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Raman micro-spectroscopy of UOX and MOX spent nuclear fuel characterization and oxidation resistance of the high burn-up structure

机译:UOX和MOX乏核燃料的拉曼光谱表征和高燃尽结构的抗氧化性

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Raman micro-spectroscopy was applied to study the structure and oxidation resistance of UO2 (burnup 60 GWd/tHM) and MOX (burnup 47 GWd/tHM) irradiated fuels. The Raman technique, adapted to working under extreme conditions, enabled structural information to be obtained at the cubic micrometer scale in various zones of interest within irradiated fuel (central and zones like the Rim for UOX60, and the plutonium-enriched agglomerates for MOX47 characterized by a high burn-up structure), and the study of their oxidation resistance. As regards the structural information after irradiation, the spectra obtained make up a set of data consistent with the systematic presence of the T-2g band characteristic of the fluorite structure, and of a triplet band located between 500 and 700 cm(-1). The existence of this triplet can be attributed to the presence of defects originating in changes to the fuel chemistry occurring in the reactor (presence of fission products) and to the accumulation of irradiation damage. As concerns the oxidation resistance of the different zones of interest, Raman spectroscopy results confirmed the good stability of the restructured zones (plutonium-enriched agglomerates and Rim) rich in fission products compared to the non-restructured UO2 grains. A greater structural stability was noticed in the case of high plutonium content agglomerates, as this element favors the maintenance of the fluorite structure. (C) 2015 Elsevier B.V. All rights reserved.
机译:拉曼光谱用于研究UO2(燃尽60 GWd / tHM)和MOX(燃耗47 GWd / tHM)辐照燃料的结构和抗氧化性。拉曼技术适合在极端条件下工作,能够在辐射燃料内的各个感兴趣区域(中心和区域,如UOX60的Rim和MOX47的the富集料)中,以立方微米尺度获得结构信息。高燃耗结构),并研究其抗氧化性。关于辐照后的结构信息,获得的光谱组成了一组数据,这些数据与系统存在的萤石结构的T-2g谱带特征和位于500至700 cm(-1)之间的三重态谱带一致。该三重态的存在可以归因于缺陷的存在,所述缺陷的存在是由于反应堆中发生的燃料化学变化(裂变产物的存在)和辐照损伤的累积所致。关于感兴趣的不同区域的抗氧化性,拉曼光谱结果证实了与未重组的UO2晶粒相比,富含裂变产物的重组区域(富lu团聚体和Rim)具有良好的稳定性。在p含量高的附聚物的情况下,观察到更大的结构稳定性,因为该元素有利于维持萤石结构。 (C)2015 Elsevier B.V.保留所有权利。

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