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热质量对溶液冷却速率及热等静压Astroloy合金部件性能的影响。

Thermal Mass Effect on the Solution Cooling Rate and on HIPped Astroloy Component Properties.

作者信息

Napal Unai Galech, Segarra Miren Aristizabal, Lazcano Borja Elguezabal, Sivo Antonio, Zubillaga Iñigo Iturriza

机构信息

CEIT-Basque Research and Technology Alliance (BRTA), Manuel Lardizabal 15, 20018 Donostia-San Sebastián, Spain.

Tecnun, Manuel Lardizabal 13, Universidad de Navarra, 20018 Donostia-San Sebastián, Spain.

出版信息

Materials (Basel). 2022 Feb 15;15(4):1434. doi: 10.3390/ma15041434.

Abstract

Astroloy is a Ni-based superalloy with high-volume fraction of γ', which gives high temperature properties but reduces its forgeability. Therefore, powder metallurgy manufacturing processes such as Near Net Shape HIPping are the most suitable manufacturing technology for Astroloy. However, NNSHIP has its own drawbacks, such as the formation of prior particle boundaries (PPBs), which usually tend to decrease material mechanical properties. The detrimental effect of PPBs can be reduced by optimizing the entire HIP processing route. Conventional HIP cycles have very low cooling rates, especially in big components from industry, and thus a series of post-heat treatments must be applied in order to achieve desirable microstructures and improve the mechanical properties. Standard heat treatments for Astroloy are long and tedious with several steps of solutioning, stabilization and precipitation. In this work, two main studies have been performed. First, the effect of the cooling rate after the solutioning treatment, which is driven by the materials' thermal mass, on the Astroloy microstructure and mechanical properties was studied. Experimental analyses and simulation techniques have been used in the present work and it has been found that higher cooling rates after solutioning increase the density of tertiary γ' precipitates by 85%, and their size decreases by 22%, which leads to an increase in hardness from 356 to 372 HB30. This hardness difference tends to reduce after subsequent standard heat treatment (HT) that homogenizes the microstructure. The second study shows the effect of different heat treatments on the microstructure and hardness of samples with two different thermal masses (can and cube). More than double the density of γ' precipitates was found in small cubes in comparison with cans with a higher thermal mass. Therefore, the hardness in cubes is between 4 and 20 HB 30 higher than in large cans, depending on the applied HT.

摘要

Astroloy是一种γ'体积分数较高的镍基高温合金,它具有高温性能,但降低了其可锻性。因此,诸如近净形热等静压(Near Net Shape HIPping)之类的粉末冶金制造工艺是最适合Astroloy的制造技术。然而,近净形热等静压有其自身的缺点,例如形成原始颗粒边界(PPBs),这通常会降低材料的机械性能。通过优化整个热等静压加工路线,可以减少PPBs的有害影响。传统的热等静压循环冷却速率非常低,尤其是在工业大型部件中,因此必须进行一系列的后续热处理,以获得理想的微观结构并改善机械性能。Astroloy的标准热处理过程漫长且繁琐,包括多个固溶处理、稳定化处理和析出处理步骤。在这项工作中,进行了两项主要研究。首先,研究了由材料热容量驱动的固溶处理后的冷却速率对Astroloy微观结构和机械性能的影响。在本工作中使用了实验分析和模拟技术,发现固溶处理后较高的冷却速率使三级γ'析出相的密度增加了85%[103],其尺寸减小了22%,这导致硬度从356 HB30增加到372 HB30。在随后使微观结构均匀化的标准热处理(HT)后,这种硬度差异趋于减小。第二项研究显示了不同热处理对具有两种不同热容量(罐形和立方体形)的样品的微观结构和硬度的影响。与热容量较高的罐形相比,在小立方体中发现γ'析出相的密度增加了一倍多。因此,根据所应用的热处理,立方体的硬度比大罐形高4至20 HB 30。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b579/8874756/43b970a92dc6/materials-15-01434-g001.jpg

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