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Influence of the initial cooling rate from γ′ supersolvus temperatures on microstructure and phase compositions in a nickel superalloy

机译:γ'Supersolvus温度对镍超合金中微结构和相组合物的初始冷却速率的影响

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摘要

Different cooling paths from a supersolvus temperature have been applied to FGH96, a polycrystalline nickel base superalloy for turbine disc applications, in order to simulate the different microstructures that exist through the thickness of a disc following an industrial heat treatment. Secondary and tertiary γ′ precipitate size distributions and morphology have been analysed and compared for the different heat treatments using SEM and atom probe tomography (APT). Detailed compositional data for both γ′ precipitate and γ matrix are presented, and compared to equilibrium compositions calculated by Thermo-Calc. For the heat-treatments studied, the secondary γ′ composition indicates a shell of differing composition to that towards the precipitate core. From sequential equilibria compositional calculations, it is suggested that the ‘shell’ forms at a lower temperature than the precipitate core. The fine tertiary precipitates do not show the core-shell compositional differences on continuous cooling. W peaks are noted at the γ/γ′ interfacial region, which is of significance for retarding coarsening. A γ′ depletion zone surrounds the secondary precipitates, within which the γ matrix composition differs significantly to the γ far-field values, Finally, a precipitate nucleation and growth mechanistic model is suggested based on the experimental data and Thermo-Calc calculations.
机译:为了模拟在工业热处理后通过盘片厚度存在的不同微观结构,已经将来自超溶剂温度的不同冷却路径应用于FGH96(一种用于涡轮盘应用的多晶镍基高温合金)。使用SEM和原子探针层析成像(APT)分析并比较了不同热处理的次生和三次生γ'沉淀物的大小分布和形态。给出了γ'沉淀物和γ基质的详细组成数据,并将其与通过Thermo-Calc计算的平衡组成进行了比较。对于所研究的热处理,次要的γ'组成表示壳的组成与朝向沉淀核的组成不同。根据顺序平衡组成计算,建议“壳”在比沉淀核更低的温度下形成。细的三次沉淀物在连续冷却时没有显示出核-壳组成的差异。在γ/γ′界面区域注意到W峰,这对于延迟粗化具有重要意义。 γ'耗尽区围绕着次生析出物,其中γ基体组成与γ远场值明显不同。最后,基于实验数据和Thermo-Calc计算,提出了析出物成核和生长机理模型。

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