论文标题

Saber North的地位和前景

Status and prospects of SABRE North

论文作者

Mariani, A., Benziger, J. B., Calaprice, F., Copello, S., Dafinei, I., D'Angelo, D., D'Imperio, G., Di Carlo, G., Diemoz, M., Di Giacinto, A., Di Ludovico, A., Ianna, M., Ianni, A., Milana, S., Orlandi, D., Pettinacci, V., Pietrofaccia, L., Rahatlou, S., Suerfu, B., Tomei, C., Vignoli, C., Zani, A.

论文摘要

我们介绍了Saber North实验的低背景NAI(TL)晶体的表征。在意大利的实验室Nazionali del Gran Sasso进行了两个不同的设置中对Crystal Nai-33进行了研究。原理证明(POP)检测器配备了液体闪烁剂否决权,并收集了大约一个月(90千克$ \ times $ $天)的数据。流行干燥设置由纯粹的被动屏蔽中的NAI-33组成,并收集了将近一年的数据(891千克$ \ times $ $ $)。对于暗物质搜索的感兴趣区域(1-6 KEV)的平均背景为1.20 $ \ pm $ 0.05和1.39 $ \ pm $ 0.02计数/天/天/千克/kev和流行音乐设置。该结果为Saber North检测器的物理阶段进行了新的屏蔽设计,该设计无法预见使用有机液体闪烁体外部否决。

We present the characterization of a low background NaI(Tl) crystal for the SABRE North experiment. The crystal NaI-33, was studied in two different setups at Laboratori Nazionali del Gran Sasso, Italy. The Proof-of-Principle (PoP) detector was equipped with a liquid scintillator veto and collected data for about one month (90 kg$\times$days). The PoP-dry setup consisted of NaI-33 in a purely passive shielding and collected data for almost one year (891 kg$\times$days). The average background in the energy region of interest (1-6 keV) for dark matter search was 1.20 $\pm$ 0.05 and 1.39 $\pm$ 0.02 counts/day/kg/keV within the PoP and the PoP-dry setup, respectively. This result opens to a new shielding design for the physics phase of the SABRE North detector, that does not foresee the use of an organic liquid scintillator external veto.

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