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Stability of vacancy-type defect clusters in Ni based on first-principles and molecular dynamics simulations

机译:基于第一原理和分子动力学模拟的NI空置型缺陷簇的稳定性

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AbstractUsing first-principles calculations based on density-functional theory, the energetics of different vacancy-type defects, including voids, stacking fault tetrahedra (SFT) and vacancy loops, in Ni are investigated. It is found that voids are more stable than SFT at 0K, which is also the case after taking into account the volumetric strains. By carrying outab initiomolecular dynamics simulations at temperatures up to 1000K, direct transformations from vacancy loops and voids into SFT are observed. Our results suggest the importance of temperature effects in determining thermodynamic stability of vacancy clusters in face-centered cubic metals.Graphical abstractFirst-principles calculations indicate voids are more stable than SFT in a typicalfccmetal at zero temperature. Direct transformations of voids and loops to SFT are revealed at finite temperatures.Display Omitted]]>
机译:<![cdata [ 抽象 使用基于密度 - 功能理论的第一原理计算,不同空位型缺陷的能量学,包括空隙研究了NI中的堆叠故障四面体(SFT)和空缺环。结果发现,在0k时,空隙比SFT更稳定,这也是在考虑体积菌株后的情况。通过进行 AB Initio 在温度下的斜体>高达1000k的分子动力学模拟,观察到空位环和空隙的直接转换。我们的研究结果表明,温度效应在以面向中心的立方金属中确定空位簇的热力学稳定性的重要性。 图形抽象 所有“>首字母计算指示空隙比SFT更稳定,在典型的 FCC 金属处为零温度。在有限温度下显示空隙和循环到SFT的直接转换。 ]]>

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