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131 results on '"M. Clemenza"'

1. Temporal markers in a temperate ice core: insights from 3H and 137Cs profiles from the Adamello Glacier

Author: E. Di Stefano, G. Baccolo, M. Clemenza, B. Delmonte, D. Fiorini, R. Garzonio, M. Schwikowski, and V. Maggi
Subjects: Environmental sciences, GE1-350, Geology, QE1-996.5
Abstract: The article discusses the use of tritium (3H) and cesium (137Cs) as temporal markers in ice cores extracted from temperate glaciers. We present a complete tritium profile for a 46 m ice core drilled from the Adamello Glacier, a temperate glacier in the Italian Alps, and compare it to the 137Cs profile from the same ice core. Our analysis reveals tritium contamination between 19 and 32 m of depth, which can be attributed to the global radioactive fallout caused by atmospheric nuclear-bomb testing that took place in the 1950s and 1960s. Results show that the radioactive peak associated with 1963 does not occur at the same depth for both 3H and 137Cs; instead, the tritium peak is 1.5 m above the cesium one. Our hypothesis is that this misalignment is caused by meltwater-induced post-depositional processes that affect 137Cs, which is more sensitive to percolation than 3H. The total inventory of 137Cs in this ice core is also among the lowest ever reported, providing additional evidence that the presence of meltwater has affected the distribution of this radionuclide within the ice. In contrast, the total tritium inventory is comparable to what is reported in the literature, making it a more reliable temporal marker for temperate glaciers.
Published: 2024
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2. Optimization of the first CUPID detector module

Author: CUPID Collaboration, K. Alfonso, A. Armatol, C. Augier, F. T. Avignone, O. Azzolini, M. Balata, A. S. Barabash, G. Bari, A. Barresi, D. Baudin, F. Bellini, G. Benato, M. Beretta, M. Bettelli, M. Biassoni, J. Billard, V. Boldrini, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, A. Campani, C. Capelli, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, E. Celi, C. Chang, D. Chiesa, M. Clemenza, I. Colantoni, S. Copello, E. Craft, O. Cremonesi, R. J. Creswick, A. Cruciani, A. D’Addabbo, G. D’Imperio, S. Dabagov, I. Dafinei, F. A. Danevich, M. De Jesus, P. de Marcillac, S. Dell’Oro, S. Di Domizio, S. Di Lorenzo, T. Dixon, V. Dompè, A. Drobizhev, L. Dumoulin, G. Fantini, M. Faverzani, E. Ferri, F. Ferri, F. Ferroni, E. Figueroa-Feliciano, L. Foggetta, J. Formaggio, A. Franceschi, C. Fu, S. Fu, B. K. Fujikawa, A. Gallas, J. Gascon, S. Ghislandi, A. Giachero, A. Gianvecchio, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, C. Grant, P. Gras, P. V. Guillaumon, T. D. Gutierrez, K. Han, E. V. Hansen, K. M. Heeger, D. L. Helis, H. Z. Huang, L. Imbert, J. Johnston, A. Juillard, G. Karapetrov, G. Keppel, H. Khalife, V. V. Kobychev, Yu. G. Kolomensky, S. I. Konovalov, R. Kowalski, T. Langford, M. Lefevre, R. Liu, Y. Liu, P. Loaiza, L. Ma, M. Madhukuttan, F. Mancarella, L. Marini, S. Marnieros, M. Martinez, R. H. Maruyama, Ph. Mas, B. Mauri, D. Mayer, G. Mazzitelli, Y. Mei, S. Milana, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, S. Nisi, C. Nones, E. B. Norman, V. Novosad, I. Nutini, T. O’Donnell, E. Olivieri, M. Olmi, J. L. Ouellet, S. Pagan, C. Pagliarone, L. Pagnanini, L. Pattavina, M. Pavan, H. Peng, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, D. V. Poda, O. G. Polischuk, I. Ponce, S. Pozzi, E. Previtali, A. Puiu, S. Quitadamo, A. Ressa, R. Rizzoli, C. Rosenfeld, P. Rosier, J. Scarpaci, B. Schmidt, V. Sharma, V. N. Shlegel, V. Singh, M. Sisti, P. Slocum, D. Speller, P. T. Surukuchi, L. Taffarello, C. Tomei, J. A. Torres, V. I. Tretyak, A. Tsymbaliuk, M. Velazquez, K. J. Vetter, S. L. Wagaarachchi, G. Wang, L. Wang, R. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, M. Xue, L. Yan, J. Yang, V. Yefremenko, V. I. Umatov, M. M. Zarytskyy, J. Zhang, A. Zolotarova, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract CUPID will be a next generation experiment searching for the neutrinoless double $$\beta $$ β decay, whose discovery would establish the Majorana nature of the neutrino. Based on the experience achieved with the CUORE experiment, presently taking data at LNGS, CUPID aims to reach a background free environment by means of scintillating Li $$_{2}$$ 2 $$^{100}$$ 100 MoO $$_4$$ 4 crystals coupled to light detectors. Indeed, the simultaneous heat and light detection allows us to reject the dominant background of $$\alpha $$ α particles, as proven by the CUPID-0 and CUPID-Mo demonstrators. In this work we present the results of the first test of the CUPID baseline module. In particular, we propose a new optimized detector structure and light sensors design to enhance the engineering and the light collection, respectively. We characterized the heat detectors, achieving an energy resolution of (5.9 ± 0.2) keV FWHM at the Q-value of $$^{100}$$ 100 Mo (about 3034 keV). We studied the light collection of the baseline CUPID design with respect to an alternative configuration which features gravity-assisted light detectors’ mounting. In both cases we obtained an improvement in the light collection with respect to past measures and we validated the particle identification capability of the detector, which ensures an $$\alpha $$ α particle rejection higher than 99.9%, fully satisfying the requirements for CUPID.
Published: 2022
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3. Radiopurity of a kg-scale PbWO $$_4$$ 4 cryogenic detector produced from archaeological Pb for the RES-NOVA experiment

Author: The RES-NOVA Group of Interest, J. W. Beeman, G. Benato, C. Bucci, L. Canonica, P. Carniti, E. Celi, M. Clemenza, A. D’Addabbo, F. A. Danevich, S. Di Domizio, S. DiLorenzo, O. M. Dubovik, N. Ferreiro Iachellini, F. Ferroni, E. Fiorini, S. Fu, A. Garai, S. Ghislandi, L. Gironi, P. Gorla, C. Gotti, P. V. Guillaumon, D. L. Helis, G. P. Kovtun, M. Mancuso, L. Marini, M. Olmi, L. Pagnanini, L. Pattavina, G. Pessina, F. Petricca, S. Pirro, S. Pozzi, A. Puiu, S. Quitadamo, J. Rothe, A. P. Scherban, S. Schönert, D. A. Solopikhin, R. Strauss, E. Tarabini, V. I. Tretyak, I. A. Tupitsyna, and V. Wagner
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract RES-NOVA is a newly proposed experiment for detecting neutrinos from astrophysical sources, mainly Supernovae, using an array of cryogenic detectors made of PbWO $$_4$$ 4 crystals produced from archaeological Pb. This unconventional material, characterized by intrinsic high radiopurity, enables low-background levels in the region of interest for the neutrino detection via Coherent Elastic neutrino-Nucleus Scattering (CE $$\nu $$ ν NS). This signal lies at the detector energy threshold, O(1 keV), and it is expected to be hidden by naturally occurring radioactive contaminants of the crystal absorber. Here, we present the results of a radiopurity assay on a 0.84 kg PbWO $$_4$$ 4 crystal produced from archaeological Pb operated as a cryogenic detector. The crystal internal radioactive contaminations are: $$^{232}$$ 232 Th
Published: 2022
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4. Background identification in cryogenic calorimeters through $$\alpha -\alpha $$ α - α delayed coincidences

Author: O. Azzolini, J. W. Beeman, F. Bellini, M. Beretta, M. Biassoni, C. Brofferio, C. Bucci, S. Capelli, L. Cardani, P. Carniti, N. Casali, D. Chiesa, M. Clemenza, O. Cremonesi, A. Cruciani, I. Dafinei, A. D’Addabbo, S. Di Domizio, F. Ferroni, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, G. Keppel, M. Martinez, S. Nagorny, M. Nastasi, S. Nisi, C. Nones, D. Orlandi, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rusconi, K. Schäffner, C. Tomei, M. Vignati, and A. Zolotarova
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract Localization and modeling of radioactive contaminations is a challenge that ultra-low background experiments are constantly facing. These are fundamental steps both to extract scientific results and to further reduce the background of the detectors. Here we present an innovative technique based on the analysis of $$\alpha -\alpha $$ α - α delayed coincidences in $${}^{232}$$ 232 Th and $${}^{238}$$ 238 U decay chains, developed to investigate the contaminations of the ZnSe crystals in the CUPID-0 experiment. This method allows to disentangle surface and bulk contaminations of the detectors relying on the different probability to tag delayed coincidences as function of the $$\alpha $$ α decay position.
Published: 2021
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5. Search for double-beta decay of $$\mathrm {^{130}Te}$$ 130 Te to the $$0^+$$ 0 + states of $$\mathrm {^{130}Xe}$$ 130 Xe with CUORE

Author: D. Q. Adams, C. Alduino, K. Alfonso, F. T. III Avignone, O. Azzolini, G. Bari, F. Bellini, G. Benato, 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, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D’Addabbo, I. Dafinei, C. J. Davis, S. Dell’Oro, S. Di Domizio, V. Dompè, 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, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, 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. Nones, 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, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The CUORE experiment is a large bolometric array searching for the lepton number violating neutrino-less double beta decay ( $$0\nu \beta \beta $$ 0 ν β β ) in the isotope $$\mathrm {^{130}Te}$$ 130 Te . In this work we present the latest results on two searches for the double beta decay (DBD) of $$\mathrm {^{130}Te}$$ 130 Te to the first $$0^{+}_2$$ 0 2 + excited state of $$\mathrm {^{130}Xe}$$ 130 Xe : the $$0\nu \beta \beta $$ 0 ν β β decay and the Standard Model-allowed two-neutrinos double beta decay ( $$2\nu \beta \beta $$ 2 ν β β ). Both searches are based on a 372.5 kg $$\times $$ × yr TeO $$_2$$ 2 exposure. The de-excitation gamma rays emitted by the excited Xe nucleus in the final state yield a unique signature, which can be searched for with low background by studying coincident events in two or more bolometers. The closely packed arrangement of the CUORE crystals constitutes a significant advantage in this regard. The median limit setting sensitivities at 90% Credible Interval (C.I.) of the given searches were estimated as $$\mathrm {S^{0\nu }_{1/2} = 5.6 \times 10^{24} \, \mathrm {yr}}$$ S 1 / 2 0 ν = 5.6 × 10 24 yr for the $${0\nu \beta \beta }$$ 0 ν β β decay and $$\mathrm {S^{2\nu }_{1/2} = 2.1 \times 10^{24} \, \mathrm {yr}}$$ S 1 / 2 2 ν = 2.1 × 10 24 yr for the $${2\nu \beta \beta }$$ 2 ν β β decay. No significant evidence for either of the decay modes was observed and a Bayesian lower bound at $$90\%$$ 90 % C.I. on the decay half lives is obtained as: $$\mathrm {(T_{1/2})^{0\nu }_{0^+_2} > 5.9 \times 10^{24} \, \mathrm {yr}}$$ ( T 1 / 2 ) 0 2 + 0 ν > 5.9 × 10 24 yr for the $$0\nu \beta \beta $$ 0 ν β β mode and $$\mathrm {(T_{1/2})^{2\nu }_{0^+_2} > 1.3 \times 10^{24} \, \mathrm {yr}}$$ ( T 1 / 2 ) 0 2 + 2 ν > 1.3 × 10 24 yr for the $$2\nu \beta \beta $$ 2 ν β β mode. These represent the most stringent limits on the DBD of $$^{130}$$ 130 Te to excited states and improve by a factor $$\sim 5$$ ∼ 5 the previous results on this process.
Published: 2021
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6. Reducing the impact of radioactivity on quantum circuits in a deep-underground facility

Author: L. Cardani, F. Valenti, N. Casali, G. Catelani, T. Charpentier, M. Clemenza, I. Colantoni, A. Cruciani, G. D’Imperio, L. Gironi, L. Grünhaupt, D. Gusenkova, F. Henriques, M. Lagoin, M. Martinez, G. Pettinari, C. Rusconi, O. Sander, C. Tomei, A. V. Ustinov, M. Weber, W. Wernsdorfer, M. Vignati, S. Pirro, and I. M. Pop
Subjects: Science
Abstract: Background radiation has been identified as a key factor limiting the coherence times of superconducting circuits. Here, the authors measure the impact of environmental and cosmic radiation on a superconducting resonator with varying degrees of shielding, including an underground facility.
Published: 2021
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7. Characterization of cubic Li $$_{2}$$ 2 $$^{100}$$ 100 MoO $$_4$$ 4 crystals for the CUPID experiment

Author: The CUPID Collaboration, A. Armatol, E. Armengaud, W. Armstrong, C. Augier, F. T. Avignone, O. Azzolini, A. Barabash, G. Bari, A. Barresi, D. Baudin, F. Bellini, G. Benato, M. Beretta, L. Bergé, M. Biassoni, J. Billard, V. Boldrini, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, A. Cazes, E. Celi, C. Chang, M. Chapellier, A. Charrier, D. Chiesa, M. Clemenza, I. Colantoni, F. Collamati, S. Copello, O. Cremonesi, R. J. Creswick, A. Cruciani, A. D’Addabbo, G. D’Imperio, I. Dafinei, F. A. Danevich, M. de Combarieu, M. De Jesus, P. de Marcillac, S. Dell’Oro, S. Di Domizio, V. Dompè, A. Drobizhev, L. Dumoulin, G. Fantini, M. Faverzani, E. Ferri, F. Ferri, F. Ferroni, E. Figueroa-Feliciano, J. Formaggio, A. Franceschi, C. Fu, S. Fu, B. K. Fujikawa, J. Gascon, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, P. Gras, M. Gros, T. D. Gutierrez, K. Han, E. V. Hansen, K. M. Heeger, D. L. Helis, H. Z. Huang, R. G. Huang, L. Imbert, J. Johnston, A. Juillard, G. Karapetrov, G. Keppel, H. Khalife, V. V. Kobychev, Yu. G. Kolomensky, S. Konovalov, Y. Liu, P. Loaiza, L. Ma, M. Madhukuttan, F. Mancarella, R. Mariam, L. Marini, S. Marnieros, M. Martinez, R. H. Maruyama, B. Mauri, D. Mayer, Y. Mei, S. Milana, D. Misiak, T. Napolitano, M. Nastasi, X. F. Navick, J. Nikkel, R. Nipoti, S. Nisi, C. Nones, E. B. Norman, V. Novosad, I. Nutini, T. O’Donnell, E. Olivieri, C. Oriol, J. L. Ouellet, S. Pagan, C. Pagliarone, L. Pagnanini, P. Pari, L. Pattavina, B. Paul, M. Pavan, H. Peng, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, D. V. Poda, T. Polakovic, O. G. Polischuk, S. Pozzi, E. Previtali, A. Puiu, A. Ressa, R. Rizzoli, C. Rosenfeld, C. Rusconi, V. Sanglard, J. A. Scarpaci, B. Schmidt, V. Sharma, V. Shlegel, V. Singh, M. Sisti, D. Speller, P. T. Surukuchi, L. Taffarello, O. Tellier, C. Tomei, V. I. Tretyak, A. Tsymbaliuk, M. Velazquez, K. J. Vetter, S. L. Wagaarachchi, G. Wang, L. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, M. Xue, L. Yan, J. Yang, V. Yefremenko, V. Yumatov, M. M. Zarytskyy, J. Zhang, A. Zolotarova, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The CUPID Collaboration is designing a tonne-scale, background-free detector to search for double beta decay with sufficient sensitivity to fully explore the parameter space corresponding to the inverted neutrino mass hierarchy scenario. One of the CUPID demonstrators, CUPID-Mo, has proved the potential of enriched Li $$_{2}$$ 2 $$^{100}$$ 100 MoO $$_4$$ 4 crystals as suitable detectors for neutrinoless double beta decay search. In this work, we characterised cubic crystals that, compared to the cylindrical crystals used by CUPID-Mo, are more appealing for the construction of tightly packed arrays. We measured an average energy resolution of ( $$6.7\pm 0.6$$ 6.7 ± 0.6 ) keV FWHM in the region of interest, approaching the CUPID target of 5 keV FWHM. We assessed the identification of $$\alpha $$ α particles with and without a reflecting foil that enhances the scintillation light collection efficiency, proving that the baseline design of CUPID already ensures a complete suppression of this $$\alpha $$ α -induced background contribution. We also used the collected data to validate a Monte Carlo simulation modelling the light collection efficiency, which will enable further optimisations of the detector.
Published: 2021
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8. Search for double $$\beta $$ β -decay modes of $$^{64}$$ 64 Zn using purified zinc

