Exploring the keV-scale physics potential of CUORE
CUORE Collaboration: D. Q. Adams, C. Alduino, K. Alfonso, A. Armatol, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Beretta, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, J. Cao, C. Capelli, S. Capelli, L. Cappelli

TL;DR
This paper details the development of analysis techniques for CUORE to explore keV-scale physics, achieving low thresholds, background reduction, and efficiency evaluation, demonstrating CUORE's potential for rare event and dark matter searches.
Contribution
It introduces new analysis methods for keV-scale energy detection in CUORE, optimizing thresholds, background suppression, and efficiency assessment for the first time.
Findings
Achieved thresholds at 10 keV and 3 keV with low background levels.
Demonstrated the scalability of cryogenic calorimeters from keV to MeV energies.
Evaluated near-threshold reconstruction efficiencies, informing future low-energy physics searches.
Abstract
We present the analysis techniques developed to explore the keV-scale energy region of the CUORE experiment, based on more than 2 tonne yr of data collected over 5 years. By prioritizing a stricter selection over a larger exposure, we are able to optimize data selection for thresholds at 10 keV and 3 keV with 691 kg yr and 11 kg yr of data, respectively. We study how the performance varies among the 988-detector array with different detector characteristics and data taking conditions. We achieve an average baseline resolution of 2.54 0.14 keV FWHM and 1.18 0.02 keV FWHM for the data selection at 10 keV and 3 keV, respectively. The analysis methods employed reduce the overall background by about an order of magnitude, reaching 2.06 0.05 counts/(keV kg days) and 16 2 counts/(keV kg days) at the thresholds of 10 keV and 3 keV. We evaluate for the first time the…
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