首页> 外文期刊>Journal of instrumentation: an IOP and SISSA journal >High-energy 3D calorimeter for use in gamma-ray astronomy based on position-sensitive virtual Frisch-grid CdZnTe detectors
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High-energy 3D calorimeter for use in gamma-ray astronomy based on position-sensitive virtual Frisch-grid CdZnTe detectors

机译:高能量3D量热计用于基于位置敏感的虚拟Frisch-Grid Cdznte探测器的伽马射线天文学

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摘要

We will present a concept for a calorimeter based on a novel approach of 3D positionsensitive virtual Frisch-grid CdZnTe (hereafter CZT) detectors. This calorimeter aims to measure photons with energies from ~100 keV to 20–50MeV. The expected energy resolution at 662 keV is better than 1% FWHM, and the photon interaction position-measurement accuracy is better than 1mm in all 3 dimensions. Each CZT bar is a rectangular prism with typical cross-section from 5 × 5 to 7 × 7mm~2 and length of 2–4 cm. The bars are arranged in modules of 4 × 4 bars, and the modules themselves can be assembled into a larger array. The 3D virtual voxel approach solves a long-standing problem with CZT detectors associated with material imperfections that limit the performance and usefulness of relatively thick detectors (i.e., > 1 cm). Also, it allows us to use the standard (unselected) grade crystals, while achieving the energy resolution of the premium detectors and thus substantially reducing the cost of the instrument. Such a calorimeter can be successfully used in space telescopes that use Compton scattering of γ-rays, such as AMEGO, serving as part of its calorimeter and providing the position and energy measurement for Compton-scattered photons (like a focal plane detector in a Compton camera). Also, it could provide suitable energy resolution to allow for spectroscopic measurements of γ-ray lines from nuclear decays.
机译:基于3D位置敏感虚拟FRISCH-GRD CDZNTE(以下CZT)探测器的新方法,我们将为热量计提出一种概念。该量热计旨在测量从〜100kev到20-50mev的能量的光子。 662keV的预期能量分辨率优于1%FWHM,光子相互作用位置 - 测量精度在所有3个维度中优于1mm。每个CZT棒是矩形棱镜,典型的横截面为5×5至7×7mm〜2和长度为2-4厘米。条形条布置在4×4巴的模块中,并且模块本身可以组装成更大的阵列。 3D虚拟体素方法解决了与材料缺陷相关的CZT探测器的长期问题,这些缺陷限制了相对较厚的探测器的性能和有用性(即> 1cm)。此外,它允许我们使用标准(未选择的)级晶体,同时实现高级探测器的能量分辨,从而大大降低了仪器的成本。这种量热计可以成功地用于使用玉米射线的康普顿散射的太空望远镜,例如Amego,作为其量热计的一部分,并为康普顿散射的光子提供位置和能量测量(如康普顿中的焦平面检测器就像焦平面检测器一样相机)。而且,它可以提供合适的能量分辨率,以允许来自核衰减的γ射线线的光谱测量。

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