Author: F. Bellini, M. Beretta, L. Cardani, P. Carniti, N. Casali, E. Celi, D. Chiesa, M. Clemenza, I. Dafinei, S. Di Domizio, F. Ferroni, L. Gironi, Yu. V. Gorbenko, C. Gotti, G. P. Kovtun, M. Laubenstein, S. Nagorny, S. Nisi, L. Pagnanini, L. Pattavina, G. Pessina, S. Pirro, E. Previtali, C. Rusconi, K. Schäffner, A. P. Shcherban, D. A. Solopikhin, V. D. Virich, C. Tomei, and M. Vignati
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The production of ultra-pure raw material is a crucial step to ensure the required background level in rare event searches. In this work, we establish an innovative technique developed to produce high-purity (99.999%) granular zinc. We demonstrate the effectiveness of the refining procedure by measuring the internal contaminations of the purified zinc with a high-purity germanium detector at the Laboratori Nazionali del Gran Sasso. The total activity of cosmogenic activated nuclides is measured at the level of a few mBq/kg, as well as limits on naturally occurring radionuclides are set to less than mBq/kg. The excellent radiopurity of the zinc sample allows us to search for electron capture with positron emission and neutrinoless double electron capture of $$^{64}$$ 64 Zn, setting the currently most stringent lower limits on their half-lives, $$T_{1/2}^{\varepsilon \beta ^+} > 2.7\times 10^{21}~\text {year}$$ T 1 / 2 ε β + > 2.7 × 10 21 year (90% CI), and $$T_{1/2}^{0\nu 2\varepsilon }> 2.6\times 10^{21}~\text {year}$$ T 1 / 2 0 ν 2 ε > 2.6 × 10 21 year (90% CI), respectively.
Published: 2021
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9. Search for neutrinoless double beta decay of $$^{64}$$ 64 Zn and $$^{70}$$ 70 Zn with CUPID-0

Author: O. Azzolini, J. W. Beeman, F. Bellini, M. Beretta, M. Biassoni, C. Brofferio, C. Bucci, S. Capelli, L. Cardani, E. Celi, P. Carniti, N. Casali, D. Chiesa, M. Clemenza, O. Cremonesi, A. Cruciani, A. D’Addabbo, I. Dafinei, S. Di Domizio, F. Ferroni, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, G. Keppel, M. Martinez, S. Nagorny, M. Nastasi, S. Nisi, C. Nones, D. Orlandi, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rusconi, K. Schäffner, C. Tomei, M. Vignati, and A. Zolotarova
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract CUPID-0 is the first pilot experiment of CUPID, a next-generation project searching for neutrinoless double beta decay. In its first scientific run, CUPID-0 operated 26 ZnSe cryogenic calorimeters coupled to light detectors in the underground Laboratori Nazionali del Gran Sasso. In this work, we analyzed a ZnSe exposure of 11.34 kg year to search for the neutrinoless double beta decay of $$^{70}$$ 70 Zn and for the neutrinoless positron-emitting electron capture of $$^{64}$$ 64 Zn. We found no evidence for these decays and set 90$$\%$$ % credible interval limits of $$\hbox {T}_{1/2}^{0\nu \beta \beta }$$ T1/20νββ ($$^{70}$$ 70 Zn) > 1.6 $$10^{21}$$ 1021 year and $$\hbox {T}_{1/2}^{0\nu EC \beta +}$$ T1/20νECβ+ ($$^{64}$$ 64 Zn) > 1.2$$\times 10^{22}$$ ×1022 year, surpassing by more than one order of magnitude the previous experimental results (Belli et al. in J Phys G 38(11):115107, https://doi.org/10.1088/0954-3899/38/11/115107, 2011).
Published: 2020
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10. Measurement of 216Po half-life with the CUPID-0 experiment

Author: O. Azzolini, J.W. Beeman, F. Bellini, M. Beretta, M. Biassoni, C. Brofferio, C. Bucci, S. Capelli, L. Cardani, P. Carniti, V. Caracciolo, N. Casali, D. Chiesa, M. Clemenza, I. Colantoni, O. Cremonesi, A. Cruciani, I. Dafinei, A. D'Addabbo, S. Di Domizio, F. Ferroni, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, G. Keppel, M. Martinez, S. Nagorny, M. Nastasi, S. Nisi, C. Nones, D. Orlandi, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rusconi, K. Schäffner, C. Tomei, M. Vignati, and A. Zolotarova
Subjects: Half-life measurement, Delayed coincidence, Cryogenic calorimeters, Physics, QC1-999
Abstract: Rare event physics demands very detailed background control, high-performance detectors, and custom analysis strategies. Cryogenic calorimeters combine all these ingredients very effectively, representing a promising tool for next-generation experiments. CUPID-0 is one of the most advanced examples of such a technique, having demonstrated its potential with several results obtained with limited exposure. In this paper, we present a further application. Exploiting the analysis of delayed coincidence, we can identify the signals caused by the 220Rn-216Po decay sequence on an event-by-event basis. The analysis of these events allows us to extract the time differences between the two decays, leading to a new evaluation of 216Po half-life, estimated as (143.3±2.8) ms.
Published: 2021
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11. Double-beta decay of $$^{130}\hbox {Te}$$ 130Te to the first $$0^+$$ 0+ excited state of $$^{130}\hbox {Xe}$$ 130Xe with CUORE-0

Author: C. Alduino, K. Alfonso, D. R. Artusa, F. T. Avignone III, O. Azzolini, T. I. Banks, G. Bari, J. W. Beeman, F. Bellini, A. Bersani, M. Biassoni, 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, J. Feintzeig, 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, X. Liu, Y. G. Ma, M. Maino, L. Marini, M. Martinez, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, P. J. Mosteiro, T. Napolitano, C. Nones, E. B. Norman, A. Nucciotti, T. O’Donnell, F. Orio, 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, S. Sangiorgio, D. Santone, 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, J. Wilson, L. A. Winslow, T. Wise, A. Woodcraft, L. Zanotti, G. Q. Zhang, B. X. Zhu, S. Zimmermann, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract We report on a search for double beta decay of $$^{130}\hbox {Te}$$ 130Te to the first $$0^{+}$$ 0+ excited state of $$^{130}\hbox {Xe}$$ 130Xe using a $$9.8\,\hbox {kg}\cdot \hbox {yr}$$ 9.8kg·yr exposure of $$^{130}\hbox {Te}$$ 130Te collected with the CUORE-0 experiment. In this work we exploit different topologies of coincident events to search for both the neutrinoless and two-neutrino double beta decay modes. We find no evidence for either mode and place lower bounds on the half-lives: $$T^{0\nu }_{0^+_1}>7.9\cdot 10^{23}\hbox {yr}$$ T01+0ν>7.9·1023yr and $$T^{2\nu }_{0^+_1}>2.4\cdot 10^{23}\hbox {yr}$$ T01+2ν>2.4·1023yr ($$90\%\,\hbox {CL}$$ 90%CL ). Combining our results with those obtained by the CUORICINO experiment, we achieve the most stringent constraints available for these processes: $$T^{0\nu }_{0^+_1}>1.4\cdot 10^{24}\hbox {yr}$$ T01+0ν>1.4·1024yr and $$T^{2\nu }_{0^+_1}>2.5\cdot 10^{23}\hbox {yr}$$ T01+2ν>2.5·1023yr ($$90\%\,\hbox {CL}$$ 90%CL ).
Published: 2019
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12. Background model of the CUPID-0 experiment

Author: O. Azzolini, J. W. Beeman, F. Bellini, M. Beretta, M. Biassoni, C. Brofferio, C. Bucci, S. Capelli, L. Cardani, P. Carniti, N. Casali, D. Chiesa, M. Clemenza, O. Cremonesi, A. Cruciani, I. Dafinei, S. Di Domizio, F. Ferroni, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, G. Keppel, M. Martinez, S. Nagorny, M. Nastasi, S. Nisi, C. Nones, D. Orlandi, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rusconi, K. Schäffner, C. Tomei, M. Vignati, and A. Zolotarova
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract CUPID-0 is the first large mass array of enriched Zn$$^{82}$$ 82 Se scintillating low temperature calorimeters, operated at LNGS since 2017. During its first scientific runs, CUPID-0 collected an exposure of 9.95 kg year. Thanks to the excellent rejection of $$\alpha $$ α particles, we attained the lowest background ever measured with thermal detectors in the energy region where we search for the signature of $$^{82}\hbox {Se}$$ 82Se neutrinoless double beta decay. In this work we develop a model to reconstruct the CUPID-0 background over the whole energy range of experimental data. We identify the background sources exploiting their distinctive signatures and we assess their extremely low contribution [down to $$\sim 10^{-4}$$ ∼10-4 counts/(keV kg year)] in the region of interest for $$^{82}\hbox {Se}$$ 82Se neutrinoless double beta decay search. This result represents a crucial step towards the comprehension of the background in experiments based on scintillating calorimeters and in next generation projects such as CUPID.
Published: 2019
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13. Saharan dust events in the European Alps: role in snowmelt and geochemical characterization

Author: B. Di Mauro, R. Garzonio, M. Rossini, G. Filippa, P. Pogliotti, M. Galvagno, U. Morra di Cella, M. Migliavacca, G. Baccolo, M. Clemenza, B. Delmonte, V. Maggi, M. Dumont, F. Tuzet, M. Lafaysse, S. Morin, E. Cremonese, and R. Colombo
Subjects: Environmental sciences, GE1-350, Geology, QE1-996.5
Abstract: The input of mineral dust from arid regions impacts snow optical properties. The induced albedo reduction generally alters the melting dynamics of the snowpack, resulting in earlier snowmelt. In this paper, we evaluate the impact of dust depositions on the melting dynamics of snowpack at a high-elevation site (2160 m) in the European Alps (Torgnon, Aosta Valley, Italy) during three hydrological years (2013–2016). These years were characterized by several Saharan dust events that deposited significant amounts of mineral dust in the European Alps. We quantify the shortening of the snow season due to dust deposition by comparing observed snow depths and those simulated with the Crocus model accounting, or not, for the impact of impurities. The model was run and tested using meteorological data from an automated weather station. We propose the use of repeated digital images for tracking dust deposition and resurfacing in the snowpack. The good agreement between model prediction and digital images allowed us to propose the use of an RGB index (i.e. snow darkening index – SDI) for monitoring dust on snow using images from a digital camera. We also present a geochemical characterization of dust reaching the Alpine chain during spring in 2014. Elements found in dust were classified as a function of their origin and compared with Saharan sources. A strong enrichment in Fe was observed in snow containing Saharan dust. In our case study, the comparison between modelling results and observations showed that impurities deposited in snow anticipated the disappearance of snow up to 38 d a out of a total 7 months of typical snow duration. This happened for the season 2015–2016 that was characterized by a strong dust deposition event. During the other seasons considered here (2013–2014 and 2014–2015), the snow melt-out date was 18 and 11 d earlier, respectively. We conclude that the effect of the Saharan dust is expected to reduce snow cover duration through the snow-albedo feedback. This process is known to have a series of further hydrological and phenological feedback effects that should be characterized in future research.
Published: 2019
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14. Search of the neutrino-less double beta decay of $$^{82}$$ 82 Se into the excited states of $$^{82}$$ 82 Kr with CUPID-0

Author: O. Azzolini, M. T. Barrera, J. W. Beeman, F. Bellini, M. Beretta, M. Biassoni, E. Bossio, C. Brofferio, C. Bucci, L. Canonica, S. Capelli, L. Cardani, P. Carniti, N. Casali, L. Cassina, M. Clemenza, O. Cremonesi, A. Cruciani, A. D’Addabbo, I. Dafinei, S. Di Domizio, F. Ferroni, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, G. Keppel, M. Martinez, S. Morganti, S. Nagorny, M. Nastasi, S. Nisi, C. Nones, D. Orlandi, L. Pagnanini, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rusconi, K. Schäffner, C. Tomei, M. Vignati, and A. Zolotarova
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The CUPID-0 experiment searches for double beta decay using cryogenic calorimeters with double (heat and light) read-out. The detector, consisting of 24 ZnSe crystals 95$$\%$$ % enriched in $$^{82}$$ 82 Se and two natural ZnSe crystals, started data-taking in 2017 at Laboratori Nazionali del Gran Sasso. We present the search for the neutrino-less double beta decay of $$^{82}$$ 82 Se into the 0$$_1^+$$ 1+ , 2$$_1^+$$ 1+ and 2$$_2^+$$ 2+ excited states of $$^{82}$$ 82 Kr with an exposure of 5.74 kg$$\cdot $$ · yr (2.24$$\times $$ × 10$$^{25}$$ 25 emitters$$\cdot $$ · yr). We found no evidence of the decays and set the most stringent limits on the widths of these processes: $$\varGamma $$ Γ ($$^{82}$$ 82 Se $$\rightarrow ^{82}$$ →82 Kr$$_{0_1^+}$$ 01+ )8.55$$\times $$ × 10$$^{-24}$$ -24 yr$$^{-1}$$ -1 , $$\varGamma $$ Γ ($$^{82}$$ 82 Se $$\rightarrow ^{82}$$ →82 Kr $$_{2_1^+}$$ 21+ )$$\,{
Published: 2018
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15. Analysis of cryogenic calorimeters with light and heat read-out for double beta decay searches

