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High Purity NaI(Tl) Scintillator to Search for Dark Matter

Proceedings of International Symposium on Radiation Detectors and Their Uses (ISRD2016)(2016)

University of Tokushima

Cited 8|Views27
Abstract
A high purity and large volume NaI(Tl) scintillator was developed to search for cosmic dark matter. The required densities of radioactive impurities (RIs) such as U-chain, Th-chain are less than a few ppt to establish high sensitivity to dark matter. The impurity of RIs were effectively reduced by selecting raw materials of crucible and by performing chemical reduction of lead ion in NaI raw powder. The impurity of $^{226}$Ra was reduced less than 100 $\mu$Bq/kg in NaI(Tl) crystal. It should be remarked that the impurity of $^{210}$Pb, which is difficult to reduce, is effectively reduced by chemical processing of NaI raw powder down to less than 30 $\mu$Bq/kg. The expected sensitivity to cosmic dark matter by using 250 kg of the high purity and large volume NaI(Tl) scintillator (PICO-LON; Pure Inorganic Crystal Observatory for LOw-background Neutr(al)ino) is 7$\times$10$^{-45}$ cm$^{2}$ for 50 GeV$/c^{2}$ WIMPs.
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Dark Matter
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要点】:论文介绍了开发了一种高纯度、大体积的NaI(Tl)闪烁体,以探测宇宙暗物质,并通过选择原材料及化学处理显著降低了放射性杂质,实现了对暗物质的高灵敏度。

方法】:通过精选坩埚原材料和化学还原NaI原料粉中的铅离子,有效减少了放射性杂质(如铀链、钍链)的含量。

实验】:使用高纯度NaI(Tl)晶体,$^{226}$Ra杂质降至小于100 μBq/kg,$^{210}$Pb杂质降至小于30 μBq/kg。在250 kg的高纯度NaI(Tl)闪烁体(PICO-LON)的预期灵敏度为7×10$^{-45}$ cm$^{2}$,针对50 GeV$/c^{2}$的弱相互作用大质量粒子(WIMPs)。