集群扩展
奥氏体
材料科学
星团(航天器)
渗氮
蒙特卡罗方法
铁磁性
奥氏体不锈钢
产量(工程)
动力学蒙特卡罗方法
平面的
化学物理
热力学
动能
凝聚态物理
订单(交换)
氮气
相干势近似
冶金
化学热力学
腐蚀
微观结构
溶解度
稀土元素
化学成分
作者
Tianyu Su,Brian J. Blankenau,Namhoon Kim,Jessica A. Krogstad,Elif Ertekin
标识
DOI:10.1016/j.commatsci.2025.114218
摘要
Nitrogen (N) is a key alloying element that enhances the performance of Fe-Ni-Cr austenitic stainless steels, improving austenite stability, corrosion resistance, and yield strength. In experiments, N-rich alloys often exhibit planar slip, suggesting microstructural changes associated with local chemical order. However, theoretical analysis of the N effects on chemical ordering, particularly short-range order (SRO) and long-range order (LRO), is complicated by the multisublattice structure and magnetic interactions in these alloys. In this work, we combine first-principles calculations with the spin cluster expansion (spin CE) method to systematically investigate the effects of N on chemical ordering in Fe-Ni-Cr alloys. Our atomistic models confirm a strong affinity between N and Cr, which drives the formation of N-Cr SRO and, at higher N concentrations, stabilizes M 4 N-type ordered phases (M = metal). Monte Carlo simulations reveal that low N concentrations promote local N-Cr or N-N SRO, while increasing N content leads to the emergence of Cr- and N-rich LRO structures. We also show that the presence of N suppresses intrinsic Fe-Cr and Ni-Cr SRO by competing with these interactions, particularly at high concentrations. The impact of Cr content on ordering diminishes as N approaches its solubility limit. These findings are consistent with experimental observations in high-N austenitic steels. Finally, we discuss the influence of kinetic and magnetic effects on SRO evolution in high-N alloys. This study provides a comprehensive framework for understanding N-driven chemical ordering and offers insights into microstructural changes during nitriding processes.
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