星相学蠕变过程中的晶间空化

M.A. Capano, A.S. Argon, I-W. Chen
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引用次数: 10

摘要

在0.60 ~ 0.65 Tm温度范围内,研究了γ-γ′型镍基高温合金低碳Astroloy蠕变过程中的晶间空化现象。由于晶界碳化物不论其结构如何,都能均匀地分布在所有晶界上,由此产生的空化现象也很均匀。发现空腔形核速率与平均蠕变速率成正比。在它们的生长过程中,空腔保持了球帽形状,它们的总体生长速度与无约束生长模型最相关。
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Intergranular cavitation during creep in astroloy

Intergranular cavitation during creep in low carbon Astroloy, a typical nickel-base superalloy with a γ-γ' microstructure, was studied in a temperature range of 0.60–0.65 Tm. Because the grain boundary carbides could be distributed quite uniformly on all grain boundaries regardless of their structure, cavitation which results from them was also very uniform. The cavity nucleation rate was found to be directly proportional to the average creep rate. Throughout their growth the cavities retained a spherical-caps shape and their overall growth rate correlated best with a model of unconstrained growth.

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