Author: O. Azzolini, M. T. Barrera, J. W. Beeman, F. Bellini, M. Beretta, M. Biassoni, E. Bossio, C. Brofferio, C. Bucci, L. Canonica, S. Capelli, L. Cardani, P. Carniti, N. Casali, L. Cassina, M. Clemenza, O. Cremonesi, A. Cruciani, A. D’Addabbo, I. Dafinei, S. Di Domizio, F. Ferroni, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, G. Keppel, M. Martinez, S. Morganti, S. Nagorny, M. Nastasi, S. Nisi, C. Nones, D. Orlandi, L. Pagnanini, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rusconi, K. Schäffner, C. Tomei, M. Vignati, and A. Zolotarova
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The suppression of spurious events in the region of interest for neutrinoless double beta decay will play a major role in next generation experiments. The background of detectors based on the technology of cryogenic calorimeters is expected to be dominated by $$\alpha $$ α particles, that could be disentangled from double beta decay signals by exploiting the difference in the emission of the scintillation light. CUPID-0, an array of enriched Zn$$^{82}$$ 82 Se scintillating calorimeters, is the first large mass demonstrator of this technology. The detector started data-taking in 2017 at the Laboratori Nazionali del Gran Sasso with the aim of proving that dual read-out of light and heat allows for an efficient suppression of the $$\alpha $$ α background. In this paper we describe the software tools we developed for the analysis of scintillating calorimeters and we demonstrate that this technology allows to reach an unprecedented background for cryogenic calorimeters.
Published: 2018
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16. CUPID-0: the first array of enriched scintillating bolometers for 0$$\nu \beta \beta $$ νββ decay investigations

Author: O. Azzolini, M. T. Barrera, J. W. Beeman, F. Bellini, M. Beretta, M. Biassoni, C. Brofferio, C. Bucci, L. Canonica, S. Capelli, L. Cardani, P. Carniti, N. Casali, L. Cassina, M. Clemenza, O. Cremonesi, A. Cruciani, A. D’Addabbo, I. Dafinei, S. Di Domizio, F. Ferroni, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, G. Keppel, M. Martinez, S. Morganti, S. Nagorny, M. Nastasi, S. Nisi, C. Nones, D. Orlandi, L. Pagnanini, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, F. Reindl, C. Rusconi, K. Schäffner, C. Tomei, M. Vignati, and A. Zolotarova
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The CUPID-0 detector hosted at the Laboratori Nazionali del Gran Sasso, Italy, is the first large array of enriched scintillating cryogenic detectors for the investigation of $$^{82}$$ 82 Se neutrinoless double-beta decay ($$0\nu \beta \beta $$ 0νββ ). CUPID-0 aims at measuring a background index in the region of interest (RoI) for $$0\nu \beta \beta $$ 0νββ at the level of 10$$^{-3}$$ -3 counts/(keV kg years), the lowest value ever measured using cryogenic detectors. CUPID-0 operates an array of Zn$$^{82}$$ 82 Se scintillating bolometers coupled with bolometric light detectors, with a state of the art technology for background suppression and thorough protocols and procedures for the detector preparation and construction. In this paper, the different phases of the detector design and construction will be presented, from the material selection (for the absorber production) to the new and innovative detector structure. The successful construction of the detector lead to promising preliminary detector performance which is discussed here.
Published: 2018
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17. Low energy analysis techniques for CUORE

Author: C. Alduino, K. Alfonso, D. R. Artusa, F. T. Avignone, O. Azzolini, 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. 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, D. D’Aguanno, 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, 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, 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, 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, F. Terranova, C. Tomei, 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, S. Zimmermann, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract 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 $$^{130}$$ 130 Te. 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 $$60 \, \mathrm {keV}$$ 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 inCUORE-0.
Published: 2017
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18. MOSCAB: a geyser-concept bubble chamber to be used in a dark matter search

Author: The MOSCAB Collaboration:, A. Antonicci, M. Ardid, R. Bertoni, G. Bruno, N. Burgio, G. Caruso, D. Cattaneo, F. Chignoli, M. Clemenza, M. Corcione, L. Cretara, D. Cundy, I. Felis, M. Frullini, W. Fulgione, G. Lucchini, L. Manara, M. Maspero, R. Mazza, A. Papagni, M. Perego, R. Podviyanuk, A. Pullia, A. Quintino, N. Redaelli, E. Ricci, A. Santagata, D. Sorrenti, and L. Zanotti
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The MOSCAB experiment (Materia OSCura A Bolle) uses the “geyser technique”, a variant of the superheated liquid technique of extreme simplicity. Operating principles of the new dark matter detector and technical solutions of the device are reported in detail. First results obtained in a series of test runs taken in laboratory demonstrate that we have successfully built and tested a geyser-concept bubble chamber that can be used in particle physics, especially in dark matter searches, and that we are ready to move underground for extensive data taking.
Published: 2017
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19. The projected background for the CUORE experiment

Author: 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, and M. Laubenstein
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract The Cryogenic Underground Observatory for Rare Events (CUORE) is designed to search for neutrinoless double beta decay of $$^{130}$$ 130 Te with an array of 988 TeO $$_2$$ 2 bolometers operating at temperatures around 10 mK. The experiment is currently being commissioned in Hall A of Laboratori Nazionali del Gran Sasso, Italy. The goal of CUORE is to reach a 90% C.L. exclusion sensitivity on the $$^{130}$$ 130 Te decay half-life of 9 $$\times $$ × 10 $$^{25}$$ 25 years after 5 years of data taking. The main issue to be addressed to accomplish this aim is the rate of background events in the region of interest, which must not be higher than 10 $$^{-2}$$ - 2 counts/keV/kg/year. We developed a detailed Monte Carlo simulation, based on results from a campaign of material screening, radioassays, and bolometric measurements, to evaluate the expected background. This was used over the years to guide the construction strategies of the experiment and we use it here to project a background model for CUORE. In this paper we report the results of our study and our expectations for the background rate in the energy region where the peak signature of neutrinoless double beta decay of $$^{130}$$ 130 Te is expected.
Published: 2017
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20. CUORE sensitivity to $$0\nu \beta \beta $$ 0 ν β β decay

Author: 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, and S. Zucchelli
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract We report a study of the CUORE sensitivity to neutrinoless double beta ( $$0\nu \beta \beta $$ 0 ν β β ) decay. We used a Bayesian analysis based on a toy Monte Carlo (MC) approach to extract the exclusion sensitivity to the $$0\nu \beta \beta $$ 0 ν β β decay half-life ( $$T_{1/2}^{\,0\nu }$$ T 1 / 2 0 ν ) at $$90\%$$ 90 % credibility interval (CI) – i.e. the interval containing the true value of $$T_{1/2}^{\,0\nu }$$ T 1 / 2 0 ν with $$90\%$$ 90 % probability – and the $$3~\sigma $$ 3 σ 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 $$90\%$$ 90 % CI exclusion sensitivity of $$2\cdot 10^{25}$$ 2 · 10 25 year with 3 months, and $$9\cdot 10^{25}$$ 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 $$7\cdot 10^{24}$$ 7 · 10 24 year and $$4\cdot 10^{25}$$ 4 · 10 25 year, respectively.
Published: 2017
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21. Searching for Neutrinoless Double-Beta Decay of 130Te with CUORE

Author: D. R. Artusa, F. T. Avignone, O. Azzolini, M. Balata, T. I. Banks, 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, S. Copello, 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. Fernandes, 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-Yeomans, 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. Nones, 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. Wielgus, J. Wilson, L. A. Winslow, T. Wise, A. Woodcraft, L. Zanotti, C. Zarra, B. X. Zhu, and S. Zucchelli
Subjects: Physics, QC1-999
Abstract: Neutrinoless double-beta (0νββ) decay is a hypothesized lepton-number-violating process that offers the only known means of asserting the possible Majorana nature of neutrino mass. The Cryogenic Underground Observatory for Rare Events (CUORE) is an upcoming experiment designed to search for 0νββ decay of 130Te using an array of 988 TeO2 crystal bolometers operated at 10 mK. The detector will contain 206 kg of 130Te and have an average energy resolution of 5 keV; the projected 0νββ decay half-life sensitivity after five years of livetime is 1.6 × 1026 y at 1σ (9.5 × 1025 y at the 90% confidence level), which corresponds to an upper limit on the effective Majorana mass in the range 40–100 meV (50–130 meV). In this paper, we review the experimental techniques used in CUORE as well as its current status and anticipated physics reach.
Published: 2015
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22. Current Status and Future Perspectives of the LUCIFER Experiment

Author: J. W. Beeman, F. Bellini, P. Benetti, L. Cardani, N. Casali, D. Chiesa, M. Clemenza, I. Dafinei, S. Di Domizio, F. Ferroni, A. Giachero, L. Gironi, A. Giuliani, C. Gotti, M. Maino, S. Nagorny, S. Nisi, C. Nones, F. Orio, L. Pattavina, G. Pessina, G. Piperno, S. Pirro, E. Previtali, C. Rusconi, M. Tenconi, C. Tomei, and M. Vignati
Subjects: Physics, QC1-999
Abstract: In the field of fundamental particle physics, the neutrino has become more and more important in the last few years, since the discovery of its mass. In particular, the ultimate nature of the neutrino (if it is a Dirac or a Majorana particle) plays a crucial role not only in neutrino physics, but also in the overall framework of fundamental particle interactions and in cosmology. The only way to disentangle its ultimate nature is to search for the neutrinoless double beta decay. The idea of LUCIFER is to combine the bolometric technique proposed for the CUORE experiment with the bolometric light detection technique used in cryogenic dark matter experiments. The bolometric technique allows an extremely good energy resolution while its combination with the scintillation detection offers an ultimate tool for background rejection. The goal of LUCIFER is not only to build a background-free small-scale experiment but also to directly prove the potentiality of this technique. Preliminary tests on several detectors containing different interesting DBD emitters have clearly demonstrated the excellent background rejection capabilities that arise from the simultaneous, independent, double readout of heat and scintillation light.
Published: 2013
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23. Search for Double-Beta Decay of $\mathrm{^{130}Te}$ to the $0^+$ States of $\mathrm{^{130}Xe}$ with CUORE

Author: CUORE Collaboration, Adams, D. Q., Alduino, C., Alfonso, K., Avignone III, F. T., Azzolini, O., Bari, G., Bellini, F., Benato, G., Branca, M. Biassoni A., Brofferio, C., Bucci, C., Camilleri, J., Caminata, A., Campani, A., Canonica, L., Cao, X. G., Capelli, S., Cappelli, L., Cardani, L., Casali, P. Carniti N., Celi, E., Copello, D. Chiesa M. Clemenza S., Cosmelli, C., Cremonesi, O., Creswick, R. J., D'Addabbo, A., Dafinei, I., Davis, C. J., Di Domizio, S. Dell'Oro S., Dompè, V., Fang, D. Q., Fantini, G., Ferri, M. Faverzani 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., Heeger, K. M., Huang, R. G., Huang, H. Z., Johnston, J., Keppel, G., Kolomensky, Yu. G., Ligi, C., 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., and Zucchelli, S.
Subjects: Nuclear Experiment
Abstract: The CUORE experiment is a large bolometric array searching for the lepton number violating neutrino-less double beta decay ($0\nu\beta\beta$) in the isotope $\mathrm{^{130}Te}$. In this work we present the latest results on two searches for the double beta decay (DBD) of $\mathrm{^{130}Te}$ to the first $0^{+}_2$ excited state of $\mathrm{^{130}Xe}$: the $0\nu\beta\beta$ decay and the Standard Model-allowed two-neutrinos double beta decay ($2\nu\beta\beta$). Both searches are based on a 372.5 kg$\times$yr TeO$_2$ exposure. The de-excitation gamma rays emitted by the excited Xe nucleus in the final state yield a unique signature, which can be searched for with low background by studying coincident events in two or more bolometers. The closely packed arrangement of the CUORE crystals constitutes a significant advantage in this regard. The median limit setting sensitivities at 90\% Credible Interval (C.I.) of the given searches were estimated as $\mathrm{S^{0\nu}_{1/2} = 5.6 \times 10^{24} \: \mathrm{yr}}$ for the ${0\nu\beta\beta}$ decay and $\mathrm{S^{2\nu}_{1/2} = 2.1 \times 10^{24} \: \mathrm{yr}}$ for the ${2\nu\beta\beta}$ decay. No significant evidence for either of the decay modes was observed and a Bayesian lower bound at $90\%$ C.I. on the decay half lives is obtained as: $\mathrm{(T_{1/2})^{0\nu}_{0^+_2} > 5.9 \times 10^{24} \: \mathrm{yr}}$ for the $0\nu\beta\beta$ mode and $\mathrm{(T_{1/2})^{2\nu}_{0^+_2} > 1.3 \times 10^{24} \: \mathrm{yr}}$ for the $2\nu\beta\beta$ mode. These represent the most stringent limits on the DBD of $^{130}$Te to excited states and improve by a factor $\sim5$ the previous results on this process., Comment: 13 pages, 6 figures
Published: 2021
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24. Search for Double-Beta Decay of $\mathrm{^{130}Te}$ to the $0^+$ States of $\mathrm{^{130}Xe}$ with CUORE

Author: Collaboration, CUORE, Adams, DQ, Alduino, C, Alfonso, K, III, FT Avignone, Azzolini, O, Bari, G, Bellini, F, Benato, G, Branca, M Biassoni A, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, XG, Capelli, S, Cappelli, L, Cardani, L, Casali, P Carniti N, Celi, E, Copello, D Chiesa M Clemenza S, Cosmelli, C, Cremonesi, O, Creswick, RJ, D'Addabbo, A, Dafinei, I, Davis, CJ, Domizio, S Dell'Oro S Di, Dompè, V, Fang, DQ, Fantini, G, Ferri, M Faverzani E, Ferroni, F, Fiorini, E, Franceschi, MA, Freedman, SJ, Fu, SH, Fujikawa, BK, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, TD, Han, K, Heeger, KM, Huang, RG, Huang, HZ, Johnston, J, Keppel, G, Kolomensky, Yu G, Ligi, C, Ma, L, Ma, YG, Marini, L, Maruyama, RH, Mayer, D, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, EB, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, JL, Pagan, S, Pagliarone, CE, 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, ND, Sharma, V, Singh, V, Sisti, M, Speller, D, Surukuchi, PT, Taffarello, L, Terranova, F, Tomei, C, Vetter, KJ, and Vignati, M
Subjects: nucl-ex
Abstract: The CUORE experiment is a large bolometric array searching for the leptonnumber violating neutrino-less double beta decay ($0u\beta\beta$) in theisotope $\mathrm{^{130}Te}$. In this work we present the latest results on twosearches for the double beta decay (DBD) of $\mathrm{^{130}Te}$ to the first$0^{+}_2$ excited state of $\mathrm{^{130}Xe}$: the $0u\beta\beta$ decay andthe Standard Model-allowed two-neutrinos double beta decay ($2u\beta\beta$).Both searches are based on a 372.5 kg$\times$yr TeO$_2$ exposure. Thede-excitation gamma rays emitted by the excited Xe nucleus in the final stateyield a unique signature, which can be searched for with low background bystudying coincident events in two or more bolometers. The closely packedarrangement of the CUORE crystals constitutes a significant advantage in thisregard. The median limit setting sensitivities at 90\% Credible Interval (C.I.)of the given searches were estimated as $\mathrm{S^{0u}_{1/2} = 5.6 \times10^{24} \: \mathrm{yr}}$ for the ${0u\beta\beta}$ decay and$\mathrm{S^{2u}_{1/2} = 2.1 \times 10^{24} \: \mathrm{yr}}$ for the${2u\beta\beta}$ decay. No significant evidence for either of the decay modeswas observed and a Bayesian lower bound at $90\%$ C.I. on the decay half livesis obtained as: $\mathrm{(T_{1/2})^{0u}_{0^+_2} > 5.9 \times 10^{24} \:\mathrm{yr}}$ for the $0u\beta\beta$ mode and$\mathrm{(T_{1/2})^{2u}_{0^+_2} > 1.3 \times 10^{24} \: \mathrm{yr}}$ for the$2u\beta\beta$ mode. These represent the most stringent limits on the DBD of$^{130}$Te to excited states and improve by a factor $\sim5$ the previousresults on this process.
Published: 2021

