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首页> 外文期刊>Journal of Alloys and Compounds: An Interdisciplinary Journal of Materials Science and Solid-state Chemistry and Physics >Simulation of precipitate evolution in Fe-25 Co- 15 Mo with Si addition based on computational thermodynamics
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Simulation of precipitate evolution in Fe-25 Co- 15 Mo with Si addition based on computational thermodynamics

机译:基于计算热力学的Si添加Fe-25 Co-15 Mo中析出相的模拟

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Multi-component nucleation theory is applied to decipher the precipitate evolution of solution-treated and quenched Fe-25Co-15Mo (mass%) with Si addition during continuous heating and isothermal aging. For computer simulation of the nucleation and growth kinetics of precipitates, we optimize thermody-namic model parameters of the Fe-Co-Mo system with experimental data and enthalpies of formation of ternary ferrite phase determined by density functional theory analysis. Si-solubility in the precipitation-hardening μ-phase is considered in the thermodynamic modeling. The body-centered cubic (bcc) ferrite phase reveals a metastable miS_cibility gap between Fe- and Mo-rich phase below 1033 K. Based on thermodynamic modeling of the Fe-Co-Mo system, it is shown that the alloy Fe-25Co-15Mo is located outside the spinodal region, which is in contrast to some previous work on this system. Thermo-kinetic simulations, which are validated on experimental data from atom probe tomography, propose that during aging, the first microstructures form by means of nucleation and growth of metastable bcc-precipitates before the formation of rhombohedral u-phase. For the thermokinetic analysis, we evaluate and utilize theoretically predicted nucleus compositions of bcc-precipitates from the minimum nucleation barrier concept.
机译:应用多组分成核理论,对在连续加热和等温时效中固溶处理并淬火的Fe-25Co-15Mo(质量%)的沉淀析出进行了解释。为了对沉淀物的形核和生长动力学进行计算机模拟,我们利用密度泛函理论分析确定的实验数据和三元铁素体相形成焓,优化了Fe-Co-Mo系统的热力学模型参数。在热力学模型中考虑了在沉淀硬化μ相中的Si溶解度。体心立方(bcc)铁氧体相显示在1033 K以下,富铁和富钼相之间存在亚稳态的miS_cibility间隙。基于Fe-Co-Mo系统的热力学模型,表明Fe-25Co-合金15Mo位于旋节线区域之外,这与该系统先前的一些工作形成了对比。热动力学模拟已在原子探针层析成像的实验数据上得到验证,表明在老化过程中,首先形成的微结构是通过成核和亚稳态bcc沉淀的生长在菱形U相形成之前形成的。对于热动力学分析,我们从最小成核屏障概念评估并利用了理论预测的bcc沉淀的核成分。

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