Study of rare nuclear processes with CUORE

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.; Camacho, A.; Caminata, A.; Canonica, L.; Cao, X. G.; Capelli, S.; Cappelli, L.; Cardani, L.; Carniti, P.; Casali, N.; Cassina, L.; 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.; Deninno, M. M.; Domizio, S. Di; Vacri, M. L. Di; Dompè, V.; Drobizhev, A.; Fang, Deqing; Faverzani, M.; Ferri, E.; Ferroni, F.; Fiorini, E.; Franceschi, A.; Freedman, S. J.; Fujikawa, B. K.; Giachero, A.; Gironi, L.; Giuliani, A.; Gladstone, L.; Gorla, P.; Gotti, C.; Gutierrez, T. D.; Han, K.; Heeger, K. M.; Hennings‐Yeomans, R.; Huang, H. Z.; Keppel, G.; Kolomensky, Yu. G.; Leder, A.; Ligi, C.; Lim, K. E.; G., Y.; Marini, L.; Martinez, M.; Maruyama, R.; Mei, Y.; Moggi, N.; Morganti, S.; Nagorny, S.S.; Napolitano, T.; Nastasi, M.; Nones, C.; Norman, E. B.; Novati, V.; Nucciotti, A.; Nutini, I.; O’Donnell, T.; Ouellet, J. L.; Pagliarone, C.; Pallavicini, M.; Palmieri, V.; Pattavina, L.; Pavan, M.; Pessina, G.; Pira, C.; Pirro, S.; Pozzi, S.; Previtali, E.; Reindl, F.; Rosenfeld, C.; Rusconi, C.; Sakai, M.; Sangiorgio, S.; Santone, D.; Schmidt, Benjamin; Schmidt, Jonas; Scielzo, N. D.; Singh, V.; Sisti, M.; Taffarello, L.; Terranova, F.; Tomei, C.; Vignati, M.; Wagaarachchi, S. L.; Wang, B. S.; Wang, H. W.; Welliver, B.; Wilson, J. R.; Wilson, K.; Winslow, L. A.; Wise, T.; Zanotti, L.; Zhang, G. Q.; Zimmermann, S.; Zucchelli, S.

doi:10.1142/s0217751x18430029

Cited by 15 publications

(9 citation statements)

References 83 publications

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“…AMoRE [402] is an experiment devoted to determine the life-time of 100 Mo. After a first pilot run, the current status (AMoRE-I) is to test the technology with a 100 Mo mass of 5-6 kg, in order to demonstrate the scalability before moving to the full scale (AMoRE-II) detector, which will use 200 kg of material and is expected to start around 2020, with a final target sensitivity of T 0ν 1/2 5 × 10 26 yr. CUORE [403][404][405], already mentioned in section III B, works with 130 Te and is already taking data with the full scale detector, which will have as ultimate sensitivity T 0ν 1/2 9 × 10 25 yr after 5 yr of data taking [406,407]. The KamLAND-Zen experiment [38,408], after the previous successful data taking period, is now upgrading the detector for a new observation run with approximately 750 kg of 136 Xe and a new balloon inside the KamLAND detector.…”

Section: Current Generation Experimentsmentioning

confidence: 99%

Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects

Salas

Gariazzo

Mena

et al. 2018

Front. Astron. Space Sci.

