CUORE

Coordinates: 42°27′N 13°34′E / 42.450°N 13.567°E / 42.450; 13.567

The CUORE cryostat under construction in October 2014.

The Cryogenic Underground Observatory for Rare Events (CUORE, pronounced [ˈkwɔːre]) is a particle physics facility located at the Laboratori Nazionali del Gran Sasso in central Italy.[1] CUORE was designed primarily as a search for neutrinoless double beta decay (0νββ) in 130Te, a process that has never been observed.[2] 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 0νββ, a small peak in the observed energy spectrum around the known decay energy; for 130Te, this is Q = 2527.518±0.013 keV.[3] CUORE can also search for signals from dark matter candidates, such as axions and WIMPs.[1]

An observation of 0νββ would conclusively show that neutrinos are Majorana fermions; that is, they are their own antiparticles.[4] 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.[5] CUORE is funded by the Istituto Nazionale di Fisica Nucleare (INFN) of Italy, the United States Department of Energy (DOE), and the National Science Foundation (NSF) 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 universe over such a large contiguous volume.[4][6][7][8]

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.[9] 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, ancient low-radioactivity 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.[10]

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.[11] The tower was similar in construction to the CUORE tower, and was shielded with copper, lead, and Roman lead and was operated near 8 mK in a relatively small dilution refrigerator.[12]

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 203 kg TeO2. The new cryostat was constructed from extremely radiopure materials aims to improve on the sensitivity of CUORE-0 by an order of magnitude.[16] A large Roman lead shield will be used to shield the detectors as well.[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.[10] Data taking with CUORE is expected to begin in 2016.

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 T 0ν
½  > 2.8 × 1024 yr and effective Majorana mass of the neutrino of mν ≤ 710 eV, with a background of 0.18 ± 0.01/(keV·kg·yr) near the 0νββ decay energy.[18] Axion mass limits were also set, consistent with other experiments.[19]

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·y exposure, showing backgrounds reduced by a factor of 6 compared to CUORICINO and an energy resolution of 5.7 keV.[14] An 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 T 0ν
½  > 4.0×1024 yr.[20]

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 5 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 0.13 meV.[16]

Research and Development

CUPID is the "CUORE Upgrade with Particle Identification, a research and development project for the CUORE detector.[21] Several research groups worldwide are working together to develop materials for this upgrade. CUPID aims to use new detector materials in the same cryostat as CUORE.

ABSuRD is "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.[22]

References

  1. 1 2 C. Arnaboldi; et al. (CUORE Collaboration) (2004). "CUORE: a cryogenic underground observatory for rare events". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 518 (3): 775–798. arXiv:hep-ex/0212053. doi:10.1016/j.nima.2003.07.067.
  2. ↑ Biron, Lauren (April 23, 2015). "Extreme cold and shipwreck lead". Symmetry Magazine (Fermilab/SLAC). Retrieved February 19, 2016.
  3. ↑ 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). arXiv:0902.2139. doi:10.1103/PhysRevLett.102.212502. ISSN 0031-9007.
  4. 1 2 Shelton, Jim (October 20, 2014). "Yale systems are key to coldest cubic meter experiment". Yale News. Retrieved February 10, 2015.
  5. ↑ CUORE Collaboration. "Cuore - Institutions". Retrieved November 8, 2013.
  6. ↑ Greene, Kate (October 28, 2014). "Creating the Coldest Cubic Meter in the Universe". Berkeley Lab News Center. Retrieved March 11, 2015.
  7. ↑ "CUORE: The Coldest Heart in the Known Universe". INFN Press Release. Retrieved October 21, 2014.
  8. ↑ Ouellet, Jonathan (October 15, 2014). "The Coldest Cubic Meter in the Known Universe". arXiv:1410.1560 [physics.ins-det].
  9. ↑ Arnaboldi, C.; et al. (CUORE Collaboration) (October 1, 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.
  10. 1 2 Bellini, F.; Bucci, C.; Capelli, S.; Cremonesi, O.; Gironi, L.; Martinez, M.; Pavan, M.; Tomei, C.; Vignati, M. (April 1, 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.
  11. ↑ Andriotti, E.; et al. (CUORICINO Collaboration) (June 1, 2011). "130Te neutrinoless double-beta decay with CUORICINO". Astroparticle Physics 34 (11): 822–831. doi:10.1016/j.astropartphys.2011.02.002.
  12. ↑ Arnaboldi, C.; et al. (CUORICINO Collaboration) (April 1, 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.
  13. ↑ Arnaboldi, C.; Artusa, D. R.; Avignone III, F. T.; Balata, M.; Bandac, I.; Barucci, M.; Beeman, J. W.; Brofferio, C.; Bucci, C. (April 4, 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.
  14. 1 2 D. R. Artusa; et al. (CUORE Collaboration) (2014). "Initial performance of the CUORE-0 experiment". The European Physical Journal C 74 (8). arXiv:1402.0922. doi:10.1140/epjc/s10052-014-2956-6.
  15. ↑ Greene, Kate (April 9, 2015). "For Ultra-cold Neutrino Experiment, a Successful Demonstration". Retrieved 2015-04-10.
  16. 1 2 3 Artusa, D. R.; et al. (CUORE Collaboration) (2015). "Searching for Neutrinoless Double-Beta Decay of 130Te with CUORE". Advances in High Energy Physics 2015: 1–13. arXiv:1402.6072. doi:10.1155/2015/879871.
  17. ↑ Nosengo, Nicola (April 15, 2010). "Roman ingots to shield particle detector". Nature. doi:10.1038/news.2010.186.
  18. ↑ E. Andreotti; et al. (CUORE Collaboration) (2011). "130Te neutrinoless double-beta decay with CUORICINO". Astroparticle Physics 34 (11): 822–831. arXiv:1012.3266. doi:10.1016/j.astropartphys.2011.02.002.
  19. ↑ "Search for 14.4 keV solar axions from M1 transition of 57Fe with CUORE crystals". Journal of Cosmology and Astroparticle Physics 2013 (05): 007–007. 2013. arXiv:1209.2800. doi:10.1088/1475-7516/2013/05/007.
  20. ↑ Alfonso, K.; et al. (CUORE Collaboration) (2015-09-03). "Search for Neutrinoless Double-Beta Decay of Te 130 with CUORE-0". Physical Review Letters 115 (10). doi:10.1103/PhysRevLett.115.102502. ISSN 0031-9007.
  21. ↑ The CUPID Interest Group. "CUPID: CUORE (Cryogenic Underground Observatory for Rare Events) Upgrade with Particle IDentification". arxiv. Retrieved 22 March 2016.
  22. ↑ L. Canonica; et al. (December 21, 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, (subscription required (help))

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