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Hybrid Enrichment Verification Array: Investigations of the High-Energy Gamma-Ray Signature Origin and Use for Partial Defect Detection

机译:混合富集验证阵列:高能伽玛射线特征来源和用于部分缺陷检测的研究

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The International Atomic Energy Agency is exploring the use of an Unattended Cylinder Verification Station (UCVS) to provide independent verification of the declared relative ~(235)U enrichment, ~(235)U mass and total uranium mass of the declared UF_6 cylinders moving through modern centrifuge enrichment plants. The Hybrid Enrichment Verification Array (HEVA) method is a candidate nondestructive assay method for inclusion in a UCVS. Modeling and measured data from several field campaigns have demonstrated the potential of the HEVA method to assay relative cylinder enrichment with a precision comparable to or potentially better than today's high-resolution handheld devices. The HEVA instrument is comprised of an array of sodium iodide gamma-ray detectors that measure two primary spectral components. One of these components is the traditional, direct, weakly-penetrating ~(235)U gamma-ray signature, which contains the 186-keV photopeak. The other spectral component is a nontraditional, high-energy (above ~3 MeV) gamma-ray signature, which is generated indirectly from neutrons emitted from within the UF_6 cylinder. These neutrons are more penetrating than the ~(235)U gamma-ray signature and create high-energy gamma rays through neutron capture reactions in the steel collimators surrounding the detectors and within the detector crystals. This paper will present results from Monte Carlo simulations and analyses of the HEVA method with a focus on the origins of this high-energy signature and the ability of this nontraditional signature to reveal partial-defect scenarios wherein material is missing or substituted in the interior of the cylinder.
机译:国际原子能机构正在探索使用无人值守气瓶验证站(UCVS)来提供对经过声明的UF_6气瓶的相对(〜235)U浓度,〜(235)U质量和总铀质量的声明的相对验证的独立验证现代离心浓缩厂。杂交富集验证阵列(HEVA)方法是用于UCVS的候选非破坏性测定方法。来自数个野战的建模和测量数据表明,HEVA方法具有测定相对汽缸富集的潜力,其精确度可与当今的高分辨率手持设备相媲美,甚至可能更高。 HEVA仪器由碘化钠伽马射线探测器阵列组成,可测量两个主要光谱分量。这些成分之一是传统的,直接的,穿透力很弱的〜(235)U伽玛射线特征,其中包含186keV的光电峰。另一个光谱成分是非传统的高能(约3 MeV以上)伽玛射线特征,它是由UF_6圆柱体内发射的中子间接产生的。这些中子比〜(235)U伽马射线特征更具有穿透性,并通过在探测器周围和探测器晶体内的钢准直仪中的中子俘获反应产生高能伽马射线。本文将介绍Monte Carlo模拟和HEVA方法分析的结果,重点是这种高能特征的起源以及这种非传统特征揭示部分缺陷场景的能力,在这种情况下,材料内部缺少或被替代。圆柱体。

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