2022
DOI: 10.1140/epjc/s10052-022-10720-3
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Optimization of the first CUPID detector module

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 $$^{100}$$ … Show more

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Cited by 13 publications
(13 citation statements)
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“…An example of the distribution of the L/H parameter is shown in figure 8 (left). Similar light-to-heat ratios were obtained in more recent tests of cubic LMOs with the same size [61][62][63], and in the LUMINEU and CUPID-Mo experiments realized with cylindrical LMOs [48,51,53].…”
Section: Jinst 18 P06018supporting
confidence: 81%
See 2 more Smart Citations
“…An example of the distribution of the L/H parameter is shown in figure 8 (left). Similar light-to-heat ratios were obtained in more recent tests of cubic LMOs with the same size [61][62][63], and in the LUMINEU and CUPID-Mo experiments realized with cylindrical LMOs [48,51,53].…”
Section: Jinst 18 P06018supporting
confidence: 81%
“…Despite some difference in detectors' sensitivity, we did not observe a difference in energy resolution between LMOs instrumented with standard size NTDs and the larger ones. Also, it is interesting to note that the resolution of the 2615 keV 𝛾 peak is much better than one can expect from the baseline noise values; typically a factor 2-3 difference is reported [48,51,[61][62][63]. Thus, a large part of the measured noise does not have a notable impact on the variation of the LMO thermal signal.…”
Section: Jinst 18 P06018mentioning
confidence: 96%
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“…There is a rich landscape of experiments proposed or in preparation exploiting different ββ emitters and experimental techniques. In particular, we consider LEGEND-1000 [49] for 76 Ge, SNO+II [50] for 130 Te, nEXO [51] for 136 Xe , SuperNEMO [52] for 82 Se and CUPID [53] for 100 Mo. Each of them is characterized by a set of so called performance parameters, through which both Table 4: Performance parameters assumed here for different next-generation 0νββ experiments [2] and PSF of the respective isotope [11].…”
Section: Description Of Experimental Setups and Analysismentioning
confidence: 99%
“…We process our data using the C++ softwares Apollo and Diana [37,38], first developed for the CUORE experiment and also used by CUORICINO, CUPID-0 and CUPID [39].…”
Section: Data Processingmentioning
confidence: 99%