSE STABILIZATION, Particle identification, Particle detector, Spectral line, law.invention, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), CUORE, WIMP, NUCLEAR-DATA SHEETS, law, SIGNALS, SEARCH, 0103 physical sciences, DETECTORS, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment (nucl-ex), dark matter experiments, dark matter detectors, 010306 general physics, Nuclear Experiment, CANDIDATES, Physics, dark matter detectors, 010308 nuclear & particles physics, dark matter experiments, Bolometer, CONSTRAINTS, Astronomy and Astrophysics, Instrumentation and Detectors (physics.ins-det), CUORICINO, 3. Good health, CONDUCTION, INTERACTING MASSIVE PARTICLES, Measuring instrument, wimp, FIS/04 - FISICA NUCLEARE E SUBNUCLEARE, Astrophysics - Cosmology and Nongalactic Astrophysics
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 CUORE0 (52 bolometers) and CUORE (988 bolometers) experiments to a WIMP annual modulation signal., 9 pages, 10 figures

Published
2013

7. Search for 14.4 keV solar axions from M1 transition of Fe-57 with Cuore crystals

Author

Alessandria, F, Ardito, R, Artusa, D, Avignone III, F, Azzolini, O, Balata, M, Banks, T, Bari, G, Beeman, J, Bellini, F, Bersani, A, BIASSONI, MATTEO, Bloxham, T, BROFFERIO, CHIARA, Bucci, C, Cai, X, Canonica, L, CAPELLI, SILVIA, Carbone, L, Cardani, L, Carrettoni, M, Casali, N, Chott, N, CLEMENZA, MASSIMILIANO, Cosmelli, C, Cremonesi, O, Creswick, R, Dafinei, I, Dally, A, Datskov, V, Biasi, A, Deninno, M, Di Domizio, S, Vacri, M, Ejzak, L, Faccini, R, Fang, D, Farach, H, FERRI, ELENA, Ferroni, F, FIORINI, ETTORE, Franceschi, M, Freedman, S, Fujikawa, B, t.e.x.t.b.f..u.n.d.e.r.l.i.n.e.{.A. Giachero}, n, GIRONI, LUCA, Giuliani, A, Goett, J, Goodsell, A, Gorla, P, GOTTI, CLAUDIO, Guardincerri, E, Gutierrez, T, Haller, E, Han, K, Heeger, K, Huang, H, Kadel, R, Kazkaz, K, Keppel, G, Kogler, L, Kolomensky, Y, Lenz, D, Li, Y, Ligi, C, Liu, X, Ma, Y, Maiano, C, MAINO, MATTEO, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Newman, S, Nisi, S, Nones, C, Norman, E, NUCCIOTTI, ANGELO ENRICO LODOVICO, Orio, F, Orlandi, D, Ouellet, J, Pallavicini, M, Palmieri, V, Pattavina, L, PAVAN, MAURA, Pedretti, M, Pessina, G, Pirro, S, Previtali, E, Rampazzo, V, Reil, R, Rimondi, F, Rosenfeld, C, Rusconi, C, Sangiorgio, S, Scielzo, N, SISTI, MONICA, Smith, A, Sparks, L, Stivanello, F, Taffarello, L, Tenconi, M, Tian, W, Tomei, C, Trentalange, S, Ventura, G, Vignati, M, Wang, B, Wang, H, Whitten J.r. , C, Wise, T, Woodcraft, A, ZANOTTI, LUIGI ERNESTO, Zarra, C, Zhu, B, Zucchelli, S., CSNSM PS1, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), F. Alessandria, R. Ardito, D. R. Artusa, F. T. Avignone III, O. Azzolini, M. Balata, T. I. Bank, 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. None, 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, L. Taffarello, M. Tenconi, W. D. Tian, C. Tomei, S. Trentalange, G. Ventura, M. Vignati, B. S. Wang, H. W. Wang, C. A. Whitten Jr., T. Wise, A. Woodcraft, L. Zanotti, C. Zarra, B. X. Zhu, S. Zucchelli, IoP (FNWI), Gravitation and Astroparticle Physics Amsterdam, GRAPPA (ITFA, IoP, FNWI), Faculty of Science, Other Research IHEF (IoP, FNWI), Alessandria, F, Ardito, R, Artusa, D, Avignone III, F, Azzolini, O, Balata, M, Banks, T, Bari, G, Beeman, J, Bellini, F, Bersani, A, Biassoni, M, Bloxham, T, Brofferio, C, Bucci, C, Cai, X, Canonica, L, Capelli, S, Carbone, L, Cardani, L, Carrettoni, M, Casali, N, Chott, N, Clemenza, M, Cosmelli, C, Cremonesi, O, Creswick, R, Dafinei, I, Dally, A, Datskov, V, Biasi, A, Deninno, M, Di Domizio, S, Vacri, M, Ejzak, L, Faccini, R, Fang, D, Farach, H, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, t. e. x. t. b. f. . u. n. d. e. r. l. i. n. e. {. A. Giachero}, N, Gironi, L, Giuliani, A, Goett, J, Goodsell, A, Gorla, P, Gotti, C, Guardincerri, E, Gutierrez, T, Haller, E, Han, K, Heeger, K, Huang, H, Kadel, R, Kazkaz, K, Keppel, G, Kogler, L, Kolomensky, Y, Lenz, D, Li, Y, Ligi, C, Liu, X, Ma, Y, Maiano, C, Maino, M, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Newman, S, Nisi, S, Nones, C, Norman, E, Nucciotti, A, Orio, F, Orlandi, D, Ouellet, J, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pedretti, M, Pessina, G, Pirro, S, Previtali, E, Rampazzo, V, Reil, R, Rimondi, F, Rosenfeld, C, Rusconi, C, Sangiorgio, S, Scielzo, N, Sisti, M, Smith, A, Sparks, L, Stivanello, F, Taffarello, L, Tenconi, M, Tian, W, Tomei, C, Trentalange, S, Ventura, G, Vignati, M, Wang, B, Wang, H, Whitten J. r., C, Wise, T, Woodcraft, A, Zanotti, L, Zarra, C, Zhu, B, and Zucchelli, S

