Comparison of Characteristics of Gamma-Ray Imager Based on Coded Aperture by Varying the Thickness of the BGO Scintillator

IF 0.6 Q4 NUCLEAR SCIENCE & TECHNOLOGY
Seoryeong Park, M. Hammig, M. Jeong
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引用次数: 0

Abstract

Background: The conventional cerium-doped Gd2Al2Ga3O12 (GAGG(Ce)) scintillator-based gamma-ray imager has a bulky detector, which can lead to incorrect positioning of the gammaray source if the shielding against background radiation is not appropriately designed. In addition, portability is important in complex environments such as inside nuclear power plants, yet existing gamma-ray imager based on a tungsten mask tends to be weighty and therefore difficult to handle. Motivated by the need to develop a system that is not sensitive to background radiation and is portable, we changed the material of the scintillator and the coded aperture.Materials and Methods: The existing GAGG(Ce) was replaced with Bi4Ge3O12 (BGO), a scintillator with high gamma-ray detection efficiency but low energy resolution, and replaced the tungsten (W) used in the existing coded aperture with lead (Pb). Each BGO scintillator is pixelated with 144 elements (12 × 12), and each pixel has an area of 4 mm × 4 mm and the scintillator thickness ranges from 5 to 20 mm (5, 10, and 20 mm). A coded aperture consisting of Pb with a thickness of 20 mm was applied to the BGO scintillators of all thicknesses.Results and Discussion: Spectroscopic characterization, imaging performance, and image quality evaluation revealed the 10 mm-thick BGO scintillators enabled the portable gamma-ray imager to deliver optimal performance. Although its performance is slightly inferior to that of existing GAGG(Ce)-based gamma-ray imager, the results confirmed that the manufacturing cost and the system’s overall weight can be reduced.Conclusion: Despite the spectral characteristics, imaging system performance, and image quality is slightly lower than that of GAGG(Ce), the results show that BGO scintillators are preferable for gamma-ray imaging systems in terms of cost and ease of deployment, and the proposed design is well worth applying to systems intended for use in areas that do not require high precision.
不同BGO闪烁体厚度的编码孔径伽玛射线成像仪特性比较
背景:传统的掺杂铈的Gd2Al2Ga3O12 (GAGG(Ce))闪烁体伽玛射线成像仪的探测器体积庞大,如果对背景辐射的屏蔽设计不当,可能导致伽玛辐射源定位不正确。此外,便携性在核电站等复杂环境中很重要,但现有的基于钨掩模的伽马射线成像仪往往很重,因此难以处理。由于需要开发一种对背景辐射不敏感且便于携带的系统,我们改变了闪烁体的材料和编码孔径。材料与方法:用伽马射线探测效率高但能量分辨率低的闪烁体Bi4Ge3O12 (BGO)代替现有的GAGG(Ce),用铅(Pb)代替现有编码孔径中使用的钨(W)。每个BGO闪烁体像素为144个元素(12 × 12),每个像素的面积为4mm × 4mm,闪烁体厚度为5 ~ 20mm(5、10、20mm)。所有厚度的BGO闪烁体均采用厚度为20 mm的Pb编码孔径。结果和讨论:光谱表征、成像性能和图像质量评估显示,10mm厚的BGO闪烁体使便携式伽马射线成像仪具有最佳性能。虽然其性能略低于现有的基于GAGG(Ce)的伽马射线成像仪,但结果证实,制造成本和系统的整体重量可以降低。结论:尽管光谱特性、成像系统性能和图像质量略低于GAGG(Ce),但结果表明,BGO闪烁体在成本和易于部署方面更适合伽马射线成像系统,并且所提出的设计非常值得应用于不需要高精度的领域。
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来源期刊
Journal of Radiation Protection and Research
Journal of Radiation Protection and Research Physics and Astronomy-Radiation
CiteScore
1.00
自引率
0.00%
发文量
6
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