CUORE

The Cryogenic Underground Observatory for Rare Events (CUORE) – also cuore for 'heart'; it) – is a particle physics experiment located underground at the Laboratori Nazionali del Gran Sasso in Assergi, Italy.[1][2] CUORE was designed primarily as a search for neutrinoless double beta decay in 130Te, a process that has never been observed.[3] It uses tellurium dioxide (TeO2) crystals as both the source of the decay and as bolometers to detect the resulting electrons. CUORE searches for the characteristic signal of neutrinoless double beta decay, a small peak in the observed energy spectrum around the known decay energy; for 130Te, this is Q = 2527.518 ± 0.013 keV.[4] CUORE can also search for signals from dark matter candidates, such as axions and WIMPs.[1]

An observation of neutrinoless double beta decay would conclusively show that neutrinos are Majorana fermions; that is, they are their own antiparticles.[5] This is relevant to many topics in particle physics, including lepton number conservation, nuclear structure, and neutrino masses and properties.

The CUORE collaboration involves physicists from several countries, primarily from the United States and Italy.[6] CUORE is funded by the Istituto Nazionale di Fisica Nucleare of Italy, the United States Department of Energy, and the National Science Foundation of the United States.

In September 2014, as part of the testing of the CUORE dilution refrigerator, scientists in the CUORE collaboration cooled a copper vessel with a volume of one cubic meter to 6 mK (0.006 K, −273.144 °C) for 15 days, setting a record for the lowest temperature in the known natural universe over such a large contiguous volume.[5][7][8][9]

## Contents

* 1 Detectors
* 2 History
* 3 Results
* 4 Research and development
* 5 References
* 6 External links

## Detectors

The CUORE detectors are TeO2 crystals used as low heat capacity bolometers, arranged into towers and cooled in a large cryostat to approximately 10 mK with a dilution refrigerator. The detectors are isolated from environmental thermal, electromagnetic, and other particle backgrounds by ultrapure low-radioactivity shielding. Temperature spikes from electrons emitted in Te double beta decays are collected for spectrum analysis. The detectors are calibrated using 232Th, the first element in a long decay chain that includes several prominent gamma rays up to 2615 keV.

For the construction of CUORE, the collaboration followed several procedures to minimize radioactive contamination that can cause the detectors to register background events at energies close to the energy released in neutrinoless double beta decay. The crystals were grown by the Shanghai Institute of Ceramics at the Chinese Academy of Sciences with strict radiopurity requirements.[10] The crystals are held in place by PTFE support in towers constructed from oxygen-free high thermal conductivity copper and were assembled under nitrogen inside gloveboxes in cleanrooms. Copper, lead, low-radioactivity ancient Roman lead, and borated polyethylene are used to shield the detectors. Coincidence algorithms are also used to reject events that caused multiple channels to trigger, such as would be caused by an incoming cosmic ray muon or a gamma ray that Compton scatters in multiple crystals.[11]

## History

Cuoricino was the first large-scale bolometer tower used for a rare event search and was operated from 2003 to 2008. It had 62 TeO2 crystals (11 kg of 130Te), with some crystals enriched in 130Te and others with natural isotopic abundance, and some slightly larger and some smaller crystals.[12] The tower was similar in construction to the CUORE tower, and was shielded with copper, lead, and Roman lead. Cuoricino was operated near 8 mK in a relatively small dilution refrigerator.[13]

Using the results of Cuoricino, the final details of the CUORE detector towers were finalized, and an assembly sequence was set up for the construction of these 19 towers.[13] CUORE-0 was the first detector tower produced on this assembly line. It had 52 improved TeO2 crystals in a copper tower with better surface purity and significantly reduced radon and other contamination.[14] It was operated in the Cuoricino cryostat from 2013 to 2015 as a first test of the new CUORE assembly procedures as the assembly of the CUORE towers was completed.[15]

CUORE is a scaled-up version of CUORE-0, hosted in a new custom-built cryostat capable of supporting a detector with a mass of approximately one ton. It contains 988 5×5×5 cm3 crystals, with 741 kg TeO2 (206 kg of 130Te). The new cryostat was constructed from extremely radiopure materials,[16] and a large Ancient Roman lead shield is used to shield the detectors .[17] There is a 73-ton octagonal shield outside of the cryostat, constructed of lead and borated polyethlene, to reduce the number of environmental gamma rays and neutrons reaching the detector.[16] Due to the large number of discrete detectors, cosmic ray muons can be easily excluded by rejecting events that occur simultaneously in multiple detectors.[11]

The CUORE towers were installed in the cryostat in August 2016,[18] and data taking with CUORE began in May 2017.