Subjects
Particle physics, axions, dark matter experiment, FOS: Physical sciences, 01 natural sciences, High Energy Physics - Experiment, law.invention, Nuclear physics, High Energy Physics - Experiment (hep-ex), Experiment, dark matter experiments, CUORE, Low energy, law, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Matrix element, High Energy Physics, 010306 general physics, Pseudovector, Axion, Physics, 010308 nuclear & particles physics, Bolometer, Astronomy and Astrophysics, INVARIANCE, STRONG CP PROBLEM, solar axions
Abstract

We report the results of a search for axions from the 14.4 keV M1 transition from Fe-57 in the core of the sun using the axio-electric effect in TeO2 bolometers. The detectors are 5x5x5 cm3 crystals operated at about 10 mK in a facility used to test bolometers for the CUORE experiment at the Laboratori Nazionali del Gran Sasso in Italy. An analysis of 43.65 kg d of data was made using a newly developed low energy trigger which was optimized to reduce the detectors energy threshold. An upper limit of 0.63 c kg-1 d-1 was established at 95% C.L.. From this value, a lower bound at 95% C.L. was placed on the Peccei-Quinn energy scale of fa >= 0.76 10**6 GeV for a value of S=0.55 for the flavor-singlet axial vector matrix element. Bounds are given for the interval 0.15 < S < 0.55., 14 pages, 6 figures, submitted to JCAP

