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Energetic driving force for preferential binding of self-interstitial atoms to Fe grain boundaries over vacancies

机译:自空位原子优先优先结合到空位上的Fe晶界的能量驱动力

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摘要

Molecular dynamics simulations of 50 Fe grain boundaries were used to understand their interaction with vacancies and self-interstitial atoms, which is important for designing radiation-resistant polycrystalline materials. Site-to-site variation of formation energies within the boundary is substantial, with the majority of sites having lower formation energies than in the bulk. Comparing the vacancy and self-interstitial atom binding energies for each site shows that there is an energetic driving force for mterstitials to preferentially bind to grain boundary sites over vacancies.
机译:使用50个Fe晶界的分子动力学模拟来了解它们与空位和自填隙原子的相互作用,这对于设计耐辐射多晶材料非常重要。边界内地层能量的逐点变化是很大的,大多数位置的地层能量比整体中的低。比较每个位点的空位和自填隙原子的结合能表明,存在一种能量驱动力,使材料优先于空位而优先结合到晶界位点。

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