25. Experimental determination of the energy dependence of the rate of the muon transfer reaction from muonic hydrogen to oxygen for collision energies up to 0.1 eV

Author: M. Stoilov, A. Adamczak, D. Bakalov, P. Danev, E. Mocchiutti, C. Pizzolotto, G. Baldazzi, M. Baruzzo, R. Benocci, M. Bonesini, D. Cirrincione, M. Clemenza, F. Fuschino, A. D. Hillier, K. Ishida, P. J. C. King, A. Menegolli, S. Monzani, R. Ramponi, L. P. Rignanese, R. Sarkar, A. Sbrizzi, L. Tortora, E. Vallazza, A. Vacchi, Stoilov M., Adamczak A., Bakalov D., Danev P., Mocchiutti E., Pizzolotto C., Baldazzi G., Baruzzo M., Benocci R., Bonesini M., Cirrincione D., Clemenza M., Fuschino F., Hillier A.D., Ishida K., King P.J.C., Menegolli A., Monzani S., Ramponi R., Rignanese L.P., Sarkar R., Sbrizzi A., Tortora L., Vallazza E., and Vacchi A.
Subjects: Atomic, Molecular & Optical, Atomic Physics (physics.atom-ph), FOS: Physical sciences, Scattering of atoms, molecules, clusters & ion, Fine & hyperfine structure, Physics - Atomic Physics
Abstract: We report the first experimental determination of the collision-energy dependence of the muon transfer rate from the ground state of muonic hydrogen to oxygen at near-thermal energies. A sharp increase by nearly an order of magnitude in the energy range 0 - 70 meV was found that is not observed in other gases. The results set a reliable reference for quantum-mechanical calculations of low-energy processes with exotic atoms, and provide firm ground for the measurement of the hyperfine splitting in muonic hydrogen and the determination of the Zemach radius of the proton by the FAMU collaboration., 30 pages, 10 figures
Published: 2023

26. Final Result on the Neutrinoless Double Beta Decay of Se82 with CUPID-0

Author: O. Azzolini, J. W. Beeman, F. Bellini, M. Beretta, M. Biassoni, C. Brofferio, C. Bucci, S. Capelli, V. Caracciolo, L. Cardani, P. Carniti, N. Casali, D. Chiesa, M. Clemenza, I. Colantoni, O. Cremonesi, A. Cruciani, A. D’Addabbo, I. Dafinei, F. De Dominicis, S. Di Domizio, F. Ferroni, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, G. Keppel, M. Martinez, S. Nagorny, M. Nastasi, S. Nisi, C. Nones, D. Orlandi, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, C. Rusconi, K. Schäffner, C. Tomei, M. Vignati, and A. S. Zolotarova
Subjects: General Physics and Astronomy
Published: 2022
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27. The new INFN-CHNet neutron imaging facility

Author: N. Gelli, L. Giuntini, F. Cantini, O. Sans-Planell, M. Magalini, M. Manetti, L. Sodi, M. Massi, L. Castelli, C. Czelusniak, F. Taccetti, T.E. Bella, G. Marcucci, M. Clemenza, D. Di Martino, M. Morigi, M. Bettuzzi, L. Vigorelli, A. Re, A. Lo Giudice, D. Alloni, M. Prata, S. Altieri, A. Salvini, F. Grazzi, Gelli, N, Giuntini, L, Cantini, F, Sans-Planell, O, Magalini, M, Manetti, M, Sodi, L, Massi, M, Castelli, L, Czelusniak, C, Taccetti, F, Bella, T, Marcucci, G, Clemenza, M, Di Martino, D, Morigi, M, Bettuzzi, M, Vigorelli, L, Re, A, Lo Giudice, A, Alloni, D, Prata, M, Altieri, S, Salvini, A, and Grazzi, F
Subjects: Neutron tomography, Nuclear and High Energy Physics, Neutron imaging, Thermal neutron, Morphological analysi, Cultural heritage application, Instrumentation
Abstract: In this paper, NICHE (Neutron Imaging for Cultural HEritage), the new neutron imaging facility of the Italian National Institute of Nuclear Physics (INFN) is shortly presented. We report on the main features of the beamline, the specifications of the detection set-up, and the performances of the imaging system. NICHE is installed at the TRIGA reactor of LENA (Laboratorio Energia Nucleare Applicata) Pavia University laboratory (Italy). The imaging facility was designed during 2020, installed in the spring 2021, and has been in operation since May 2021. NICHE is the first Italian neutron imaging station open to national external users through the INFN-CHNet network application system. NICHE allows users to obtain neutron radiographies and tomographies, thus allowing for morphological characterisation of samples. First results to highlight the potential of the facility are reported. In particular, we show the first results about spatial resolution measurement and 3D reconstruction to provide morphological analysis capabilities.
Published: 2023
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28. Characterization of a kg-scale archaeological lead-based PbWO4 cryogenic detector for the RES-NOVA experiment

Author: J.W. Beeman, G. Benato, C. Bucci, L. Canonica, P. Carniti, E. Celi, M. Clemenza, A. D’Addabbo, F.A. Danevich, S. Di Domizio, S. Di Lorenzo, O.M. Dubovik, N. Ferreiro Iachellini, F. Ferroni, E. Fiorini, S. Fu, A. Garai, S. Ghislandi, L. Gironi, P. Gorla, C. Gotti, P.V. Guillaumon, D.L. Helis, G.P. Kovtun, M. Mancuso, L. Marini, M. Olmi, L. Pagnanini, L. Pattavina, G. Pessina, F. Petricca, S. Pirro, S. Pozzi, A. Puiu, S. Quitadamo, J. Rothe, A.P. Scherban, S. Schönert, D.A. Solopikhin, R. Strauss, E. Tarabini, V.I. Tretyak, I.A. Tupitsyna, and V. Wagner
Subjects: Radiation
Published: 2023
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29. Latest results from CUPID-0

Author: Guido Fantini, O. Azzolini, J.W. Beeman, F. Bellini, M. Beretta, M. Biassoni, C. Brofferio, C. Bucci, S. Capelli, V. Caracciolo, L. Cardani, P. Carniti, N. Casali, E. Celi, D. Chiesa, M. Clemenza, I. Colantoni, O. Cremonesi, A. Cruciani, A. D’Addabbo, I. Dafinei, S. DiDomizio, V. Dompè, F. Ferroni, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, G. Keppel, J. Kotila, M. Martinez, S. Nagorny, M. Nastasi, S. Nisi, C. Nones, D. Orlandi, L. Pagnanini, M. Pallavicini, L. Pattavina, M. Pavan, G. Pessina, V. Pettinacci, S. Pirro, S. Pozzi, E. Previtali, A. Puiu, A. Ressa, C. Rusconi, K. Schäffner, C. Tomei, M. Vignati, A.S. Zolotarova, Fantini, G, Azzolini, O, Beeman, J, Bellini, F, Beretta, M, Biassoni, M, Brofferio, C, Bucci, C, Capelli, S, Caracciolo, V, Cardani, L, Carniti, P, Casali, N, Celi, E, Chiesa, D, Clemenza, M, Colantoni, I, Cremonesi, O, Cruciani, A, D'Addabbo, A, Dafinei, I, Di Domizio, S, Dompe, V, Ferroni, F, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Keppel, G, Kotila, J, Martinez, M, Nagorny, S, Nastasi, M, Nisi, S, Nones, C, Orlandi, D, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Ressa, A, Rusconi, C, Schaffner, K, Tomei, C, Vignati, M, Zolotarova, A, 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), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
Subjects: background, Settore FIS/04, scintillation counter, cryogenics, tutkimuslaitteet, double-beta decay, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], hiukkasfysiikka, Bayesian, decay modes, crystal, ilmaisimet, detector, upgrade, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], spectral, ground state, ydinfysiikka, calorimeter, cryogenics, CUPID-0, Double beta decay, cryogenic calorimeters, scintillation, exotic decay modes
Abstract: International audience; CUPID-0 is a pilot experiment in scintillating cryogenic calorimetry for the search of neutrino-less double beta decay. 26 ZnSe crystals were operated continuously in the first project phase (March 2017 - December 2018), demonstrating unprecedented low levels of background in the region of interest at the Q-value of $^{82}\rm{Se}$. From this successful experience comes a demonstration of full alpha to beta/gamma background separation, the most stringent limits on the $^{82}\rm{Se}$ neutrino-less double beta decay, as well as the most precise measurement of the $^{82}$Se half-life. After a detector upgrade, CUPID-0 began its second and last phase (June 2019 - February 2020). We present the latest results on the neutrino-less double beta decay of $^{82}\rm{Se}$ with the full isotope exposure of $8.82~\rm{kg}\times\rm{yr}$. We set a lower bound to the ground state half life $\rm{T}_{1/2}( ^{82}\rm{Se})>4.6\times10^{24}$ yr (90 % C.I.). We review the most recent results from a Bayesian search for spectral distortions to the $^{82}\rm{Se}$ double-beta decay spectrum due to exotic decay modes.
Published: 2022
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30. Machine Learning Techniques for Pile-Up Rejection in Cryogenic Calorimeters

Author: G. Fantini, A. Armatol, E. Armengaud, W. Armstrong, C. Augier, F. T. Avignone, O. Azzolini, A. Barabash, G. Bari, A. Barresi, D. Baudin, F. Bellini, G. Benato, M. Beretta, L. Bergé, M. Biassoni, J. Billard, V. Boldrini, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, A. Cazes, E. Celi, C. Chang, M. Chapellier, A. Charrier, D. Chiesa, M. Clemenza, I. Colantoni, F. Collamati, S. Copello, F. Cova, O. Cremonesi, R. J. Creswick, A. Cruciani, A. D’Addabbo, G. D’Imperio, I. Dafinei, F. A. Danevich, M. de Combarieu, M. De Jesus, P. de Marcillac, S. Dell’Oro, S. Di Domizio, V. Dompè, A. Drobizhev, L. Dumoulin, M. Fasoli, M. Faverzani, E. Ferri, F. Ferri, F. Ferroni, E. Figueroa-Feliciano, J. Formaggio, A. Franceschi, C. Fu, S. Fu, B. K. Fujikawa, J. Gascon, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, P. Gras, M. Gros, T. D. Gutierrez, K. Han, E. V. Hansen, K. M. Heeger, D. L. Helis, H. Z. Huang, R. G. Huang, L. Imbert, J. Johnston, A. Juillard, G. Karapetrov, G. Keppel, H. Khalife, V. V. Kobychev, Yu. G. Kolomensky, S. Konovalov, Y. Liu, P. Loaiza, L. Ma, M. Madhukuttan, F. Mancarella, R. Mariam, L. Marini, S. Marnieros, M. Martinez, R. H. Maruyama, B. Mauri, D. Mayer, Y. Mei, S. Milana, D. Misiak, T. Napolitano, M. Nastasi, X. F. Navick, J. Nikkel, R. Nipoti, S. Nisi, C. Nones, E. B. Norman, V. Novosad, I. Nutini, T. O’Donnell, E. Olivieri, C. Oriol, J. L. Ouellet, S. Pagan, C. Pagliarone, L. Pagnanini, P. Pari, L. Pattavina, B. Paul, M. Pavan, H. Peng, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, D. V. Poda, T. Polakovic, O. G. Polischuk, S. Pozzi, E. Previtali, A. Puiu, A. Ressa, R. Rizzoli, C. Rosenfeld, C. Rusconi, V. Sanglard, J. Scarpaci, B. Schmidt, V. Sharma, V. Shlegel, V. Singh, M. Sisti, D. Speller, P. T. Surukuchi, L. Taffarello, O. Tellier, C. Tomei, V. I. Tretyak, A. Tsymbaliuk, A. Vedda, M. Velazquez, K. J. Vetter, S. L. Wagaarachchi, G. Wang, L. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, M. Xue, L. Yan, J. Yang, V. Yefremenko, V. Yumatov, M. M. Zarytskyy, J. Zhang, A. Zolotarova, S. Zucchelli, Fantini, G, Armatol, A, Armengaud, E, Armstrong, W, Augier, C, Avignone, FT, Azzolini, O, Barabash, A, Bari, G, Barresi, A, Baudin, D, Bellini, F, Benato, G, Beretta, M, Berge, L, Biassoni, M, Billard, J, Boldrini, V, Branca, A, Brofferio, C, Bucci, C, Camilleri, J, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cazes, A, Celi, E, Chang, C, Chapellier, M, Charrier, A, Chiesa, D, Clemenza, M, Colantoni, I, Collamati, F, Copello, S, Cova, F, Cremonesi, O, Creswick, RJ, Cruciani, A, D'Addabbo, A, D'Imperio, G, Dafinei, I, Danevich, FA, de Combarieu, M, De Jesus, M, de Marcillac, P, Dell'Oro, S, Di Domizio, S, Dompe, V, Drobizhev, A, Dumoulin, L, Fasoli, M, Faverzani, M, Ferri, E, Ferri, F, Ferroni, F, Formaggio, J, Franceschi, A, Fu, C, Fu, S, Fujikawa, BK, Gascon, J, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gras, P, Gros, M, Gutierrez, TD, Han, K, Hansen, EV, Heeger, KM, Helis, DL, Huang, HZ, Huang, RG, Imbert, L, Johnston, J, Juillard, A, Karapetrov, G, Keppel, G, Khalife, H, Kobychev, VV, Kolomensky, YG, Konovalov, S, Liu, Y, Loaiza, P, Ma, L, Madhukuttan, M, Mancarella, F, Mariam, R, Marini, L, Marnieros, S, Martinez, M, Maruyama, RH, Mauri, B, Mayer, D, Mei, Y, Milana, S, Misiak, D, Napolitano, T, Nastasi, M, Navick, XF, Nikkel, J, Nipoti, R, Nisi, S, Nones, C, Norman, EB, Novosad, V, Nutini, I, O'Donnell, T, Olivieri, E, Oriol, C, Ouellet, JL, Pagan, S, Pagliarone, C, Pagnanini, L, Pari, P, Pattavina, L, Paul, B, Pavan, M, Peng, H, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Poda, DV, Polakovic, T, Polischuk, OG, Pozzi, S, Previtali, E, Puiu, A, Ressa, A, Rizzoli, R, Rosenfeld, C, Rusconi, C, Sanglard, V, Scarpaci, J, Schmidt, B, Sharma, V, Shlegel, V, Singh, V, Sisti, M, Speller, D, Surukuchi, PT, Taffarello, L, Tellier, O, Tomei, C, Tretyak, VI, Tsymbaliuk, A, Vedda, A, Velazquez, M, Vetter, KJ, Wagaarachchi, SL, Wang, G, Wang, L, Welliver, B, Wilson, J, Wilson, K, Winslow, LA, Xue, M, Yan, L, Yang, J, Yefremenko, V, Yumatov, V, Zarytskyy, MM, Zhang, J, Zolotarova, A, Zucchelli, S, Laboratoire de Cryogénie (LC), Service de physique de l'état condensé (SPEC - UMR3680), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Institut Rayonnement Matière de Saclay (IRAMIS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Avignone, F, Bergé, L, Creswick, R, D’Addabbo, A, D’Imperio, G, Danevich, F, Dell’Oro, S, Domizio, S, Dompè, V, Figueroa-Feliciano, E, Fujikawa, B, Gutierrez, T, Hansen, E, Heeger, K, Helis, D, Huang, H, Huang, R, Kobychev, V, Kolomensky, Y, Maruyama, R, Navick, X, Norman, E, O’Donnell, T, Ouellet, J, Poda, D, Polischuk, O, Surukuchi, P, Tretyak, V, Vetter, K, Wagaarachchi, S, Winslow, L, and Zarytskyy, M
Subjects: neural network, Convolutional neural network, hierarchy, crystal, Cryogenic calorimeters, neutrino, Machine learning, CUPID, calorimeter, [INFO]Computer Science [cs], General Materials Science, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Neutrinoless double beta decay, neutrinoless, Pile-up, CUORE, background, double-beta decay, Condensed Matter Physics, Atomic and Molecular Physics, and Optics, Gran Sasso, injection, cryogenics, efficiency, mass, readout, Convolutional neural networks, upgrade, Cryogenic calorimeter, performance, Majorana
Abstract: CUORE Upgrade with Particle IDentification (CUPID) is a foreseen ton-scale array of Li2MoO4 (LMO) cryogenic calorimeters with double readout of heat and light signals. Its scientific goal is to fully explore the inverted hierarchy of neutrino masses in the search for neutrinoless double beta decay of 100Mo. Pile-up of standard double beta decay of the candidate isotope is a relevant background. We generate pile-up heat events via injection of Joule heater pulses with a programmable waveform generator in a small array of LMO crystals operated underground in the Laboratori Nazionali del Gran Sasso, Italy. This allows to label pile-up pulses and control both time difference and underlying amplitudes of individual heat pulses in the data. We present the performance of supervised learning classifiers on data and the attained pile-up rejection efficiency.
Published: 2022
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31. Negative muons for the characterization of thin layers in Cultural Heritage artefacts