Published
2013

8. Validation of techniques to mitigate copper surface contamination in CUORE

Author

F. Orio, L. Taffarello, M. Carrettoni, B. S. Wang, Kareem Kazkaz, O. Azzolini, Ke Han, Reina H. Maruyama, C. Rosenfeld, Stuart J. Freedman, A. Woodcraft, H. A. Farach, P. Gorla, A. Giuliani, F. Ferroni, V. Palmieri, Emanuele Ferri, Eugene E. Haller, M. M. Deninno, D. Orlandi, Y. L. Li, Ettore Fiorini, Eric B. Norman, A. Bersani, Massimiliano Clemenza, M. A. Franceschi, L. Canonica, Silvio Morganti, T. Napolitano, L. Kogler, N. Moggi, N. Chott, A. Giachero, G. Bari, Larissa M. Ejzak, M. Maino, Samuele Sangiorgio, Stefano Nisi, F. Bellini, W. D. Tian, H. W. Wang, C. Cosmelli, M. Biassoni, F. Stivanello, L. Zanotti, Y. Mei, Deqing Fang, A. Nucciotti, Claudio Gotti, X. Z. Cai, Marisa Pedretti, Simone Capelli, R. W. Kadel, C. Bucci, T. D. Gutierrez, T. Bloxham, M. L. Di Vacri, Raffaele Ardito, C. Brofferio, R. J. Creswick, S. Pirro, Oliviero Cremonesi, C. Maiano, K. M. Heeger, A. Goodsell, J. Goett, L. Carbone, Ezio Previtali, Marco Pallavicini, L. Gironi, F. T. Avignone, G. Pessina, G. Ventura, M. Balata, H. Z. Huang, Yu. G. Kolomensky, Franco Rimondi, S. Zucchelli, Nicholas Scielzo, J. L. Ouellet, R. Faccini, N. Casali, C. Nones, E. Guardincerri, X. Liu, Ioan Dafinei, Jeffrey W. Beeman, S. Newman, V. Rampazzo, L. Pattavina, F. Alessandria, M. I. Martínez, M. Tenconi, B. X. Zhu, Carlo Ligi, M. Pavan, Vladimir Datskov, S. Di Domizio, Yu-Gang Ma, C. Zarra, B. K. Fujikawa, M. Vignati, A. De Biasi, T. I. Banks, A. Dally, Claudia Tomei, Alan R. Smith, S. Trentalange, G. Keppel, D. R. Artusa, Monica Sisti, L. Cardani, C. A. Whitten, L. Sparks, R. Reil, C. Rusconi, D. Lenz, T. Wise, CSNSM PS1, Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre Interdisciplinaire de Nanoscience de Marseille (CINaM), Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS), DAM Île-de-France (DAM/DIF), Direction des Applications Militaires (DAM), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), F. Alessandria, R. Ardito, D.R. Artusa, F.T. Avignone III, O. Azzolini, M. Balata, T.I. Bank, 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.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, A. Goodsell, 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, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, S. Newman, S. Nisi, C. None, 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, R. Reil, F. Rimondi, C. Rosenfeld, C. Rusconi, S. Sangiorgio, N.D. Scielzo, M. Sisti, A.R. Smith, L. Spark, 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 Jr, T. Wise, A. Woodcraft, L. Zanotti, C. Zarra, B.X. Zhu, S. Zucchelli, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Aix Marseille Université (AMU), Alessandria, F, Ardito, R, Artusa, D, Avignone III, F, Azzolini, O, Balata, M, Banks, T, Bari, G, Beeman, J, Bellini, F, Bersani, A, Biassoni, M, Bloxham, T, Brofferio, C, Bucci, C, Cai, X, Canonica, L, Capelli, S, Carbone, L, Cardani, L, Carrettoni, M, Casali, N, Chott, N, Clemenza, M, Cosmelli, C, Cremonesi, O, Creswick, R, Dafinei, I, Dally, A, Datskov, V, De Biasi, A, Deninno, M, Di Domizio, S, di Vacri, M, Ejzak, L, Faccini, R, Fang, D, Farach, H, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Goett, J, Goodsell, A, Gorla, P, Gotti, C, Guardincerri, E, Gutierrez, T, Haller, E, Han, K, Heeger, K, Huang, H, Kadel, R, Kazkaz, K, Keppel, G, Kogler, L, Kolomensky, Y, Lenz, D, Li, Y, Ligi, C, Liu, X, Ma, Y, Maiano, C, Maino, M, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Newman, S, Nisi, S, Nones, C, Norman, E, Nucciotti, A, Orio, F, Orlandi, D, Ouellet, J, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pedretti, M, Pessina, G, Pirro, S, Previtali, E, Rampazzo, V, Reil, R, Rimondi, F, Rosenfeld, C, Rusconi, C, Sangiorgio, S, Scielzo, N, Sisti, M, Smith, A, Sparks, L, Stivanello, F, Taffarello, L, Tenconi, M, Tian, W, Tomei, C, Trentalange, S, Ventura, G, Vignati, M, Wang, B, Wang, H, Whitten Jr, C, Wise, T, Woodcraft, A, Zanotti, L, Zarra, C, Zhu, B, and Zucchelli, S

Subjects
Physics - Instrumentation and Detectors, Nuclear engineering, bolometer, neutrinoless double beta decay, radioactive background, surface contamination, FOS: Physical sciences, chemistry.chemical_element, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 01 natural sciences, Bolometer, Neutrinoless Double Beta Decay, Surface contamination, Radioactive background, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), CUORE, 0103 physical sciences, Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment, Physics, 010308 nuclear & particles physics, Detector, Astronomy and Astrophysics, Instrumentation and Detectors (physics.ins-det), Contamination, Copper, NEUTRINOS, FIS/01 - FISICA SPERIMENTALE, RARE EVENTS, chemistry, DOUBLE-BETA DECAY, FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
Abstract

In this article we describe the background challenges for the CUORE experiment posed by surface contamination of inert detector materials such as copper, and present three techniques explored to mitigate these backgrounds. Using data from a dedicated test apparatus constructed to validate and compare these techniques we demonstrate that copper surface contamination levels better than 10E-07 - 10E-08 Bq/cm2 are achieved for 238U and 232Th. If these levels are reproduced in the final CUORE apparatus the projected 90% C.L. upper limit on the number of background counts in the region of interest is 0.02-0.03 counts/keV/kg/y depending on the adopted mitigation technique., 10 pages, 6 figures, 6 tables

Published
2013

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