193

197

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The ordering of the neutrino masses is a crucial input for a deep understanding of flavor physics, and its determination may provide the key to establish the relationship among the lepton masses and mixings and their analogous properties in the quark sector. The extraction of the neutrino mass ordering is a data-driven field expected to evolve very rapidly in the next decade. In this review, we both analyze the present status and describe the physics of subsequent prospects. Firstly, the different current available tools to measure the neutrino mass ordering are described. Namely, reactor, long-baseline (accelerator and atmospheric) neutrino beams, laboratory searches for beta and neutrinoless double beta decays and observations of the cosmic background radiation and the large scale structure of the universe are carefully reviewed. Secondly, the results from an up-to-date comprehensive global fit are reported: the Bayesian analysis to the 2018 publicly available oscillation and cosmological data sets provides strong evidence for the normal neutrino mass ordering versus the inverted scenario, with a significance of 3.5 standard deviations. This preference for the normal neutrino mass ordering is mostly due to neutrino oscillation measurements. Finally, we shall also emphasize the future perspectives for unveiling the neutrino mass ordering. In this regard, apart from describing the expectations from the aforementioned probes, we also focus on those arising from alternative and novel methods, as 21 cm cosmology, core-collapse supernova neutrinos and the direct detection of relic neutrinos.10 Here, σ 8 corresponds to the normalization of the matter power spectrum on scales of 8h −1 Mpc, see Equation (13). 11 The thermal SZ thermal effect consists on a spectral distortion on CMB photons which arrive along the line of sight of a cluster.

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Section: Current Generation Experimentsmentioning

confidence: 99%

Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects

Salas

Gariazzo

Mena

et al. 2018

Front. Astron. Space Sci.

193

197

View full text Add to dashboard Cite

show abstract

“…CUORE chose 130 Te because of its high Q ββ ¼ ð2527.518 AE 0.013Þ keV [25][26][27]-above most of the natural radioactive background-and isotopic abundance of ð34.167 AE 0.002Þ% [28], which allows cost-effective use of natural tellurium. CUORE is the culmination of decades of development of large-scale bolometric detectors [29][30][31][32][33] and its successful operation demonstrates the high potential of this technology.…”

mentioning

confidence: 99%

Improved Limit on Neutrinoless Double-Beta Decay in Te130 with CUORE

Adams¹,

Alduino²,

Alfonso³

et al. 2020

Phys. Rev. Lett.

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187

147

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“…The stable conditions provided by the cryogenics facility allowed for continued data taking with minimal human intervention and this were highly beneficial during the COVID-19 lock-down. While 0𝜈𝛽𝛽 remains the focus of the CUORE experiment, the large target mass and the ultra-low backgrounds make CUORE an excellent detector to search for exotic and rare decays [96], as well as to study the interactions of WIMPs and solar axions in the detectors described later in section 8.…”

Section: The Cuore Detector Arraymentioning

confidence: 99%

CUORE Opens the Door to Tonne-scale Cryogenics Experiments

Adams,

Alduino,

Alessandria

et al. 2021

Preprint

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The past few decades have seen major developments in the design and operation of cryogenic particle detectors. This technology offers an extremely good energy resolution -comparable to semiconductor detectors -and a wide choice of target materials, making low temperature calorimetric detectors ideal for a variety of particle physics applications. Rare event searches have continued to require ever greater exposures, which has driven them to ever larger cryogenic detectors, with the CUORE experiment being the first to reach a tonne-scale, mK-cooled, experimental mass. CUORE, designed to search for neutrinoless double beta decay, has been operational since 2017 at a temperature of about 10 mK. This result has been attained by the use of an unprecedentedly large cryogenic infrastructure called the CUORE cryostat: conceived, designed and commissioned for this purpose.In this article the main characteristics and features of the cryogenic facility developed for the CUORE experiment are highlighted. A brief introduction of the evolution of the field and of the past cryogenic facilities are given. The motivation behind the design and development of the CUORE cryogenic facility is detailed as are the steps taken toward realization, commissioning, and operation of the CUORE cryostat. The major challenges overcome by the collaboration and the solutions implemented throughout the building of the cryogenic facility will be discussed along with the potential improvements for future facilities.The success of CUORE has opened the door to a new generation of large-scale cryogenic facilities in numerous fields of science. Broader implications of the incredible feat achieved by the CUORE collaboration on the future cryogenic facilities in various fields ranging from neutrino and dark matter experiments to quantum computing will be examined.

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Study of rare nuclear processes with CUORE

Cited by 15 publications

References 83 publications

Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects

Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects

Improved Limit on Neutrinoless Double-Beta Decay in Te130 with CUORE

CUORE Opens the Door to Tonne-scale Cryogenics Experiments

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