Author: M Cataldo, A D Hillier, S Porcinai, K Ishida, F Grazzi, and M Clemenza
Subjects: History, Computer Science Applications, Education
Abstract: Muonic atom X-ray Emission Spectroscopy (µ-XES) is a novel technique based on the detection of high-energy X-rays emitted after the interaction of a negative muon beam with matter. Thanks to the multi-elemental range, negligible self-absorption of the x-rays and the possibility of performing depth profile studies, the technique is a very powerful probe for the analysis of cultural heritage artefacts. By tuning the energy of the incident muon beam, indeed, it is possible to investigate the different layers that constitute a sample. In this work, we report preliminary results of the analysis on two fire-gilded surfaces, in which the data analysis is coupled with Monte Carlo-based simulation software. Here, to perform a depth profile characterization, the samples were analysed at different beam energies (or momentum). Each of the resulting x-ray spectra was then analysed and compared with the output of the simulations software and a remarkably good agreement was reached. The results of the work are promising and with this approach, it will be possible to enhance the capability offered by the technique, both in terms of data analysis and data interpretation.
Published: 2023
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32. Optimization of a single module of CUPID

Author: Alberto Ressa, A. Armatol, E. Armengaud, W. Armstrong, C. Augier, F. T. Avignone, O. Azzolini, A. Barabash, G. Bari, A. Barresi, D. Baudin, F. Bellini, G. Benato, M. Beretta, L. Bergé, M. Biassoni, J. Billard, V. Boldrini, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, A. Cazes, E. Celi, A. Chang, M. Chapellier, A. Charrier, D. Chiesa, M. Clemenza, I. Colantoni, F. Collamati, S. Copello, O. Cremonesi, R. J. Creswick, A. Cruciani, A. D’ Addabbo, G. D’ Imperio, I. Dafinei, F. A. Danevich, M. de Combarieu, M. De Jesus, P. de Marcillac, S. Dell’Oro, S. Di Domizio, V. Dompè, A. Drobizhev, L. Dumoulin, G. Fantini, M. Faverzani, E. Ferri, F. Ferri, F. Ferroni, E. Figueroa-Feliciano, J. Formaggio, A. Franceschi, C. Fu, S. Fu, B. K. Fujikawa, J. Gascon, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, P. Gras, M. Gros, T. D. Gutierrez, K. Han, E. V. Hansen, K. M. Heeger, B. L. Helis, H.Z. Huang, R. G. Huang, L. Imbert, J. Johnston, A. Juillard, G. Karapetrov, G. Keppel, H. Khalife, V. V. Kobychev, Yu. G. Kolomensky, S. Konovalov, Y. Liu, P. Loaiza, L. Ma, M. Madhukuttan, F. Mancarella, R. Mariam, L. Marini, S. Marnieros, M. Martinez, R. H. Maruyama, B. Mauri, D. Mayer, Y. Mei, S. Milana, D. Misiak, T. Napolitano, M. Nastasi, X. F. Navick, J. Nikkel, R. Nipoti, S. Nisi, C. Nones, C. B. Norman, V. Novosad, I. Nutini, T. O’Donnell, E. Olivieri, C. Oriol, J. L. Ouellet, S. Pagan, C. Pagliarone, L. Pagnanini, P. Pari, L. Pattavina, B. Paul, M. Pavan, H. Peng, G. Pessina, V. Pettinacci, C. Pira, S. Pirro, D. V. Poda, T. Polakovic, O. G. Polischuk, S. Pozzi, E. Previtali, A. Puiu, A. Ressa, R. Rizzoli, C. Rosenfeld, C. Rusconi, V. Sanglard, J. Scarpaci, B. Schmidt, V. Sharma, V. Shlegel, V. Singh, M. Sisti, D. Speller, P. T. Surukuchi, L. Taffarello, O. Tellier, C. Tomei, V. I. Tretyak, A. Tsymbaliuk, M. Velazquez, K. J. Vetter, S. L. Wagaarachchi, G. Wang, L. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, M. Xue, L. Yan, J. Yang, V. Yefremenko, V. Yumatov, M. M. Zarytskyy, J. Zhang, A. Zolotarova, S. Zucchelli, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), 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), Science et Ingénierie des Matériaux et Procédés (SIMaP), Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), and CUPID
Subjects: photon yield, History, tector design, helium background, energy resolution, lithium, molybdenum nuclide, molybdenum oxygen, scintillation counter, crystal bolometer, CUORE performance, photon yield, Physics::Instrumentation and Detectors, Astrophysics::Instrumentation and Methods for Astrophysics, energy resolution, helium background, molybdenum oxygen, CUORE performance, Computer Science Applications, Education, Gran Sasso, double-beta decay: (0neutrino), lithium, crystal bolometer, molybdenum nuclide, calorimeter: cryogenics, High Energy Physics::Experiment, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], activity report, scintillation counter, detector: design, performance, tector design
Abstract: CUPID is the next generation experiment which will use scintillating cryogenic calorimeters to search for the neutrinoless double β decay. This unobserved process would shed light on the nature of the neutrino, which up to our knowledge could be a Majorana or a Dirac particle, and would give us an important hint to explain the lack of antimatter in the universe. This ambitious search needs a detector with unique characteristics such as an extremely low background level and an excellent energy resolution. CUPID is now in advanced R&D state to optimize the detector design in order to completely exploit the potentialities of scintillating cryogenic calorimeters. In the following I will describe the test performed at the LNGS (Laboratori Nazionali del Gran Sasso) of a single module of the future CUPID detector. In this contribution we present the performance obtained with a novel assembly concept, proving that it matches the requirements for CUPID.
Published: 2021
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33. Expected sensitivity to $^{128}$Te neutrinoless double beta decay with the CUORE TeO$_2$ cryogenic bolometers

Author: V. Dompè, D. Q. Adams, 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, S. Di Lorenzo, 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, S. Ghislandi, 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, R. Kowalski, 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. Nones, E. B. Norman, A. Nucciotti, I. Nutini, T. O’Donnell, M. Olmi, 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, S. Quitadamo, A. Ressa, 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, 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, Dompe, V, 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, Di Lorenzo, S, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fu, S, Fujikawa, B, Ghislandi, S, 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, Kowalski, R, 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, Olmi, M, 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, Quitadamo, S, Ressa, 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, Adams, DQ, Avignone, FT, Cao, XG, Creswick, RJ, Fang, DQ, Franceschi, MA, Freedman, SJ, Fu, SH, Fujikawa, BK, Gutierrez, TD, Hansen, EV, Heeger, KM, Huang, RG, Huang, HZ, Kolomensky, YG, Ma, YG, Maruyama, RH, Norman, EB, Ouellet, JL, Pagliarone, CE, Scielzo, ND, Surukuchi, PT, Vetter, KJ, Wagaarachchi, SL, Wang, BS, and Winslow, LA
Subjects: CUORE, Physics::Instrumentation and Detectors, Astrophysics::Instrumentation and Methods for Astrophysics, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Condensed Matter Physics, Cryogenic bolometer, Atomic and Molecular Physics, and Optics, CUORE, Cryogenic Bolometers, Cryogenic bolometers, General Materials Science, High Energy Physics::Experiment, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Neutrinoless double beta decay, Tellurium, Nuclear Experiment, 128-Te
Abstract: The CUORE experiment is a ton-scale array of $$\hbox {TeO}_2$$ TeO 2 cryogenic bolometers located at the underground Laboratori Nazionali del Gran Sasso of Istituto Nazionale di Fisica Nucleare (INFN), in Italy. The CUORE detector consists of 988 crystals operated as source and detector at a base temperature of $$\sim 10$$ ∼ 10 mK. Such cryogenic temperature is reached and maintained by means of a custom built cryogen-free dilution cryostat, designed with the aim of minimizing the vibrational noise and the environmental radioactivity. The primary goal of CUORE is the search for neutrinoless double beta decay of $$^{130}\hbox {Te}$$ 130 Te , but thanks to its large target mass and ultra-low background it is suitable for the study of other rare processes as well, such as the neutrinoless double beta decay of $$^{128}\hbox {Te}$$ 128 Te . This tellurium isotope is an attractive candidate for the search of this process, due to its high natural isotopic abundance of 31.75%. The transition energy at (866.7 ± 0.7) keV lies in a highly populated region of the energy spectrum, dominated by the contribution of the two-neutrino double beta decay of $$^{130}\hbox {Te}$$ 130 Te . As the first ton-scale infrastructure operating cryogenic $$\hbox {TeO}_2$$ TeO 2 bolometers in stable conditions, CUORE is able to achieve a factor $$>10$$ > 10 higher sensitivity to the neutrinoless double beta decay of this isotope with respect to past direct experiments.
Published: 2021
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34. Search for double $$\beta $$-decay modes of $$^{64}$$Zn using purified zinc

Author: S. Di Domizio, G. Pessina, Yu.V. Gorbenko, M. Beretta, Ezio Previtali, M. Vignati, L. Gironi, S. Nisi, V.D. Virich, Claudio Gotti, Francesca Bellini, S.S. Nagorny, Davide Chiesa, Claudia Tomei, L. Pattavina, M. Clemenza, L. Cardani, Stefano Pirro, Matthias Laubenstein, L. Pagnanini, K. Schäffner, C. Rusconi, Ioan Dafinei, E. Celi, N. Casali, D. A. Solopikhin, Paolo Carniti, G.P. Kovtun, F. Ferroni, A. P. Shcherban, Bellini, F, Beretta, M, Cardani, L, Carniti, P, Casali, N, Celi, E, Chiesa, D, Clemenza, M, Dafinei, I, Di Domizio, S, Ferroni, F, Gironi, L, Gorbenko, Y, Gotti, C, Kovtun, G, Laubenstein, M, Nagorny, S, Nisi, S, Pagnanini, L, Pattavina, L, Pessina, G, Pirro, S, Previtali, E, Rusconi, C, Schaffner, K, Shcherban, A, Solopikhin, D, Virich, V, Tomei, C, and Vignati, M
Subjects: Physics, Radionuclide, Physics - Instrumentation and Detectors, double beta decay, radioactivity, Physics and Astronomy (miscellaneous), 010308 nuclear & particles physics, Electron capture, Analytical chemistry, double beta decay, chemistry.chemical_element, Zinc, 01 natural sciences, Semiconductor detector, chemistry, Double beta decay, 0103 physical sciences, Production (computer science), Nuclide, Positron emission, 010306 general physics, Engineering (miscellaneous)
Abstract: The production of ultra-pure raw material is a crucial step to ensure the required background level in rare event searches. In this work, we establish an innovative technique developed to produce high-purity (99.999%) granular zinc. We demonstrate the effectiveness of the refining procedure by measuring the internal contaminations of the purified zinc with a high-purity germanium detector at the Laboratori Nazionali del Gran Sasso. The total activity of cosmogenic activated nuclides is measured at the level of a few mBq/kg, as well as limits on naturally occurring radionuclides are set to less than mBq/kg. The excellent radiopurity of the zinc sample allows us to search for electron capture with positron emission and neutrinoless double electron capture of $$^{64}$$ 64 Zn, setting the currently most stringent lower limits on their half-lives, $$T_{1/2}^{\varepsilon \beta ^+} > 2.7\times 10^{21}~\text {year}$$ T 1 / 2 ε β + > 2.7 × 10 21 year (90% CI), and $$T_{1/2}^{0\nu 2\varepsilon }> 2.6\times 10^{21}~\text {year}$$ T 1 / 2 0 ν 2 ε > 2.6 × 10 21 year (90% CI), respectively.
Published: 2021
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35. Searching for New Physics in two-neutrino double beta decay with CUPID

