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

机译:利用分子轨道法预测初期熔化图和Ni基超合金的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 (θ) named alloying angle. DSC thermal analysis and quantitative microstructural evaluations showed that a decrease in θ magnitude increases γ' solvus and y' 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:基于分子轨道计算,基于含有Al和TA的商业CM247 LC的实验镍基超合金在恒定的总TA + W含量(在wt%中)设计。利用该方法预测了γ'Solvus,γ/γ'共晶溶解温度及初生熔化的敏感性。在Cannon-Muskegon公司指示下进行溶液和老化处理。为了简化模型,MD和BO参数被命名合并角的新电子参数(θ)取代。 DSC热分析和定量微观结构评估表明,在溶解和老化条件下显着增加θ幅度的变量幅度增加γ'溶剂和Y'体积分数。还提出了初期熔体馏分(IMF)地图与Al和TA含量,以预测溶液治疗期间从初始熔点的安全区。结果,Al + Ta含量必须小于6wt%以达到IMF <1%。

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