## Results

Cuoricino took data from April 2003 to June 2008. Final results using 19.75 kg·y of 130Te exposure set world-leading 90% limits on the 130Te 0νββ half-life of Template:Subsup > 2.8 × 1024 yr, with a background of 0.18 ± 0.01/(keV·kg·yr) near the 0νββ decay energy.[19] Axion mass limits were also set, consistent with other experiments.[20]

The first paper detailing the initial performance of CUORE-0 was published in August 2014 using data taken March to September 2013, with 7.1 kg·yr exposure, showing backgrounds reduced by a factor of 6 compared to CUORICINO and an energy resolution of 5.7 keV.[14] A limit on 0νββ was presented in April 2015, combining 9.8 kg·yr of CUORE-0 exposure with the Cuoricino exposure to set a new limit of Template:Subsup > 4.0×1024 yr.[21]

CUORE has a background goal of 0.01·counts/(keV·kg·y) in the 0νββ region of interest with an energy resolution goal of 5.0 keV. After five years, CUORE is estimated to have a 90% CL half-life sensitivity to 0νββ of 9.5 × 1025 yr, and an effective Majorana neutrino mass sensitivity of 0.05-0.13 eV (depending on the nuclear matrix elements used).[16]

First results of the full CUORE experiment were published 2018 finding no evidence for neutrinoless double beta decay setting a 90% CI Bayesian lower limit for the lifetime of Tββ0ν>1.5⋅1025 years.[22] In 2020 and 2022 new limits were given at Tββ0ν>3.2⋅1025[23] and Tββ0ν>2.2⋅1025[24][25] years at the same confidence level. In 2026, the limit was increased to Tββ0ν>3.5⋅1025 years.[26]

## Research and development

CUPID (CUORE Upgrade With Particle Identification) a research and development project for the CUORE detector.[27] Several research groups worldwide are working to develop materials for this upgrade.[28] CUPID aims to use new detector materials in the same cryostat as CUORE.

ABSuRD (A Background Surface Rejection Detector) research and development project for the CUORE detector. The project aims to develop a scintillating bolometer with the ability to veto ionizing background radiation.[29]