Author: A Armatol, E Armengaud, W Armstrong, C Augier, F T Avignone, O Azzolini, A Barabash, G Bari, A Barresi, D Baudin, F Bellini, G Benato, M Beretta, L Bergé, M Biassoni, J Billard, V Boldrini, A Branca, C Brofferio, C Bucci, J Camilleri, S Capelli, L Cappelli, L Cardani, P Carniti, N Casali, A Cazes, E Celi, C Chang, M Chapellier, A Charrier, D Chiesa, M Clemenza, I Colantoni, F Collamati, S Copello, O Cremonesi, R J Creswick, A Cruciani, A D’ Addabbo, G D’ Imperio, I Dafinei, F A Danevich, M de Combarieu, M De Jesus, P de Marcillac, S Dell’Oro, S Di Domizio, V Dompè, A Drobizhev, L Dumoulin, G Fantini, M Faverzani, E Ferri, F Ferri, F Ferroni, E Figueroa-Feliciano, J Formaggio, A Franceschi, C Fu, S Fu, B K Fujikawa, J Gascon, S Ghislandi, A Giachero, L Gironi, A Giuliani, P Gorla, C Gotti, P Gras, M Gros, T D Gutierrez, K Han, E V Hansen, K M Heeger, D L Helis, H Z Huang, R G Huang, L Imbert, J Johnston, A Juillard, G Karapetrov, G Keppel, H Khalife, V V Kobychev, J Kotila, Yu G Kolomensky, S Konovalov, Y Liu, P Loaiza, L Ma, M Madhukuttan, F Mancarella, R Mariam, L Marini, S Marnieros, M Martinez, R H Maruyama, B Mauri, D Mayer, Y Mei, S Milana, D Misiak, T Napolitano, M Nastasi, X F Navick, J Nikkel, R Nipoti, S Nisi, C Nones, E B Norman, V Novosad, I Nutini, T O’Donnell, E Olivieri, C Oriol, J L Ouellet, S Pagan, C Pagliarone, L Pagnanini, P Pari, L Pattavina, B Paul, M Pavan, H Peng, G Pessina, V Pettinacci, C Pira, S Pirro, D V Poda, T Polakovic, O G Polischuk, S Pozzi, E Previtali, A Puiu, S Quitadamo, A Ressa, R Rizzoli, C Rosenfeld, C Rusconi, V Sanglard, J Scarpaci, B Schmidt, V Sharma, V Shlegel, V Singh, M Sisti, D Speller, P T Surukuchi, L Taffarello, O Tellier, C Tomei, V I Tretyak, A Tsymbaliuk, M Velazquez, K J Vetter, S L Wagaarachchi, G Wang, L Wang, B Welliver, J Wilson, K Wilson, L A Winslow, M Xue, L Yan, J Yang, V Yefremenko, V Yumatov, M M Zarytskyy, J Zhang, A Zolotarova, S Zucchelli, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), 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 Rayonnement Matière de Saclay (IRAMIS), Science et Ingénierie des Matériaux et Procédés (SIMaP), Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), and Université Grenoble Alpes (UGA)
Subjects: CUPID, Neutrinoless Double Beta Decay, LNGS, Particle Physics, Neutrino, Majorana Neutrino, History, LNGS, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], hiukkasfysiikka, Neutrinoless Double Beta Decay, Education, crystal, CUPID, Neutrino, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], double-beta decay: (2neutrino), Particle Physics, scintillation counter, symmetry: violation, background, new physics: search for, Majorana Neutrino, neutriinot, sensitivity, violation: Lorentz, Majoron, Computer Science Applications, calorimeter: cryogenics, electron: energy spectrum, symmetry: Lorentz, ydinfysiikka
Abstract: In the past few years, attention has been drawn to the fact that a precision analysis of two-neutrino double beta decay (2υββ) allows the study of interesting physics cases like the emission of Majoron bosons and possible Lorentz symmetry violation. These processes modify the summed-energy distribution of the two electrons emitted in 2υββ. CUPID is a next-generation experiment aiming to exploit 100Mo-enriched scintillating Li2MoO4 crystals, operating as cryogenic calorimeters. Given the relatively fast half-life of 100Mo 2υββ and the large exposure that can be reached by CUPID, we expect to measure with very high precision the 100Mo 2υββ spectrum shape, reaching great sensitivities in the search for distortions induced by the physics beyond the Standard Model. In this contribution, we present the CUPID exclusion sensitivity for such New Physics processes, as well as the preliminary projected background of CUPID.
Published: 2021
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36. Double beta decay results from the CUPID-0 experiment

Author: Davide Chiesa, C. Nones, S. Nagorny, A. D'Addabbo, C. Bucci, P. Gorla, F. Ferroni, L. Pagnanini, Silvia Capelli, Massimiliano Nastasi, J. W. Beeman, N. Casali, M. I. Martínez, M. Biassoni, S. Di Domizio, M. Beretta, Francesca Bellini, K. Schäffner, Stefano Pozzi, Marco Pallavicini, C. Brofferio, G. Pessina, M. Vignati, A. S. Zolotarova, S. Nisi, Ioan Dafinei, L. Gironi, A. Puiu, A. Cruciani, Claudio Gotti, V. Pettinacci, O. Azzolini, L. Pattavina, L. Cardani, Oliviero Cremonesi, Stefano Pirro, D. Orlandi, E. Celi, M. Pavan, C. Rusconi, Giorgio Keppel, Claudia Tomei, Ezio Previtali, Paolo Carniti, M. Clemenza, A. Giuliani, 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, Chiesa, D, Azzolini, O, Beeman, J, Bellini, F, Beretta, M, Biassoni, M, Brofferio, C, Bucci, C, Capelli, S, Cardani, L, Celi, E, Carniti, P, Casali, N, Clemenza, M, Cremonesi, O, Cruciani, A, D'Addabbo, A, Dafinei, I, Di Domizio, S, Ferroni, F, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Keppel, G, Martinez, M, Nagorny, S, Nastasi, M, Nisi, S, Nones, C, Orlandi, D, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rusconi, C, Schaffner, K, Tomei, C, Vignati, M, and Zolotarova, A
Subjects: Physics, Detector, Phase (waves), background: model, double beta decay, FOS: Physical sciences, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 7. Clean energy, Nuclear physics, electron: spectrum, nucleus: transition, Double beta decay, calorimeter: cryogenics, detector: energy resolution, double-beta decay: (2neutrino), scintillation counter: crystal, Nuclear Experiment (nucl-ex), energy resolution: high, Nuclear Experiment, Counting rate, experimental results
Abstract: A convincing observation of neutrino-less double beta decay (0$\nu$DBD) relies on the possibility of operating high energy-resolution detectors in background-free conditions. Scintillating cryogenic calorimeters are one of the most promising tools to fulfill the requirements for a next-generation experiment. Several steps have been taken to demonstrate the maturity of this technique, starting from the successful experience of CUPID-0. The CUPID-0 experiment demonstrated the complete rejection of the dominant alpha background measuring the lowest counting rate in the region of interest for this technique. Furthermore, the most stringent limit on the $^{82}$Se 0$\nu$DBD was established running 26 ZnSe crystals during two years of continuous detector operation. In this contribution we present the final results of CUPID-0 Phase I including a detailed model of the background, the measurement of the $^{82}$Se 2$\nu$DBD half-life and the evidence that this nuclear transition is single state dominated., Comment: 40th International Conference on High Energy physics - ICHEP2020 July 28 - August 6, 2020 Prague, Czech Republic (virtual meeting)
Published: 2020
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37. DEMETRA: Suppression of the Relaxation Induced by Radioactivity in Superconducting Qubits

Author: I. Colantoni, Laura Cardani, N. Casali, M. Vignati, Lukas Gruenhaupt, M. I. Martínez, L. Gironi, Wolfgang Wernsdorfer, Francesco Valenti, Fabio Henriques, Daria Gusenkova, Stefano Pirro, Marc Lagoin, C. Rusconi, Ioan Pop, M. Clemenza, Alexey V. Ustinov, Angelo Cruciani, Gianluigi Catelani, Thibault Charpentier, Cardani, L, Casali, N, Catelani, G, Charpentier, T, Clemenza, M, Colantoni, I, Cruciani, A, Gironi, L, Gruenhaupt, L, Gusenkova, D, Henriques, F, Lagoin, M, Martinez, M, Pirro, S, Pop, I, Rusconi, C, Ustinov, A, Valenti, F, Vignati, M, and Wernsdorfer, W
Subjects: Kinetic inductance detectors, Quantum bits, Radioactivity, Phonon, Cosmic ray, 01 natural sciences, 010305 fluids & plasmas, Kinetic inductance detector, Condensed Matter::Superconductivity, 0103 physical sciences, General Materials Science, ddc:530, 010306 general physics, Computer Science::Databases, Physics, Superconductivity, Condensed matter physics, Quantum bit, Condensed Matter Physics, Condensed Matter::Mesoscopic Systems and Quantum Hall Effect, Atomic and Molecular Physics, and Optics, Qubit, Quasiparticle, Condensed Matter::Strongly Correlated Electrons, Cooper pair, Coherence (physics)
Abstract: Non-equilibrium quasiparticles can deteriorate the performance of superconducting qubits by reducing their coherence. We are investigating a source of quasiparticles that has been too long neglected, namely radioactivity: cosmic rays, environmental radioactivity and contaminants in the materials can all generate phonons of energy sufficient to break Cooper pairs and thus increase the number of quasiparticles. In this contribution, we describe the status of the project and its perspectives.
Published: 2020
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38. Results from the CUORE experiment

Author: D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, 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, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, 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. Singh, M. Sisti, D. Speller, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, S. Zucchelli, Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, 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, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, 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, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, and Zucchelli, S
Subjects: neutrinoless double beta decay
Published: 2020

39. Ce:LaBr$_3$ crystals with SiPM array readout and temperature control for the FAMU experiment at RAL

Author: M. Baruzzo, M. Rossella, E. Vallazza, D. Ghittori, R. Mazza, Roberto Benocci, M. Clemenza, E. Mocchiutti, Alessandro Menegolli, Michele Prata, M. Bonesini, R. Bertoni, A. de Bari, Bonesini, M, Benocci, R, Bertoni, R, Clemenza, M, Ghittori, D, Mazza, R, Vallazza, E, De Bari, A, Menegolli, A, Prata, M, Rossella, M, Baruzzo, M, and Mocchiutti, E
Subjects: Physics - Instrumentation and Detectors, APDS, X-ray detector, FOS: Physical sciences, 01 natural sciences, 030218 nuclear medicine & medical imaging, law.invention, 03 medical and health sciences, 0302 clinical medicine, Optics, Silicon photomultiplier, law, 0103 physical sciences, APDs, visible and IR photons (solid-state) (PIN diodes, CMOS imagers, Instrumentation, Photon detectors for UV, CCDs, EBCCDs, EMCCDs, etc), G-APDs, Si-PMTs, X-ray detectors, Mathematical Physics, Photon detectors for UV, APDs, CCDs, CMOS imagers, EBCCDs, EMCCDs, G-APDs, Si-PMTs, visible and IR photons (solid-state), PIN diodes, X-ray detectors, Physics, Temperature control, Regulated power supply, 010308 nuclear & particles physics, business.industry, Detector, PIN diode, Instrumentation and Detectors (physics.ins-det), Full width at half maximum, business
Abstract: Compact X-rays detectors made of 1/2 inch Ce:LaBr3 crystals of cubic shape with SiPM array readout have been developed for the FAMUexperiment at RIKEN-RAL, to instrument regions of difficult access. Due to the high photon yield of Ce:LaBr3 it was possible to use a simple readout scheme based on CAEN V1730 digitizers, without a dedicated amplification stage. The drift with temperature of SiPM gain was corrected by using CAEN A7885D regulated power supply chips with temperature feedback. Energy resolutions (FWHM) around 3:5% at the 137Cs peak and around 9% at the 57Co peak were obtained., Comment: 15th Topical Seminar on Innovative Particle and Radiation Detectors (IPRD19) 14-17 October 2019 Siena, Italy
Published: 2020
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40. Results from the CUORE experiment

Author: Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, 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, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, 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, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, 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, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, 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. Singh, M. Sisti, D. Speller, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, S. Zucchelli, Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, 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, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, 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, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, 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, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, 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. Singh, M. Sisti, D. Speller, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, and S. Zucchelli
Published: 2020

41. Performance of the low threshold Optimum Trigger on CUORE data

Author: Branca, A, Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, 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, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, A. Branca, D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Biassoni, 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, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, 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, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, S. Zucchelli, Branca, A, Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, 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, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, Zucchelli, S, A. Branca, D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Biassoni, 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, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, 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, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, and S. Zucchelli
Abstract: The Optimum Trigger (OT) is based on a threshold algorithm applied on waveforms filtered by exploiting the matched filter technique. The OT trigger thresholds improve by 60-90% with respect to the thresholds obtained with the standard trigger, ranging between ∼ 20 and 100 keV . Low trigger thresholds open the way to Dark Matter searches and to improvements in the neutrinoless double beta decay analysis. Nevertheless, running the OT on CUORE data is demanding from the computational resources point of view. For this reason, the algorithm has been revised and adapted to cope with CUORE data. The work done to implement OT in CUORE and its performances will be discussed.
Published: 2020

42. Background model of the CUPID-0 experiment

Author: C. Nones, Davide Chiesa, M. Biassoni, P. Gorla, F. Ferroni, M. Clemenza, A. Cruciani, Claudio Gotti, L. Pattavina, A. Giuliani, L. Pagnanini, A. S. Zolotarova, Oliviero Cremonesi, S. Di Domizio, C. Bucci, O. Azzolini, Paolo Carniti, F. Bellini, C. Brofferio, Claudia Tomei, Ioan Dafinei, A. Puiu, Stefano Pozzi, M. Pavan, L. Gironi, C. Rusconi, N. Casali, S.S. Nagorny, M. Vignati, Silvia Capelli, Massimiliano Nastasi, K. Schäffner, M. I. Martínez, Marco Pallavicini, V. Pettinacci, G. Pessina, L. Cardani, S. Nisi, Stefano Pirro, G. Keppel, J. W. Beeman, D. Orlandi, M. Beretta, Ezio Previtali, 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), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, CUPID, Azzolini, O, Beeman, J, Bellini, F, Beretta, M, Biassoni, M, Brofferio, C, Bucci, C, Capelli, S, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Clemenza, M, Cremonesi, O, Cruciani, A, Dafinei, I, Domizio, S, Ferroni, F, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Keppel, G, Martinez, M, Nagorny, S, Nastasi, M, Nisi, S, Nones, C, Orlandi, D, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rusconi, C, Schaffner, K, Tomei, C, Vignati, M, and Zolotarova, A
Subjects: Particle physics, Physics - Instrumentation and Detectors, experimental methods, Physics and Astronomy (miscellaneous), Bolometer, background: model, FOS: Physical sciences, chemistry.chemical_element, lcsh:Astrophysics, helium, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Rare Event, neutrino less double beta decay, 01 natural sciences, thermal, law.invention, double-beta decay: (0neutrino), temperature: low, law, Double beta decay, lcsh:QB460-466, 0103 physical sciences, calorimeter, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment (nucl-ex), Neutrinos, Double Beta Decay, 010306 general physics, Nuclear Experiment, Engineering (miscellaneous), scintillation counter, Helium, Physics, Range (particle radiation), 010308 nuclear & particles physics, Instrumentation and Detectors (physics.ins-det), Background model, Gran Sasso, Calorimeter, chemistry, Scintillation counter, lcsh:QC770-798, bolometers, Neutrino, Energy (signal processing)
Abstract: CUPID-0 is the first large mass array of enriched Zn$^{82}$Se scintillating low temperature calorimeters, operated at LNGS since 2017. During its first scientific runs, CUPID-0 collected an exposure of 9.95 kg yr. Thanks to the excellent rejection of $\alpha$ particles, we attained the lowest background ever measured with thermal detectors in the energy region where we search for the signature of $^{82}$Se neutrinoless double beta decay. In this work we develop a model to reconstruct the CUPID-0 background over the whole energy range of experimental data. We identify the background sources exploiting their distinctive signatures and we assess their extremely low contribution (down to $\sim10^{-4}$ counts/(keV kg yr)) in the region of interest for $^{82}$Se neutrinoless double beta decay search. This result represents a crucial step towards the comprehension of the background in experiments based on scintillating calorimeters and in next generation projects such as CUPID., Comment: This is a post-peer-review, pre-copyedit version of an article published in Eur. Phys. J. C. The final authenticated version is available online at: https://doi.org/10.1140/epjc/s10052-019-7078-8
Published: 2019
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43. CUORE: The first bolometric experiment at the ton scale for the search for neutrino-less double beta decay

