- Main
Lowering the Energy Threshold of the CUORE Experiment: Benefits in the Surface Alpha Events Reconstruction
- Campani, Alice;
- Adams, DQ;
- Alduino, C;
- Alfonso, K;
- Avignone, FT;
- Azzolini, O;
- Bari, G;
- Bellini, F;
- Benato, G;
- Biassoni, M;
- Branca, A;
- Brofferio, C;
- Bucci, C;
- Caminata, A;
- Canonica, L;
- Cao, XG;
- Capelli, S;
- Cappelli, L;
- Cardani, L;
- Carniti, P;
- Casali, N;
- Chiesa, D;
- Chott, N;
- Clemenza, M;
- Copello, S;
- Cosmelli, C;
- Cremonesi, O;
- Creswick, RJ;
- D’Addabbo, A;
- D’Aguanno, D;
- Dafinei, I;
- Davis, CJ;
- Dell’Oro, S;
- Di Domizio, S;
- Dompè, V;
- Fang, DQ;
- Fantini, G;
- Faverzani, M;
- Ferri, E;
- Ferroni, F;
- Fiorini, E;
- Franceschi, MA;
- Freedman, SJ;
- Fujikawa, BK;
- Giachero, A;
- Gironi, L;
- Giuliani, A;
- Gorla, P;
- Gotti, C;
- Gutierrez, TD;
- Han, K;
- Heeger, KM;
- Huang, RG;
- Huang, HZ;
- Johnston, J;
- Keppel, G;
- Kolomensky, Yu G;
- Ligi, C;
- Ma, YG;
- Ma, L;
- Marini, L;
- Maruyama, RH;
- Mei, Y;
- Moggi, N;
- Morganti, S;
- Napolitano, T;
- Nastasi, M;
- Nikkel, J;
- Nones, C;
- Norman, EB;
- Novati, V;
- Nucciotti, A;
- Nutini, I;
- O’Donnell, T;
- Ouellet, JL;
- Pagliarone, CE;
- Pagnanini, L;
- Pallavicini, M;
- Pattavina, L;
- Pavan, M;
- Pessina, G;
- Pettinacci, V;
- Pira, C;
- Pirro, S;
- Pozzi, S;
- Previtali, E;
- Puiu, A;
- Rosenfeld, C;
- Rusconi, C;
- Sakai, M;
- Sangiorgio, S;
- Schmidt, B;
- Scielzo, ND;
- Sharma, V;
- Singh, V;
- Sisti, M;
- Speller, D;
- Taffarello, L;
- Terranova, F;
- Tomei, C;
- Vignati, M;
- Wagaarachchi, SL;
- Wang, BS;
- Welliver, B;
- Wilson, J;
- Wilson, K;
- Winslow, LA;
- Zanotti, L;
- Zimmermann, S;
- Zucchelli, S
- et al.
Published Web Location
https://doi.org/10.1007/s10909-020-02487-2Abstract
CUORE is a tonne-scale cryogenic experiment located at the Laboratori Nazionali del Gran Sasso that exploits bolometric technique to search for neutrinoless double beta decay of 130Te. Thanks to its very low background and large mass, CUORE is also a powerful tool to study a broad class of phenomena, such as solar axions and WIMP scattering. The ability to conduct such sensitive searches crucially depends on the energy threshold, which has to be kept as low as possible. In this contribution, we show how the trigger algorithm affects the sensitivity to low-energy phenomena and the interpretation of the energy spectrum. In particular, we focus on the impact that the trigger algorithm has on the identification of the coincidence events among different crystals and, consequently, on the reconstruction of the background.
Many UC-authored scholarly publications are freely available on this site because of the UC's open access policies. Let us know how this access is important for you.
Main Content
Enter the password to open this PDF file:
-
-
-
-
-
-
-
-
-
-
-
-
-
-