## References

1. ↑ 1.0 1.1 Arnaboldi, C. (2004). "CUORE: a cryogenic underground observatory for rare events". Nuclear Instruments and Methods in Physics Research Section A 518 (3): 775–798. doi:10.1016/j.nima.2003.07.067. Bibcode: 2004NIMPA.518..775A.
2. ↑ Borghino, Dario (March 31, 2018). ""CUORE" experiment seeks to get to the heart of the matter – and antimatter". NewAtlas.com. https://newatlas.com/are-neutrinos-majorana-fermions/54036/.
3. ↑ Biron, Lauren (April 23, 2015). "Extreme cold and shipwreck lead". Symmetry Magazine (Fermilab/SLAC). http://www.symmetrymagazine.org/article/april-2015/extreme-cold-and-shipwreck-lead.
4. ↑ Redshaw, Matthew; Mount, Brianna J.; Myers, Edmund G.; Avignone, Frank T. (2009). "Masses of 130Te and 130Xe and Double-β-Decay Q Value of 130Te". Physical Review Letters 102 (21). doi:10.1103/PhysRevLett.102.212502. PMID 19519099. Bibcode: 2009PhRvL.102u2502R.
5. ↑ 5.0 5.1 Shelton, Jim (October 20, 2014). "Yale systems are key to coldest cubic meter experiment". http://news.yale.edu/2014/10/20/yale-systems-are-key-coldest-cubic-meter-experiment.
6. ↑ CUORE Collaboration. "Cuore - Institutions". http://crio.mib.infn.it/wigmi/pages/cuore/institutions.php.
7. ↑ Greene, Kate (October 28, 2014). "Creating the Coldest Cubic Meter in the Universe". Berkeley Lab News Center. http://newscenter.lbl.gov/2014/10/28/creating-the-coldest-cubic-meter-in-the-universe/.
8. ↑ "CUORE: The Coldest Heart in the Known Universe". INFN Press Release. http://www.interactions.org/cms/?pid=1034217.
9. ↑ Ouellet, Jonathan (October 15, 2014). "The Coldest Cubic Meter in the Known Universe". arXiv:1410.1560 [physics.ins-det].
10. ↑ Arnaboldi, C. (2010). "Production of high purity TeO2 single crystals for the study of neutrinoless double beta decay". Journal of Crystal Growth 312 (20): 2999–3008. doi:10.1016/j.jcrysgro.2010.06.034. Bibcode: 2010JCrGr.312.2999A.
11. ↑ 11.0 11.1 Bellini, F.; Bucci, C.; Capelli, S.; Cremonesi, O.; Gironi, L.; Martinez, M.; Pavan, M.; Tomei, C. et al. (2010). "Monte Carlo evaluation of the external gamma, neutron and muon induced background sources in the CUORE experiment". Astroparticle Physics 33 (3): 169–174. doi:10.1016/j.astropartphys.2010.01.004. Bibcode: 2010APh....33..169B.
12. ↑ Andriotti, E. (2011). "130Te neutrinoless double-beta decay with CUORICINO". Astroparticle Physics 34 (11): 822–831. doi:10.1016/j.astropartphys.2011.02.002. Bibcode: 2011APh....34..822A.
13. ↑ 13.0 13.1 Arnaboldi, C. (2004). "First results on neutrinoless double beta decay of 130Te with the calorimetric CUORICINO experiment". Physics Letters B 584 (3–4): 260–268. doi:10.1016/j.physletb.2004.01.040. Bibcode: 2004PhLB..584..260A.
14. ↑ 14.0 14.1 Artusa, D. R. (2014). "Initial performance of the CUORE-0 experiment". The European Physical Journal C 74 (8). doi:10.1140/epjc/s10052-014-2956-6. Bibcode: 2014EPJC...74.2956A.
15. ↑ Greene, Kate (April 9, 2015). "For Ultra-cold Neutrino Experiment, a Successful Demonstration". http://newscenter.lbl.gov/2015/04/09/for-ultra-cold-neutrino-experiment-a-successful-demonstration/.
16. ↑ 16.0 16.1 16.2 Artusa, D. R. (2015). "Searching for Neutrinoless Double-Beta Decay of 130Te with CUORE". Advances in High Energy Physics 2015: 1–13. doi:10.1155/2015/879871.
17. ↑ Nosengo, Nicola (April 15, 2010). "Roman ingots to shield particle detector". Nature News. doi:10.1038/news.2010.186. http://www.nature.com/news/2010/100415/full/news.2010.186.html.
18. ↑ Laasch, Ricarda (2 September 2016). "CUORE almost ready for first cool-down". http://www.symmetrymagazine.org/article/cuore-almost-ready-for-first-cool-down.
19. ↑ E. Andreotti (2011). "130Te neutrinoless double-beta decay with CUORICINO". Astroparticle Physics 34 (11): 822–831. doi:10.1016/j.astropartphys.2011.02.002. Bibcode: 2011APh....34..822A.
20. ↑ Alessandria, F. (2013). "Search for 14.4 keV solar axions from M1 transition of 57Fe with CUORE crystals". Journal of Cosmology and Astroparticle Physics 2013 (5): 007. doi:10.1088/1475-7516/2013/05/007. Bibcode: 2013JCAP...05..007C.
21. ↑ Alfonso, K. (2015). "Search for Neutrinoless Double-Beta Decay of Te 130 with CUORE-0". Physical Review Letters 115 (10). doi:10.1103/PhysRevLett.115.102502. PMID 26382673. Bibcode: 2015PhRvL.115j2502A.
22. ↑ Alduino, C. et al. (2018). "First Results from CUORE: A Search for Lepton Number Violation via 0νββ Decay of Te130". Physical Review Letters 120 (13). doi:10.1103/PhysRevLett.120.132501. PMID 29694201.
23. ↑ Adams, D.Q. (26 March 2020). "Improved Limit on Neutrinoless Double-Beta Decay in 130Te with CUORE". Physical Review Letters 124 (12). doi:10.1103/PhysRevLett.124.122501. PMID 32281829. Bibcode: 2020PhRvL.124l2501A.
24. ↑ Adams, D. Q.; Alduino, C.; Alfonso, K.; Avignone, F. T.; Azzolini, O.; Bari, G.; Bellini, F.; Benato, G. et al. (April 2022). "Search for Majorana neutrinos exploiting millikelvin cryogenics with CUORE" (in en). Nature 604 (7904): 53–58. doi:10.1038/s41586-022-04497-4. ISSN 1476-4687. PMID 35388194. Bibcode: 2022Natur.604...53C.
25. ↑ Becker, Adam (2022-04-06). "CUORE team places new limits on the bizarre behavior of neutrinos" (in en-US). https://newscenter.lbl.gov/2022/04/06/cuore-team-places-new-limits-on-the-bizarre-behavior-of-neutrinos/.
26. ↑ Zhao, K. (28 January 2026). "Latest results from CUORE and prospects for CUPID". Journal of Instrumentation 21. doi:10.1088/1748-0221/21/01/C01049. https://iopscience.iop.org/article/10.1088/1748-0221/21/01/C01049. Retrieved 9 March 2026.
27. ↑ The CUPID Interest Group (2015). "CUPID: CUORE (Cryogenic Underground Observatory for Rare Events) Upgrade with Particle IDentification". arXiv:1504.03599 [physics.ins-det].
28. ↑ The CUPID Interest Group (2015). "R&D towards CUPID (CUORE Upgrade with Particle IDentification)". arXiv:1504.03612 [physics.ins-det].
29. ↑ Canonica, L. (2013). "Rejection of surface background in thermal detectors: The ABSuRD project". Nuclear Instruments and Methods in Physics Research A 732: 286–289. doi:10.1016/j.nima.2013.05.114. Bibcode: 2013NIMPA.732..286C.

