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Crystal structures of (Mg1-xFex)SiO3postperovskite at high pressures

机译:(Mg1-xFex)SiO3钙钛矿在高压下的晶体结构

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摘要

X-ray diffraction experiments on postperovskite (ppv) with compositions (Mg0.9Fe0.1)SiO3 and (Mg0.6Fe0.4)SiO3 at Earth core-mantle boundary pressures reveal different crystal structures. The former adopts the CaIrO3-type structure with space group Cmcm, whereas the latter crystallizes in a structure with the Pmcm (Pmma) space group. The latter has a significantly higher density (ρ = 6.119(1) g/cm3) than the former (ρ = 5.694(8) g/cm3) due to both the larger amount of iron and the smaller ionic radius of Fe2+ as a result of an electronic spin transition observed by X-ray emission spectroscopy (XES). The smaller ionic radius for low-spin compared to high-spin Fe2+ also leads to an ordered cation distribution in the M1 and M2 crystallographic sites of the higher density ppv structure. Rietveld structure refinement indicates that approximately 70% of the total Fe2+ in that phase occupies the M2 site. XES results indicate a loss of 70% of the unpaired electronic spins consistent with a low spin M2 site and high spin M1 site. First-principles calculations of the magnetic ordering confirm that Pmcm with a two-site model is energetically more favorable at high pressure, and predict that the ordered structure is anisotropic in its electrical and elastic properties. These results suggest that interpretations of seismic structure in the deep mantle need to treat a broader range of mineral structures than previously considered.
机译:在地核-地幔边界压力下对钙钛矿型(ppv)组成为(Mg0.9Fe0.1)SiO3和(Mg0.6Fe0.4)SiO3的X射线衍射实验揭示了不同的晶体结构。前者采用具有Cmcm空间群的CaIrO3型结构,而后者则结晶成具有Pmcm(Pmma)空间群的结构。后者的密度(ρ= 6.119(1)g / cm 3 )明显高于前者(ρ= 5.694(8)g / cm 3 ),原因是X射线发射光谱法(XES)观察到电子自旋跃迁的结果表明,铁的含量较高且Fe 2 + 的离子半径较小。与高旋转的Fe 2 + 相比,低旋转的离子半径更小,从而在较高密度ppv结构的M1和M2晶体学位点中导致有序的阳离子分布。 Rietveld结构的细化表明,该相中大约70%的Fe 2 + 占据了M2位置。 XES结果表明,与低自旋M2位点和高自旋M1位点一致的未配对电子自旋损失70%。磁有序的第一性原理计算证实,具有两点模型的Pmcm在高压下在能量上更有利,并预测有序结构的电和弹性性质是各向异性的。这些结果表明,深部地幔中地震结构的解释需要处理比以前考虑的更广泛的矿物结构。

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