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SABRE-North暗物质实验中NaI(Tl)探测器光学耦合材料候选研究

Investigating Optical Coupling Material Candidates in NaI(Tl) Detectors for the SABRE-North Dark Matter Experiment

Chemseddine Ananna, Gabriella Cataldi, Davide D'Angelo, Giulia D'Imperio, Maria Luisa De Giorgi, Giuseppe Di Carlo, Attilio Di Giacinto, Marcella Diemoz, Aldo Ianni, Sana Gul Khattak, Edoardo Martinenghi, Alessandro Miccoli, Marcin Misiaszek, Daniele Montanino, Valerio Pettinacci, Lidio Pietrofaccia, Shahram Rahatlou, Krzysztof Szczepaniec, Claudia Tomei, Valerio Toso, Chiara Vignoli, Samina Zuhra, Francesco Ferella, Stefano Nisi

arXiv 2610.06029首次发表:更新:

AI 中文总结

本研究为SABRE-North实验评估四种NaI(Tl)探测器光学耦合材料,测量光学透过率与放射性纯度,发现无单一材料全面最优,需进一步测试以确定最终选择。

AI 中文摘要

直接暗物质探测使用NaI(Tl)闪烁体需要超低本底材料。硅胶光学垫片若能提供足够的光学透过率和放射性纯度,可将NaI(Tl)晶体与光电倍增管(PMT)耦合。我们为SABRE-North实验表征了四种候选材料:商用EJ-560(作为参考)以及三种在萨伦托大学生产的材料(SYLGARD 184、EGel 3002 A/B和一种混合配方),采用不同的催化剂比例和固化条件,共制备十个样品。通过紫外/可见/近红外分光光度法测量了310至850 nm的光学透过率。放射性纯度在LNGS的STELLA设施使用高纯锗(HPGe)γ射线能谱法评估,对于EJ-560还使用高分辨率ICP-MS。在410 nm的NaI(Tl)发射峰处,EJ-560的吸光系数为$0.064\pm0.017$ mm$^{-1}$。本地生产的最佳样品中,SYLGARD 184(10:2基料与催化剂比例)在室温和40°C固化时分别达到$0.097\pm0.015$和$0.093\pm0.014$ mm$^{-1}$,EGel 3002(2B:A比例)在40°C固化时为$0.125\pm0.015$ mm$^{-1}$,混合配方10:1 EGel A:CataSYL在室温固化时为$0.106\pm0.014$ mm$^{-1}$。EJ-560检测到约1.8 mBq/kg的$^{232}$Th链活度,且$^{40}$K活度最高,为$(120\pm20)$ mBq/kg。本地生产的材料未检测到Th链污染,但$^{226}$Ra活度约为2.3 mBq/kg,且$^{40}$K水平较低。没有单一材料在所有标准下均最优。需要额外的ICP-MS筛查、固化垫片的HPGe测量以及直接的NaI(Tl)-PMT光产额测试,才能最终确定SABRE-North的材料选择。

英文摘要

Direct dark matter detection with NaI(Tl) scintillators requires ultra-low-background materials. Silicone optical pads can couple NaI(Tl) crystals to photomultiplier tubes (PMTs) if they provide adequate optical transmission and radiopurity. We characterize four candidate materials for the SABRE-North experiment: commercial EJ-560, used as a reference, and three materials produced at the University of Salento (SYLGARD 184, EGel 3002 A/B, and a hybrid formulation) using different catalyst ratios and curing conditions, yielding ten samples in total. Optical transmittance was measured from 310 to 850 nm by UV/Vis/NIR spectrophotometry. Radiopurity was assessed at the STELLA facility at LNGS using high-purity germanium (HPGe) $γ$-ray spectrometry and, for EJ-560, high-resolution ICP-MS. At the 410 nm NaI(Tl) emission peak, EJ-560 shows an absorbance coefficient of $0.064\pm0.017$ mm$^{-1}$. The best locally produced samples reach $0.097\pm0.015$ and $0.093\pm0.014$ mm$^{-1}$ for SYLGARD 184 with a 10:2 base-to-catalyst ratio cured at room temperature and at $40^\circ$C, respectively, $0.125\pm0.015$ mm$^{-1}$ for EGel 3002 with a 2B:A ratio cured at $40^\circ$C, and $0.106\pm0.014$ mm$^{-1}$ for the hybrid 10:1 EGel A:CataSYL formulation cured at room temperature. EJ-560 exhibits detectable $^{232}$Th-chain activity at about 1.8 mBq/kg and the highest $^{40}$K activity, $(120\pm20)$ mBq/kg. The locally produced materials show no detectable Th-chain contamination but exhibit $^{226}$Ra activities of about 2.3 mBq/kg and lower $^{40}$K levels. No single material is optimal across all criteria. Additional ICP-MS screening, HPGe measurements of cured pads, and direct NaI(Tl)-PMT light-yield tests are required for a conclusive SABRE-North material selection.

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