## External links

* CUORE experiment record on INSPIRE-HEP
* Official CUORE Experiment page
* CUORE at LNGS
* Milan CUORE page
* Berkeley group CUORE page
* Main CUORICINO page

* v
* t
* e

Neutrino detectors, experiments, and facilities

Discoveries|

* Cowan–Reines (νe)
* Lederman–Schwartz–Steinberger (νμ)
* DONUT (ντ)
* Neutrino oscillation
* SN 1987 neutrino burst

Operating
(divided by
primary
neutrino
source)|

| Astronomical|

* ANITA
* ANTARES
* BDUNT
* Borexino
* BUST
* HALO
* IceCube
* LVD
* NEVOD
* SAGE
* Super-Kamiokande
* SNEWS

|

Reactor|

* Daya Bay
* Double Chooz
* KamLAND
* RENO
* STEREO

Accelerator|

* ICARUS (Fermilab)
* MicroBooNE
* MINERνA
* MiniBooNE
* NA61/SHINE
* NOνA
* NuMI
* T2K
* COHERENT

0νββ|

* AMoRE
* COBRA
* CUORE
* EXO
* GERDA
* KamLAND-Zen
* MAJORANA
* NEXT
* PandaX
* XMASS

Other|

* KATRIN
* WITCH

Construction|

* ANNIE
* ARA
* ARIANNA
* BEST
* DUNE
* JUNO
* KM3NeT
* SNO+
* SuperNEMO

Retired|

* AMANDA
* CDHS
* Chooz
* CNGS
* Cuoricino
* DONUT
* ERPM
* GALLEX
* Gargamelle
* GNO
* Heidelberg-Moscow
* Homestake
* ICARUS
* IGEX
* IMB
* K2K
* Kamiokande
* KARMEN
* KGF
* LSND
* MACRO
* MINOS
* MINOS+
* NARC
* NEMO
* OPERA
* RICE
* SciBooNE
* SNO
* Soudan 2
* Utah

Proposed|

* CUPID
* GRAND
* Hyper-Kamiokande
* INO
* LAGUNA
* LEGEND
* LENA
* Neutrino Factory
* nEXO
* Nucifer
* SBND
* UNO
* JEM-EUSO
* WATCHMAN

Cancelled|

* DUMAND Project
* Long Baseline Neutrino Experiment
* NEMO Project
* NESTOR Project
* SOX
* BOREX

See also|

* BNO
* Kamioka Observatory
* LNGS
* SNOLAB
* List of neutrino experiments

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