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首页> 外文期刊>Journal of Nuclear Materials: Materials Aspects of Fission and Fusion >Microstructural evolution of a uranium-10 wt.% molybdenum alloy for nuclear reactor fuels
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Microstructural evolution of a uranium-10 wt.% molybdenum alloy for nuclear reactor fuels

机译:用于核反应堆燃料的铀含量为10%(重量)的钼合金的微观结构演变

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摘要

Low-enriched uranium-10 wt.% molybdenum (LEU-10wt.%Mo) is of interest for the fabrication of monolithic fuels to replace highly-enriched uranium (HEU) dispersion fuels in high performance research and test reactors around the world. In this work, depleted uranium-10 wt%Mo (DU-10wt%Mo) is used to simulate the solidification and microstructural evolution of LEU-10wt%Mo. Electron backscatter diffraction (EBSD) and complementary electron probe microanalysis (EPMA) reveal significant microsegregation present in the metastable gamma-phase after solidification. Homogenization is performed at 800 and 1000 degrees C for times ranging from 1 to 32 h to explore the time temperature combinations that will reduce the extent of microsegregation, as regions of higher and lower Mo content may influence local mechanical properties and provide preferred regions for y-phase decomposition. We show for the first time that EBSD can be used to qualitatively assess microstructural evolution in DU-10wt%Mo after homogenization treatments. Complementary EPMA is used to quantitatively confirm this finding. Homogenization at 1000 degrees C for 2-4 h may the regions that contain 8 wt% Mo or lower, whereas homogenization at 1000 degrees C for longer than 8 h effectively saturates Mo chemical homogeneity, but results in substantial grain growth. The appropriate homogenization time will depend upon additional microstructural considerations, such as grain growth and intended subsequent processing. Higher carbon LEU-10wt%Mo generally contains more inclusions within the grains and at grain boundaries after solidification. The effect of these inclusions on microstructural evolution (e.g. grain growth) during homogenization and as potential y-phase decomposition nucleation sites is unclear, but likely requires additional study. Published by Elsevier B.V.
机译:低浓铀10 wt。%钼(LEU-10 wt。%Mo)对于制造整体式燃料以代替全球高性能研究和测试反应堆中的高浓铀(HEU)分散燃料具有重要意义。在这项工作中,贫铀10 wt%Mo(DU-10wt%Mo)用于模拟LEU-10wt%Mo的凝固和微观结构演变。电子背散射衍射(EBSD)和互补电子探针微分析(EPMA)显示,凝固后,亚稳态伽马相中存在明显的微偏析。均质化在800和1000摄氏度下进行1到32小时,以探索时间温度组合,这将减少微偏析的程度,因为较高和较低Mo含量的区域可能会影响局部机械性能并为y提供优选区域相分解。我们首次证明,均质化处理后,EBSD可用于定性评估DU-10wt%Mo中的微结构演变。补充EPMA用于定量确认该发现。在1000摄氏度下进行2-4小时的均质化处理可能会包含Mo含量为8 wt%或更低的区域,而在1000摄氏度下进行超过8小时的均质化处理会有效地饱和Mo化学均匀性,但会导致晶粒长大。适当的均质时间将取决于其他微观结构考虑因素,例如晶粒生长和预期的后续加工。较高的碳LEU-10wt%Mo通常在凝固后在晶粒内和晶界处包含更多的夹杂物。这些夹杂物在均质化过程中以及潜在的y相分解成核位点对微观结构演变(例如晶粒生长)的影响尚不清楚,但可能需要进一步研究。由Elsevier B.V.发布

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