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Prediction of Incipient Melting Map and γ' Features of Ni-Base Superalloys Using Molecular Orbital Method

机译:分子轨道法预测镍基高温合金的初熔图和γ'特征

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Experimental nickel-base superalloys based on commercial CM247 LC containing Al and Ta were designed at a constant total Ta + W content (in wt%), on the basis of Molecular Orbital calculation. The γ' solvus, γ/γ' eutectic dissolving temperatures and susceptibility to incipient melting during solution annealing were predicted using this method. Solutioning and aging treatment were carried out following Cannon-Muskegon Corporation indication. For simplifying the model, Md and Bo parameters were replaced by a new electronic parameter (9) named alloying angle. DSC thermal analysis and quantitative microstructural evaluations showed that a decrease in 0 magnitude increases γ' solvus and γ' volume fraction considerably in the solutionized and aged condition. Also an incipient melt fraction (IMF) map versus Al and Ta contents was presented to predict a safe zone from incipient melting point of view during solutionizing treatment. As a result, Al + Ta contents must be less than 6 wt% to reach IMF < 1%.
机译:在分子轨道计算的基础上,将基于商业CM247 LC的含有Al和Ta的实验镍基高温合金设计为恒定的Ta + W总量(重量%)。使用该方法预测了γ'固溶度,γ/γ'共熔温度和固溶退火过程中初期熔化的敏感性。按照Cannon-Muskegon Corporation的指示进行固溶和时效处理。为了简化模型,Md和Bo参数被名为合金化角的新电子参数(9)代替。 DSC热分析和定量的显微组织评估表明,在固溶和老化条件下,0值的降低会显着增加γ'固溶度和γ'体积分数。还给出了初始熔体分数(IMF)与Al和Ta含量的关系图,以从固溶处理过程中的初始熔解角度预测安全区域。结果,Al + Ta含量必须小于6 wt%才能达到IMF <1%。

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