Characterization of SABRE crystal NaI-33 with direct underground counting

Autor: Andrea Zani, S. Milana, A. Di Ludovico, C. Vignoli, Marcella Diemoz, Andrew Stuchbery, I. J. Arnquist, A. Di Giacinto, T. Baroncelli, Giulia D'imperio, F. Calaprice, Federico Scutti, D. D'Angelo, Jeremy Mould, M. Wada, G. Di Carlo, Anton Wallner, Elisabetta Luigia Barberio, Michael Souza, L. Pietrofaccia, Lindsey J. Bignell, Shahram Rahatlou, Gregory Lane, Anthony G. Williams, M. Zurowski, Andrea Mariani, D. Orlandi, S. Copello, M. Antonello, Eric W. Hoppe, Francesco Nuti, V. Pettinacci, I. Bolognino, I. Mahmood, Alan R. Duffy, Claudia Tomei, L. Ioannucci, P. Urquijo, M. Iannone, Ioan Dafinei, B. Suerfu, Aldo Ianni, S. Krishnan, W. Dix, J. Benziger, M. D'Incecco
Rok vydání: 2020
Předmět:
Zdroj: European Physical Journal C, vol 81, iss 4
European Physical Journal C: Particles and Fields, Vol 81, Iss 4, Pp 1-11 (2021)
European Physical Journal
DOI: 10.48550/arxiv.2012.02610
Popis: Ultra-pure NaI(Tl) crystals are the key element for a model-independent verification of the long standing DAMA result and a powerful means to search for the annual modulation signature of dark matter interactions. The SABRE collaboration has been developing cutting-edge techniques for the reduction of intrinsic backgrounds over several years. In this paper we report the first characterization of a 3.4 kg crystal, named NaI-33, performed in an underground passive shielding setup at LNGS. NaI-33 has a record low $$^{39}$$ 39 K contamination of 4.3 ± 0.2 ppb as determined by mass spectrometry. We measured a light yield of 11.1 ± 0.2 photoelectrons/keV and an energy resolution of 13.2% (FWHM/E) at 59.5 keV. We evaluated the activities of $$^{226}$$ 226 Ra and $$^{228}$$ 228 Th inside the crystal to be $$5.9\pm 0.6~\upmu $$ 5.9 ± 0.6 μ Bq/kg and $$1.6\pm 0.3~\upmu $$ 1.6 ± 0.3 μ Bq/kg, respectively, which would indicate a contamination from $$^{238}$$ 238 U and $$^{232}$$ 232 Th at part-per-trillion level. We measured an activity of 0.51 ± 0.02 mBq/kg due to $$^{210}$$ 210 Pb out of equilibrium and a $$\alpha $$ α quenching factor of 0.63 ± 0.01 at 5304 keV. We illustrate the analyses techniques developed to reject electronic noise in the lower part of the energy spectrum. A cut-based strategy and a multivariate approach indicated a rate, attributed to the intrinsic radioactivity of the crystal, of $$\sim $$ ∼ 1 count/day/kg/keV in the [5–20] keV region.
Databáze: OpenAIRE