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Ab initio simulations of iron-nickel alloys at Earth's core conditions

机译:地球核心条件下铁镍合金的从头算模拟

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We report ab initio density functional theory calculations on iron-nickel (Fe-Ni) alloys at conditions representative of the Earth's inner core. We test different concentrations of Ni, up to ~39. wt% using ab initio lattice dynamics, and investigate the thermodynamic and vibrational stability of the three candidate crystal structures (bcc, hcp and fcc). First of all, at inner core pressures, we find that pure Fe transforms from the hcp to the fcc phase at around 6000. K. Secondly, in agreement with low pressure experiments on Fe-Ni alloys, we find the fcc structure is stabilised by the incorporation of Ni under core pressures and temperatures. Our results show that the fcc structure may, therefore, be stable under core conditions depending on the temperature in the inner core and the Ni content. Lastly, we find that within the quasi-harmonic approximation, there is no stability field for Fe-Ni alloys in the bcc structure under core conditions.
机译:我们报告了在代表地球内核的条件下对铁-镍(Fe-Ni)合金进行的从头算密度泛函理论计算。我们测试了多达39种不同浓度的Ni。重量百分数使用从头算晶格动力学,并研究三种候选晶体结构(bcc,hcp和fcc)的热力学和振动稳定性。首先,在内核压力下,我们发现纯铁在大约6000 K时从hcp转变为fcc相。其次,与在Fe-Ni合金上进行的低压实验一致,我们发现fcc结构通过以下方式稳定化: Ni在核心压力和温度下的结合。我们的结果表明,取决于内芯温度和Ni含量,fcc结构在芯条件下可能是稳定的。最后,我们发现在准谐波近似范围内,在核心条件下,bcc结构中的Fe-Ni合金没有稳定性场。

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