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Development of a detector based on Silicon Drift Detectors for gamma-ray spectroscopy and imaging applications

机译:基于硅漂移探测器的探测器的开发,用于伽马射线光谱学和成像应用

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摘要

This work deals with the development of a new gamma detector based on Silicon Drift Detectors (SDDs) to readout large LaBr3:Ce scintillators for gamma-ray spectroscopy and imaging applications. The research is supported by the European Space Agency through the Technology Research Programme (TRP) and by Istituto Nazionale di Fisica Nucleare (INFN) within the Gamma project. The SDDs, produced at Fondazione Bruno Kessler (FBK) semiconductor laboratories, are designed as monolithic arrays of 3 x 3 units, each one of an active area of 8mm x 8mm (overall area of 26mm x 26 mm). The readout electronics and the architecture of the camera are briefly described and then first experimental results coupling the SDD array with a 1" x 1" LaBr3:Ce scintillator are reported. An energy resolution of 3% FWHM at 662 keV has been measured at -20 degrees C, better than coupling the same scintillator with a photomultiplier tube. The same scintillator is also used to evaluate position sensitivity with a 1mm collimated Cs-137 source. The main difficulty in determining the position of the gamma-ray interaction in the crystal is associated to the high thickness/diameter ratio of the crystal (1:1) and the use of reflectors on all lateral and top sides the crystal. This last choice enhances energy resolution but makes imaging capability more challenging because light is spread over all photodetectors. Preliminary results show that the camera is able to detect shifts in the measured signals, when the source is moved with steps of 5 mm. A modified version of the centroid method is finally implemented to evaluate the imaging capability of the system.
机译:这项工作涉及基于硅漂移检测器(SDD)的新型伽马探测器的开发,以读出大型LaBr3:Ce闪烁体,用于伽马射线光谱学和成像应用。该研究得到了欧洲航天局的技术研究计划(TRP)的支持,并获得了伽马项目中的纳粹科学研究院(INFN)的支持。由Fondazione Bruno Kessler(FBK)半导体实验室生产的SDD被设计为3 x 3单元的单片阵列,每个有效面积为8mm x 8mm(总面积为26mm x 26 mm)。简要描述了读出的电子设备和相机的结构,然后报告了将SDD阵列与1“ x 1” LaBr3:Ce闪烁体耦合的第一实验结果。在-20摄氏度下测量了662 keV时3%FWHM的能量分辨率,比将同一个闪烁体与光电倍增管耦合更好。同一闪烁体也可用于评估1mm准直Cs-137光源的位置灵敏度。确定晶体中伽马射线相互作用的位置的主要困难与晶体的高厚度/直径比(1:1)以及在晶体的所有侧面和顶部使用反射镜有关。最后一个选择提高了能量分辨率,但由于光会散布在所有光电探测器上,因此成像能力更具挑战性。初步结果显示,当以5毫米的步距移动光源时,摄像机能够检测到测量信号的偏移。最后实现了质心方法的改进版本,以评估系统的成像能力。

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