Author: James R. Wilson, N. Moggi, Monica Sisti, Carlo Cosmelli, Samuele Sangiorgio, Lindley Winslow, Jeremy S. Cushman, C. Rosenfeld, A. Nucciotti, Claudio Gotti, C. Alduino, C. Bucci, T. D. Gutierrez, S. Copello, V. Pettinacci, P. Gorla, F. Ferroni, C. Tomei, C. Brofferio, M. Faverzani, Stefano Pirro, D. D'Aguanno, S. Morganti, Paolo Carniti, A. Giuliani, Davide Chiesa, C. Rusconi, C. J. Davis, I. Dafinei, M. Sakai, M. Pavan, S. Zucchelli, K. Wilson, Y. Mei, N. Chott, S. Di Domizio, L. Cappelli, Eric B. Norman, T. Napolitano, V. Dompè, Oliviero Cremonesi, Jonathan Ouellet, G. Bari, A. D'Addabbo, Stefano Dell'Oro, M. Clemenza, Laura Cardani, T. Wise, D. Q. Fang, B. K. Fujikawa, Vasundhara Singh, Stefano Pozzi, Xi-Guang Cao, H. Z. Huang, K. M. Heeger, G. Keppel, M. Biassoni, L. Taffarello, C. Pagliarone, S. Zimmermann, Marco Pallavicini, T. O'Donnell, A. Caminata, Carlo Ligi, Yu. G. Kolomensky, Ezio Previtali, G. Pessina, B. Schmidt, Danielle Speller, B. S. Wang, B. Welliver, M. Vignati, O. Azzolini, Irene Nutini, Ettore Fiorini, V. Novati, Andrea Giachero, A. Campani, C. Pira, L. Pattavina, A. Drobizhev, Silvia Capelli, C. Nones, A. Puiu, F. Terranova, Yu-Gang Ma, Massimiliano Nastasi, D. Q. Adams, K. Alfonso, N. Casali, Giovanni Benato, M. A. Franceschi, G. Fantini, A. Branca, R. G. Huang, Ke Han, Reina H. Maruyama, Stuart J. Freedman, S. L. Wagaarachchi, L. Gironi, F. T. Avignone, A. Bersani, R. J. Creswick, F. Bellini, A. Leder, N. D. Scielzo, L. Zanotti, L. Canonica, L. Marini, J. Johnston, Evelyn Ferri, 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), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Adams D.Q., Alduino C., Alfonso K., Avignone F.T., Azzolini O., Bari G., Bellini F., Benato G., Bersani A., Biassoni M., Branca A., Brofferio C., Bucci C., Caminata A., Campani A., Canonica L., Cao X.G., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Chiesa D., Chott N., Clemenza M., Copello S., Cosmelli C., Cremonesi O., Creswick R.J., Cushman J.S., D'Addabbo A., D'Aguanno D., Dafinei I., Davis C.J., Dell'Oro S., Di Domizio S., Dompe V., Drobizhev A., Fang D.Q., Fantini G., Faverzani M., Ferri E., Ferroni F., Fiorini E., Franceschi M.A., Freedman S.J., Fujikawa B.K., Giachero A., Gironi L., Giuliani A., Gorla P., Gotti C., Gutierrez T.D., Han K., Heeger K.M., Huang R.G., Huang H.Z., Johnston J., Keppel G., Kolomensky Y.G., Leder A., Ligi C., Ma Y.G., Marini L., Maruyama R.H., Mei Y., Moggi N., Morganti S., Napolitano T., Nastasi M., Nones C., Norman E.B., Novati V., Nucciotti A., Nutini I., O'Donnell T., Ouellet J.L., Pagliarone C.E., 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., Singh V., Sisti M., Speller D., Taffarello L., Terranova F., Tomei C., Vignati M., Wagaarachchi S.L., Wang B.S., Welliver B., Wilson J., Wilson K., Winslow L.A., Wise T., Zanotti L., Zimmermann S., Zucchelli S., Département de Physique des Particules (ex SPP) (DPhP), Adams, D, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Bersani, A, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, Cushman, J, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Dell'Oro, S, Di Domizio, S, Dompe, V, Drobizhev, A, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Leder, A, Ligi, C, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, Pagliarone, C, 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, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Wise, T, Zanotti, L, Zimmermann, S, and Zucchelli, S
Subjects: Cryostat, Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Dark matter, energy resolution, 01 natural sciences, tellurium: oxygen, law.invention, Nuclear physics, energy: threshold, CUORE, Bolometers, Neutrinoless double beta decay, Ton-scale detector, double-beta decay: (0neutrino), bolometer, law, Observatory, Double beta decay, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation, activity report, background: suppression, detector: design, Neutrinoless double beta decay, Ton-scale detector, Bolometers, Physics, 010308 nuclear & particles physics, Bolometer, Detector, sensitivity, cryogenics, High Energy Physics::Experiment, Neutrino, performance
Abstract: The Cryogenic Underground Observatory for Rare Events (CUORE) is the most massive bolometric experiment searching for neutrino-less double beta (0 ν β β ) decay. The detector consists of an array of 988 TeO 2 crystals (742 kg) arranged in a compact cylindrical structure of 19 towers. This paper will describe the CUORE experiment, including the cryostat, and present the detector performance during the first year of running. Additional detail will describe the effort made in improving the energy resolution in the 130Te 0 ν β β decay region of interest (ROI) and the suppression of backgrounds. A description of work to lower the energy threshold in order to give CUORE the sensitivity to search for other rare events, such as dark matter, will also be provided.
Published: 2019
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44. Result on the neutrinoless double beta decay search of 82 Se with the CUPID-0 experiment

Author: A. S. Zolotarova, Paolo Carniti, Stefano Nisi, A. Puiu, Oliverio Cremonesi, Angelo Cruciani, M. Clemenza, L. Pattavina, Ezio Previtali, Marco Pallavicini, M. Beretta, Sergio Di Domizio, A. D'Addabbo, L. Pagnanini, P. Gorla, F. Ferroni, L. Gironi, N. Casali, M. Pavan, G. Pessina, Karoline Schäffner, Laura Cardani, Stefano Pozzi, V. Palmieri, C. Bucci, Silvia Capelli, Massimiliano Nastasi, Jeffrey W. Beeman, Claudia Nones, Lorenzo Cassina, Claudio Gotti, Maria Teresa Barrera, Silvio Morganti, M. Vignati, V. Pettinacci, Stefano Pirro, A. Giuliani, Sergei Nagorny, M. Biassoni, Lucia Canonica, F. Bellini, C. Rusconi, C. Brofferio, M. I. Martínez, Ioan Dafinei, Claudia Tomei, O. Azzolini, G. Keppel, D. Orlandi, 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), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Bellini, F, Azzolini, O, Teresa Barrera, M, Beeman, J, Beretta, M, Biassoni, M, Brofferio, C, Bucci, C, Canonica, L, Capelli, S, Cardani, L, Carniti, P, Casali, N, Cassina, L, Clemenza, M, Cremonesi, O, Cruciani, A, D’Addabbo, A, Dafinei, I, Di Domizio, S, Ferroni, F, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Keppel, G, Martinez, M, Morganti, S, Nagorny, S, Nastasi, M, Nisi, S, Nones, C, Orlandi, D, Pagnanini, L, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rusconi, C, Schäffner, K, Tomei, C, Vignati, M, and Zolotarova, A
Subjects: Semileptonic decay, lcsh:QC793-793.5, Large array, General Physics and Astronomy, Majorana neutrino, Neutrinoless double beta decay, Zn82Se scintillating cryogenic calorimeters, Zn82Se scintillating cryogenic calorimeter, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 7. Clean energy, 01 natural sciences, Particle identification, law.invention, scintillation counter: cryogenics, Nuclear physics, mass: scale, background: low, bolometer, double-beta decay: (0neutrino), law, Double beta decay, 0103 physical sciences, Mass scale, neutrino: mass, 010306 general physics, Physics, 010308 nuclear & particles physics, particle: energy, Bolometer, lcsh:Elementary particle physics, semileptonic decay, Gran Sasso, calorimeter: cryogenics, neutrino: Majorana, particle identification, α particles, FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
Abstract: CUPID-0 is the first large array of scintillating Zn 82 Se cryogenic calorimeters (bolometers) implementing particle identification for the search of the neutrinoless double beta decay (0 ν β β ). The detector consists of 24 enriched Zn 82 Se bolometers for a total 82 Se mass of 5.28 kg and it has been taking data in the underground LNGS (Italy) since March 2017. In this article we show how the dual read-out provides a powerful tool for the α particles rejection. The simultaneous use of the heat and light information allows us to reduce the background down to (3.2 − 1.1 + 1.3 )×10 − 3 counts/(keV kg year), an unprecedented level for cryogenic calorimeters. In a total exposure of 5.46 kg year Zn 82 Se we set the most stringent limit on the 0 ν β β decay 82 Se half-life T 1 / 2 0 ν > 4.0 × 10 24 year at 90% C.I.
Published: 2019
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45. The Ruthenium-106 plume over Europe in 2017: a source-receptor model to estimate the source region

Author: Giovanni Baccolo, Niccolò Maffezzoli, Elena Di Stefano, M. Clemenza, Maffezzoli, N, Baccolo, G, Di Stefano, E, and Clemenza, M
Subjects: Atmospheric Science, Source-receptor model, 010504 meteorology & atmospheric sciences, Meteorology, Atmospheric models, environmental radioactivity, atmospheric modeling, 106Ru, Rutenium, 106Ru, Fallout, Backtrajectory, HYSPLIT, Source-receptor model, HYSPLIT, Atmospheric model, 010501 environmental sciences, 01 natural sciences, Backtrajectory, Settore FIS/07 - Fisica Applicata(Beni Culturali, Ambientali, Biol.e Medicin), Plume, Rutenium, Atmosphere, Altitude, Data assimilation, Trajectory, Environmental science, Fallout, 0105 earth and related environmental sciences, General Environmental Science
Abstract: Between the end of September and the beginning of October 2017, low but detectable air concentrations of Ruthenium-106 ( R 106 u ) were measured throughout the European atmosphere. To date, the source has not been clearly identified. This study aims at constraining the location of the most likely emission source, by combining HYSPLIT back trajectories and a multi-site source-receptor model. The model follows a concentration weighted trajectory (CWT) approach, based on a R 106 u measurement dataset gathered by the International Atomic Energy Agency (IAEA) shortly after the event and shared by the French Institut de Radioprotection et de Surete Nucleaire (IRSN). The back trajectories are computed using Global Data Assimilation System (GDAS) and ERA-Interim meteorological data, with horizontal resolution from 1.5° to 0.5°. The effect of the starting altitude was also investigated. The source-receptor model results show that the most likely emission source region extends from Ukraine to the West to the Russian Volga and Ural regions to the East, in accordance with two previous studies. The analyses also show that the identified source region is relatively insensitive to the type of meteorological data, their horizontal resolution and values of starting altitude. The model precision is found to increase with increasing number of receptors. The method is fully open-source, requires low computational resources and is therefore suited to estimate the source origin of radioactive pollutants on a real time basis, providing an additional tool to more sophisticated atmospheric models.
Published: 2019

46. CUPID-0: A double-readout cryogenic detector for Double Beta Decay search

Author: D. Orlandi, Davide Chiesa, C. Brofferio, Jeffrey W. Beeman, G. Keppel, S. Di Domizio, C. Rusconi, M. Clemenza, Laura Cardani, K. Schäffner, Stefano Pozzi, L. Pattavina, M. Vignati, Claudio Gotti, S. S. Nagorny, M. Pavan, L. Pagnanini, I. Dafinei, P. Gorla, F. Ferroni, C. Tomei, Silvia Capelli, Marco Pallavicini, Massimiliano Nastasi, A. Giuliani, Paolo Carniti, G. Pessina, F. Bellini, C. Zolotarova, M. Beretta, V. Pettinacci, Stefano Pirro, C. Nones, A. Puiu, N. Casali, L. Gironi, M. Biassoni, O. Azzolini, C. Bucci, Miriam Lucio Martinez, Oliviero Cremonesi, S. Morganti, Angelo Cruciani, Ezio Previtali, Stefano Nisi, 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), Département de Physique des Particules (ex SPP) (DPhP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Département de Physique des Particules (ex SPP) (DPP), Azzolini, O, Beeman, J, Bellini, F, Beretta, M, Biassoni, M, Brofferio, C, Bucci, C, Capelli, S, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Clemenza, M, Cremonesi, O, Cruciani, A, Dafinei, I, Di Domizio, S, Ferroni, F, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Keppel, G, Martinez, M, Morganti, S, Nagorny, S, Nastasi, M, Nisi, S, Nones, C, Orlandi, D, Pagnanini, L, Pallavicini, M, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rusconi, C, Schaffner, K, Tomei, C, Vignati, M, and Zolotarova, C
Subjects: Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, Crystal growth, macro-bolometers, Neutrino-less double beta decay, 7. Clean energy, 01 natural sciences, Particle identification, law.invention, Nuclear physics, double-beta decay: (0neutrino), bolometer, law, Double beta decay, 0103 physical sciences, CUPID, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, selenium, Instrumentation, Scintillation, activity report, 010302 applied physics, Physics, background, Bolometer, Detector, zinc, Alpha background, Background level, Gran Sasso, FIS/01 - FISICA SPERIMENTALE, ZnSe, calorimeter: cryogenics, scintillation counter: crystal, Cryogenic detectors, High Energy Physics::Experiment, scintillating cryogenic calorimeter, FIS/04 - FISICA NUCLEARE E SUBNUCLEARE, performance
Abstract: CUPID-0 is the first large mass neutrino-less double beta decay ( 0 ν β β ) experiment based on cryogenic calorimeters with dual read-out of light and heat for background rejection. The detector assembly, consisting of 26 ZnSe crystals, 2 natural and 24 enriched at 95% in 82Se, all coupled with bolometric light detectors, has been constructed respecting very strict protocols and procedures, from the material selection during crystal growth to the new and innovative detector framework, in the attempt to achieve the best performance of the array. The successful construction of the detector lead to promising preliminary results, here presented. The array is in fact taking data underground at LNGS (Italy) since March 2017 and the particle identification, enabled by the light read-out, provides an unprecedented background level, for cryogenic calorimeters, of only 3.2 counts keV − 1 t − 1 yr − 1 in the region of interest of the 0 ν β β search for 82Se, namely around 3 MeV.
Published: 2019
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47. CUPID-0, challenges and achievements in the struggle of 0-background double-beta decay experiments

