论文标题

测量探测器级硅用Snolab在damic的散装放射性污染

Measurement of the bulk radioactive contamination of detector-grade silicon with DAMIC at SNOLAB

论文作者

Aguilar-Arevalo, A., Amidei, D., Baxter, D., Cancelo, G., Vergara, B. A. Cervantes, Chavarria, A. E., Darragh-Ford, E., D'Olivo, J. C., Estrada, J., Favela-Perez, F., Gaïor, R., Guardincerri, Y., Hossbach, T. W., Kilminster, B., Lawson, I., Lee, S. J., Letessier-Selvon, A., Matalon, A., Mitra, P., Piers, A., Privitera, P., Ramanathan, K., Da Rocha, J., Sarkis, Y., Settimo, M., Smida, R., Thomas, R., Tiffenberg, J., Traina, M., Vilar, R., Virto, A. L.

论文摘要

我们介绍了Snolab实验中damic的高抗性硅CCD中的散装放射性核糖计师的测量。我们利用CCD的精美空间分辨率来区分$α$和$β$衰减,并以高效率地搜索各种放射性同位素序列的空间相关衰减。使用与空间相关的$β$衰减,我们在CCD中测量$^{32} $ SI的大量放射性污染,$ 140 \ pm 30 $ $ $ $ $ $ $ $ bq/kg,并在bumk $^{210} $ pb的$ <160〜μ $ bq/kg上放置上限。使用对空间相关的批量$α$衰减的类似分析,我们将$ <11 $ $ $ $ $ $ $ bq/kg(0.9 ppt)设置为$^{238} $ u,$ <7.3 $ $ $ $ $ $ $ bq/kg(1.8 ppt)$^{232} $ th。 DAMIC CCD能够识别和拒绝空间上的背景,尤其是从$^{32} $ si中识别和拒绝对下一代基于硅的暗物质实验的重大影响,其中$β$从$^{32} $ si衰减中可能是主要背景。这种能力证明了CCD技术的准备就绪,以达到KG规模的暗物质敏感性。

We present measurements of bulk radiocontaminants in the high-resistivity silicon CCDs from the DAMIC at SNOLAB experiment. We utilize the exquisite spatial resolution of CCDs to discriminate between $α$ and $β$ decays, and to search with high efficiency for the spatially-correlated decays of various radioisotope sequences. Using spatially-correlated $β$ decays, we measure a bulk radioactive contamination of $^{32}$Si in the CCDs of $140 \pm 30$ $μ$Bq/kg, and place an upper limit on bulk $^{210}$Pb of $< 160~μ$Bq/kg. Using similar analyses of spatially-correlated bulk $α$ decays, we set limits of $< 11$ $μ$Bq/kg (0.9 ppt) on $^{238}$U and of $< 7.3$ $μ$Bq/kg (1.8 ppt) on $^{232}$Th. The ability of DAMIC CCDs to identify and reject spatially-coincident backgrounds, particularly from $^{32}$Si, has significant implications for the next generation of silicon-based dark matter experiments, where $β$'s from $^{32}$Si decay will likely be a dominant background. This capability demonstrates the readiness of the CCD technology to achieve kg-scale dark matter sensitivity.

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