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Characterization of SABRE crystal NaI-33 with direct underground counting
by
Benziger, J
, Wallner, A
, Bignell, L J
, Stuchbery, A E
, Pietrofaccia, L
, Scutti, F
, Baroncelli, T
, Vignoli, C
, D’Imperio G
, Krishnan, S
, Tomei, C
, Bolognino, I
, Antonello, M
, Diemoz, M
, Lane, G J
, Nuti, F
, D’Angelo D
, D’Incecco M
, Dix, W
, Ianni, A
, Souza, M
, Arnquist, I J
, Suerfu, B
, Rahatlou, S
, Mould, J
, Iannone, M
, Barberio, E
, Urquijo, P
, Wada, M
, Mariani, A
, Duffy, A R
, Dafinei, I
, Milana, S
, Hoppe, E
, Di, Carlo G
, Zurowski, M
, Mahmood, I
, Orlandi, D
, Ioannucci, L
, Pettinacci, V
, Calaprice, F
, Di, Ludovico A
, Williams, A G
, Di, Giacinto A
, Zani, A
, Copello, S
in
Astrophysics
/ Contamination
/ Crystals
/ Dark matter
/ Energy
/ Energy resolution
/ Energy spectra
/ Experiments
/ Laboratories
/ Lead isotopes
/ Mass spectrometry
/ Photoelectrons
/ Radioactivity
/ Radium 226
/ Shielding
2021
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Characterization of SABRE crystal NaI-33 with direct underground counting
by
Benziger, J
, Wallner, A
, Bignell, L J
, Stuchbery, A E
, Pietrofaccia, L
, Scutti, F
, Baroncelli, T
, Vignoli, C
, D’Imperio G
, Krishnan, S
, Tomei, C
, Bolognino, I
, Antonello, M
, Diemoz, M
, Lane, G J
, Nuti, F
, D’Angelo D
, D’Incecco M
, Dix, W
, Ianni, A
, Souza, M
, Arnquist, I J
, Suerfu, B
, Rahatlou, S
, Mould, J
, Iannone, M
, Barberio, E
, Urquijo, P
, Wada, M
, Mariani, A
, Duffy, A R
, Dafinei, I
, Milana, S
, Hoppe, E
, Di, Carlo G
, Zurowski, M
, Mahmood, I
, Orlandi, D
, Ioannucci, L
, Pettinacci, V
, Calaprice, F
, Di, Ludovico A
, Williams, A G
, Di, Giacinto A
, Zani, A
, Copello, S
in
Astrophysics
/ Contamination
/ Crystals
/ Dark matter
/ Energy
/ Energy resolution
/ Energy spectra
/ Experiments
/ Laboratories
/ Lead isotopes
/ Mass spectrometry
/ Photoelectrons
/ Radioactivity
/ Radium 226
/ Shielding
2021
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Characterization of SABRE crystal NaI-33 with direct underground counting
by
Benziger, J
, Wallner, A
, Bignell, L J
, Stuchbery, A E
, Pietrofaccia, L
, Scutti, F
, Baroncelli, T
, Vignoli, C
, D’Imperio G
, Krishnan, S
, Tomei, C
, Bolognino, I
, Antonello, M
, Diemoz, M
, Lane, G J
, Nuti, F
, D’Angelo D
, D’Incecco M
, Dix, W
, Ianni, A
, Souza, M
, Arnquist, I J
, Suerfu, B
, Rahatlou, S
, Mould, J
, Iannone, M
, Barberio, E
, Urquijo, P
, Wada, M
, Mariani, A
, Duffy, A R
, Dafinei, I
, Milana, S
, Hoppe, E
, Di, Carlo G
, Zurowski, M
, Mahmood, I
, Orlandi, D
, Ioannucci, L
, Pettinacci, V
, Calaprice, F
, Di, Ludovico A
, Williams, A G
, Di, Giacinto A
, Zani, A
, Copello, S
in
Astrophysics
/ Contamination
/ Crystals
/ Dark matter
/ Energy
/ Energy resolution
/ Energy spectra
/ Experiments
/ Laboratories
/ Lead isotopes
/ Mass spectrometry
/ Photoelectrons
/ Radioactivity
/ Radium 226
/ Shielding
2021
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Characterization of SABRE crystal NaI-33 with direct underground counting
Journal Article
Characterization of SABRE crystal NaI-33 with direct underground counting
2021
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Overview
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 39K 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 226Ra and 228Th inside the crystal to be 5.9±0.6μBq/kg and 1.6±0.3μBq/kg, respectively, which would indicate a contamination from 238U and 232Th at part-per-trillion level. We measured an activity of 0.51 ± 0.02 mBq/kg due to 210Pb out of equilibrium and a 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 ∼1 count/day/kg/keV in the [5–20] keV region.
Publisher
Springer Nature B.V
Subject
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