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Development of Neutron Energy Spectral Signatures for Passive Monitoring of Spent Nuclear Fuels in Dry Cask Storage

机译:被动监测干木桶贮存中乏核燃料的中子能谱特征的开发

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Demand for spent nuclear fuel dry casks as an interim storage solution has increased globally and the IAEA has expressed a need for robust safeguards and verification technologies for ensuring the continuity of knowledge and the integrity of radioactive materials inside spent fuel casks. Existing research has been focusing on “fingerprinting” casks based on count rate statistics to represent radiation emission signatures. The current research aims to expand to include neutron energy spectral information as part of the fuel characteristics. First, spent fuel composition data are taken from the Next Generation Safeguards Initiative Spent Fuel Libraries, representative for Westinghouse 17?17 PWR assemblies. The ORIGEN-S code then calculates the spontaneous fission and (α,n) emissions for individual fuel rods, followed by detailed MCNP simulations of neutrons transported through the fuel assemblies. A comprehensive database of neutron energy spectral profiles is to be constructed, with different enrichment, burn-up, and cooling time conditions. The end goal is to utilize the computational spent fuel library, predictive algorithm, and a pressurized~(4)He scintillator to verify the spent fuel assemblies inside a cask. This work identifies neutron spectral signatures that correlate with the cooling time of spent fuel. Both the total and relative contributions from spontaneous fission and (α,n) change noticeably with respect to cooling time, due to the relatively short half-life (18 years) of the major neutron source~(244)Cm. Identification of this and other neutron spectral signatures allows the characterization of spent nuclear fuels in dry cask storage.
机译:全球对乏核燃料干桶作为临时存储解决方案的需求在增加,原子能机构表示需要强有力的保障和核查技术,以确保知识和乏燃料桶内放射性物质的完整性。现有的研究一直集中在基于计数率统计来表示辐射发射特征的“指纹”桶上。当前的研究旨在扩展以将中子能谱信息作为燃料特性的一部分。首先,乏燃料成分数据来自“下一代保障计划”的乏燃料图书馆,该图书馆是西屋17-17压水堆的代表。然后,ORIGEN-S代码计算单个燃料棒的自发裂变和(α,n)排放,然后对通过燃料组件传输的中子进行详细的MCNP模拟。将建立具有不同富集,燃耗和冷却时间条件的中子能谱曲线的综合数据库。最终目标是利用计算的乏燃料库,预测算法和加压〜(4)He闪烁器来验证桶内的乏燃料组件。这项工作确定了与乏燃料冷却时间相关的中子光谱特征。由于主要中子源〜(244)Cm的半衰期相对较短(18年),自发裂变和(α,n)的总贡献和相对贡献在冷却时间方面均发生显着变化。对该中子光谱特征和其他中子光谱特征的识别可以表征干桶储存中乏核燃料的特征。

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