Author: L. Gironi, N. Casali, G. Keppel, C. Nones, A. Puiu, D. Orlandi, A. D'Addabbo, I. Dafinei, Oliviero Cremonesi, Claudio Gotti, L. Pattavina, Marco Pallavicini, Lucia Canonica, S. Di Domizio, M. Clemenza, G. Pessina, F. Bellini, S. S. Nagorny, C. Bucci, Lorenzo Cassina, Miriam Lucio Martinez, A. Giuliani, Angelo Cruciani, Ezio Previtali, S. Morganti, Silvia Capelli, Laura Cardani, Stefano Pozzi, Massimiliano Nastasi, A. S. Zolotarova, L. Pagnanini, Jeffrey W. Beeman, M. T. Barrera, O. Azzolini, Paolo Carniti, M. Vignati, V. Palmieri, M. Biassoni, V. Pettinacci, Stefano Pirro, M. Pavan, K. Schäffner, P. Gorla, F. Ferroni, C. Tomei, E. Bossio, M. Beretta, C. Brofferio, C. Rusconi, Stefano Nisi, 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), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Azzolini, O, Barrera, M, Beeman, J, Bellini, F, Beretta, M, Biassoni, M, Bossio, E, Brofferio, C, Bucci, C, Canonica, L, Capelli, S, Cardani, L, Carniti, P, Casali, N, Cassina, L, Clemenza, M, Cremonesi, O, Cruciani, A, D'Addabbo, A, Dafinei, I, Domizio, S, Ferroni, F, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Keppel, G, Martinez, M, Morganti, S, Nagorny, S, Nastasi, M, Nisi, S, Nones, C, Orlandi, D, Pagnanini, L, Pallavicini, M, Palmieri, V, Pattavina, L, Pavan, M, Pessina, G, Pettinacci, V, Pirro, S, Pozzi, S, Previtali, E, Puiu, A, Rusconi, C, Schäffner, K, Tomei, C, Vignati, M, and Zolotarova, A
Subjects: Nuclear and High Energy Physics, measurement methods, shape analysis, Cryogenic bolometer, 01 natural sciences, Particle identification, law.invention, crystal, Nuclear physics, Crystal, double-beta decay: (0neutrino), bolometer, law, Double beta decay, 0103 physical sciences, Cryogenic bolometers, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, selenium, Instrumentation, background: radioactivity, scintillation counter, Nuclear and High Energy Physic, Physics, Scintillation, 010308 nuclear & particles physics, Detector, Bolometer, zinc, Scintillation counter, Neutrinoless double-beta decay, Zinc selenide scintillator, particle identification, performance, Shape analysis (digital geometry), experimental results
Abstract: The background is the key issue of any experiment searching for the neutrinoless double beta decay (0 ν DBD) and one of the possible solutions is the use of high resolution detectors in which background can be actively discriminated. CUPID-0 is the first 0 ν DBD experiment based on scintillating bolometers able to perform efficient particle identification allowing for background reduction at the unprecedented level of ∼ 10−3 cts/(keV ⋅ kg ⋅ yr). This work makes an overview of the main problems and solutions applied in the construction of the CUPID-0 experimental apparatus, starting from the production of the crystal up to the assembly of the detector. Particular attention is payed to the methods applied to avoid the radio-contamination. The recovery of enriched Se loss along the crystal production cycle is discussed as the main challenge for the budget of this kind of experiments. The good bolometric performance of crystals is emphasized together with supplementary discrimination power offered in the case of ZnSe by the pulse shape analysis, besides the bare scintillation signal. We also make a brief report on detector performance and the results obtained till present which allowed us to establish the world best half-time limit on 82Se 0 ν DBD of >2.4 ⋅ 1024 yr (90% C.I.).
Published: 2019
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48. Performance of the low threshold Optimum Trigger on CUORE data

Author: A. Branca, D. Q. Adams, C. Alduino, K. Alfonso, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Biassoni, 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, D. Chiesa, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R. J. Creswick, A. D'Addabbo, D. D'Aguanno, I. Dafinei, C. J. Davis, F. Del Corso, S. Dell'Oro, S. Di Domizio, V. Dompè, D. Q. Fang, G. Fantini, M. Faverzani, E. Ferri, F. Ferroni, E. Fiorini, M. A. Franceschi, S. J. Freedman, B. K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, T. D. Gutierrez, K. Han, K. M. Heeger, R. G. Huang, H. Z. Huang, J. Johnston, G. Keppel, Yu. G. Kolomensky, C. Ligi, L. Ma, Y. G. Ma, L. Marini, R. H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, M. Nastasi, J. Nikkel, C. Nones, E. B. Norman, V. Novati, A. Nucciotti, I. Nutini, T. O'Donnell, J. L. Ouellet, 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, L. Taffarello, F. Terranova, C. Tomei, M. Vignati, S. L. Wagaarachchi, B. S. Wang, B. Welliver, J. Wilson, K. Wilson, L. A. Winslow, L. Zanotti, S. Zimmermann, S. Zucchelli, Branca, A, Adams, D, Alduino, C, Alfonso, K, Avignone III, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Biassoni, M, Brofferio, C, Bucci, C, Camilleri, J, Caminata, A, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Davis, C, Del Corso, F, Dell'Oro, S, Di Domizio, S, Dompè, V, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Ligi, C, Ma, L, Ma, Y, Marini, L, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nikkel, J, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O'Donnell, T, Ouellet, J, 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, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Zanotti, L, Zimmermann, S, and Zucchelli, S
Subjects: Physics, History, Particle physics, CUORE, Optimal Trigger, CUORE, low energy, dark matter, WIMP, neutrino, Computer Science Applications, Education
Abstract: The Optimum Trigger (OT) is based on a threshold algorithm applied on waveforms filtered by exploiting the matched filter technique. The OT trigger thresholds improve by 60 – 90% with respect to the thresholds obtained with the standard trigger, ranging between ~ 20 and 100 keV. Low trigger thresholds open the way to Dark Matter searches and to improvements in the neutrinoless double beta decay analysis. Nevertheless, running the OT on CUORE data is demanding from the computational resources point of view. For this reason, the algorithm has been revised and adapted to cope with CUORE data. The work done to implement OT in CUORE and its performances will be discussed.
Published: 2020
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49. Results from the Cuore Experiment

Author: Deqing Fang, Benjamin Schmidt, A. Bersani, A. Caminata, L. Zanotti, S. Copello, N. Casali, Carlo Ligi, V. Dompè, C. Pira, Carlo Cosmelli, A. Campani, C. Bucci, Paolo Carniti, Chris Alduino, A. Leder, K. Wilson, C. Pagliarone, S. Zimmermann, Oliviero Cremonesi, Lindley Winslow, L. Gironi, R. Hennings-Yeomans, F. T. Avignone, Vivek Singh, Irene Nutini, T. Wise, Giovanni Benato, Ke Han, A. Branca, C. Brofferio, N. Moggi, Reina H. Maruyama, Jeremy S. Cushman, Jonathan Ouellet, Yu-Gang Ma, Claudia Tomei, G. Bari, L. Taffarello, L. Pattavina, M. Pavan, Eric B. Norman, Lucia Canonica, N. Chott, Danielle Speller, G. Fantini, Nick Scielzo, V. Novati, V. Pettinacci, Silvio Morganti, F. Bellini, T. Napolitano, Samuele Sangiorgio, T. D. Gutierrez, F. Terranova, Stefano Dell'Oro, M. Clemenza, Stefano Pirro, D. D'Aguanno, A. Nucciotti, O. Azzolini, Barbara Wang, A. Puiu, Sergio Di Domizio, A. D'Addabbo, M. Biassoni, Davide Chiesa, S. J. Freedman, G. Keppel, C. Rosenfeld, Silvia Capelli, M. Faverzani, Y. u. G. Kolomensky, P. Gorla, Massimiliano Nastasi, Claudia Nones, F. Ferroni, Claudio Gotti, Laura Cardani, Emanuele Ferri, Milena Deninno, B. K. Fujikawa, Ettore Fiorini, J. S. Wilson, C. Rusconi, Y. Mei, Stefano Pozzi, L. Marini, C. J. Davis, Andrea Giachero, J. Johnston, Ioan Dafinei, Marco Pallavicini, M. Vignati, A. Giuliani, G. Pessina, H. Z. Huang, D. Q. Adams, Sachinthya Wagaarachchi, K. Alfonso, M. Sakai, T. O'Donnell, Xi-Guang Cao, K. M. Heeger, Luigi Cappelli, M. I. Martínez, S. Zucchelli, Monica Sisti, A. Drobizhev, Richard Creswick, M. A. Franceschi, R. G. Huang, Ezio Previtali, Bradford Welliver, 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), Département de Physique des Particules (ex SPP) (DPP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Caminata A., Adams D., Alduino C., Alfonso K., Avignone F., Azzolini O., Bari G., Bellini F., Benato G., Bersani A., Biassoni M., Branca A., Brofferio C., Bucci C., Campani A., Canonica L., Cao X.-G., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Chiesa D., Chott N., Clemenza M., Copello S., Cosmelli C., Cremonesi O., Creswick R., Cushman J., D'Addabbo A., D'Aguanno D., Dafinei I., Davis C., Dell'Oro S., Deninno M., Di Domizio S., Dompe V., Drobizhev A., Fang D.-Q., Fantini G., Faverzani M., Ferri E., Ferroni F., Fiorini E., Franceschi M.A., Freedman S., Fujikawa B., Giachero A., Gironi L., Giuliani A., Gorla P., Gotti C., Gutierrez T., Han K., Heeger K., Hennings-Yeomans R., Huang R., Huang H.Z., Johnston J., Keppel G., Kolomensky Y., Leder A., Ligi C., Ma Y.-G., Marini L., Martinez M., Maruyama R., Mei Y., Moggi N., Morganti S., Napolitano T., Nastasi M., Nones C., Norman E., Novati V., Nucciotti A., Nutini I., O'Donnell T., Ouellet J., Pagliarone C., 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., Singh V., Sisti M., Speller D., Taffarello L., Terranova F., Tomei C., Vignati M., Wagaarachchi S., Wang B., Welliver B., Wilson J., Wilson K., Winslow L., Wise T., Zanotti L., Zimmermann S., Zucchelli S., Caminata, A, Adams, D, Alduino, C, Alfonso, K, Avignone, F, Azzolini, O, Bari, G, Bellini, F, Benato, G, Bersani, A, Biassoni, M, Branca, A, Brofferio, C, Bucci, C, Campani, A, Canonica, L, Cao, X, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Chiesa, D, Chott, N, Clemenza, M, Copello, S, Cosmelli, C, Cremonesi, O, Creswick, R, Cushman, J, D’Addabbo, A, D’Aguanno, D, Dafinei, I, Davis, C, Dell’Oro, S, Deninno, M, Di Domizio, S, Dompè, V, Drobizhev, A, Fang, D, Fantini, G, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, M, Freedman, S, Fujikawa, B, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gutierrez, T, Han, K, Heeger, K, Hennings-Yeomans, R, Huang, R, Huang, H, Johnston, J, Keppel, G, Kolomensky, Y, Leder, A, Ligi, C, Ma, Y, Marini, L, Martinez, M, Maruyama, R, Mei, Y, Moggi, N, Morganti, S, Napolitano, T, Nastasi, M, Nones, C, Norman, E, Novati, V, Nucciotti, A, Nutini, I, O’Donnell, T, Ouellet, J, Pagliarone, C, 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, Singh, V, Sisti, M, Speller, D, Taffarello, L, Terranova, F, Tomei, C, Vignati, M, Wagaarachchi, S, Wang, B, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Wise, T, Zanotti, L, Zimmermann, S, Zucchelli, S, Center for Neutrino Physics, and Département de Physique des Particules (ex SPP) (DPhP)
Subjects: lcsh:QC793-793.5, CUORE, Majorana Neutrino, Neutrinoless double beta decay, lower limit, energy resolution, General Physics and Astronomy, bolometer: crystal, 01 natural sciences, 7. Clean energy, Lower limit, neutrinoless double beta decay, law.invention, Nuclear physics, Effective energy, double-beta decay: (0neutrino), Observatory, law, Double beta decay, 0103 physical sciences, talk: Kolymbari 2018/07/04, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], tellurium: lifetime, structure, 010306 general physics, Physics, 010308 nuclear & particles physics, background, lcsh:Elementary particle physics, Bolometer, neutrino: Majorana: mass, observatory, Full width at half maximum, experimental results
Abstract: The Cryogenic Underground Observatory for Rare Events (CUORE) is the first bolometric experiment searching for neutrinoless double beta decay that has been able to reach the 1-ton scale. The detector consists of an array of 988 TeO 2 crystals arranged in a cylindrical compact structure of 19 towers, each of them made of 52 crystals. The construction of the experiment was completed in August 2016 and the data taking started in spring 2017 after a period of commissioning and tests. In this work we present the neutrinoless double beta decay results of CUORE from examining a total TeO 2 exposure of 86.3 kg yr , characterized by an effective energy resolution of 7.7 keV FWHM and a background in the region of interest of 0.014 counts / ( keV kg yr ) . In this physics run, CUORE placed a lower limit on the decay half-life of neutrinoless double beta decay of 130 Te &gt, 1.3 &middot, 10 25 yr (90% C.L.). Moreover, an analysis of the background of the experiment is presented as well as the measurement of the 130 Te 2 &nu, &beta, decay with a resulting half-life of T 1 / 2 2 &nu, = [ 7.9 &plusmn, 0.1 ( stat . ) &plusmn, 0.2 ( syst . ) ] &times, 10 20 yr which is the most precise measurement of the half-life and compatible with previous results.
Published: 2018
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50. CUPID-0: the first array of enriched scintillating bolometers for 0\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\nu \beta \beta $$\end{document}νββ decay investigations

Author: O, Azzolini, M T, Barrera, J W, Beeman, F, Bellini, M, Beretta, M, Biassoni, C, Brofferio, C, Bucci, L, Canonica, S, Capelli, L, Cardani, P, Carniti, N, Casali, L, Cassina, M, Clemenza, O, Cremonesi, A, Cruciani, A, D'Addabbo, I, Dafinei, S Di, Domizio, F, Ferroni, L, Gironi, A, Giuliani, P, Gorla, C, Gotti, G, Keppel, M, Martinez, S, Morganti, S, Nagorny, M, Nastasi, S, Nisi, C, Nones, D, Orlandi, L, Pagnanini, M, Pallavicini, V, Palmieri, L, Pattavina, M, Pavan, G, Pessina, V, Pettinacci, S, Pirro, S, Pozzi, E, Previtali, A, Puiu, F, Reindl, C, Rusconi, K, Schäffner, C, Tomei, M, Vignati, and A, Zolotarova
Subjects: Special Article - Tools for Experiment and Theory
Abstract: The CUPID-0 detector hosted at the Laboratori Nazionali del Gran Sasso, Italy, is the first large array of enriched scintillating cryogenic detectors for the investigation of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{82}$$\end{document}82Se neutrinoless double-beta decay (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$0\nu \beta \beta $$\end{document}0νββ). CUPID-0 aims at measuring a background index in the region of interest (RoI) for \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$0\nu \beta \beta $$\end{document}0νββ at the level of 10\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{-3}$$\end{document}-3 counts/(keV kg years), the lowest value ever measured using cryogenic detectors. CUPID-0 operates an array of Zn\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{82}$$\end{document}82Se scintillating bolometers coupled with bolometric light detectors, with a state of the art technology for background suppression and thorough protocols and procedures for the detector preparation and construction. In this paper, the different phases of the detector design and construction will be presented, from the material selection (for the absorber production) to the new and innovative detector structure. The successful construction of the detector lead to promising preliminary detector performance which is discussed here.
Published: 2018

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