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Atomistic and Kinetic Simulations of Radiation Damage in Molybdenum

机译:钼的辐射损伤原子和动力学模拟

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A new Mo potential, developed recently by using an ab initio quantum mechanics theory, was used to study formation and time evolution of radiation defects, such as self-interstitial atoms (SIAs), vacancies, and small clusters of SlAs, using molecular dynamics (MD). MD models were developed for calculation of the diffusion coefficients of vacancies, self-interstitials, and small dislocation loops containing 2 to 37 SIAs; and the rate constants were calculated. Interactions of small SIA loops with SIAs were simulated. The results show that rotation of SIA from one to another equivalent direction is an important mechanism that significantly contributes to kinetic coefficients.
机译:最近通过使用AB Initio量子力学理论而开发的新Mo潜力,用于使用分子动力学研究辐射缺陷的形成和时间演化,例如自隙缺陷(SIAS),空位和小簇,使用分子动力学( MD)。开发了MD模型,用于计算含有2至37个SIAS的空位,自隙和小型位错环的扩散系数;计算速率常数。模拟了小型SIA环与SIA的相互作用。结果表明,SIA从一个旋转到另一种等同方向是一种重要的机制,可显着贡献动力学系数。

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