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The role of Al-defects on the equation of state of Al-(Mg,Fe)SiO3 perovskite

机译:Al缺陷对Al-(Mg,Fe)SiO3钙钛矿状态方程的作用

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摘要

We performed compression curves of aluminous silicate perovskite (Al-Pv) synthesized under various conditions of pressure, temperature and MgO or SiO2 activities, using laser-heated diamond anvil cell at the ESRF (Grenoble). We refined bulk moduli (KO) from 235 to 270 GPa, in agreement with the wide range of values reported in the literature. We observe that Al-Pv phase synthesized at high temperature, in the SiO2-rich system, is more compressible than Al-Pv phase synthesized at high pressure, in the MgO-rich system. As suggested by various authors, the resolution of this controversy rests on a better understanding of the crystal chemistry of Al in perovskite, which involves at least two competitive mechanisms, substitution of Si in the octahedral site only, or a coupled substitution on both Mg and Si sites. The vacancy mechanism is expected to reduce the K-0 significantly, due to the presence of oxygen vacancies. All compression curves performed in this study can be explained by considering that the vacancy mechanism is favored at high temperatures and that the coupled mechanism is favored at high pressures. These trends agree well with previous reports. For (Mg,Fe)(Si,A1)O-3 perovskite compositions relevant to the lower mantle, the two previous reports and our new data set for a MORB-type perovskite phase agree well with each other with higher K-0 values between 260 and 270 GPa, compared with K-0=253 GPa for the pure MgSiO3 phase suggested from previous studies. In these compounds, coupled substitution of Al3+ and Fe3+ cations leads to a well constrained crystal chemistry. Therefore, the low K-0 value observed in some of the previous studies for Fe-free Al-Pv is likely to be irrelevant for mantle perovskite. Some questions may remain only for the mantle region just below the 670 km discontinuity, where pressures remain moderate, thus potentially allowing for at most 2% of oxygen vacancies. However, it is clear that using low K-0 values to extrapolate to greater depths is unjustified. (c) 2007 Elsevier B.V. All rights reserved.
机译:我们使用ESRF(格勒诺布尔)的激光加热金刚石砧盒,在压力,温度和MgO或SiO2活性的各种条件下合成了铝硅酸盐钙钛矿(Al-Pv)的压缩曲线。我们将体积模量(KO)从235 GPa精炼到270 GPa,与文献中报道的各种数值相一致。我们观察到,在富含SiO2的系统中,高温合成的Al-Pv相比在富含MgO的系统中,高压合成的Al-Pv相具有更高的可压缩性。正如不同作者所建议的那样,解决这一争议的方法在于更好地理解钙钛矿中Al的晶体化学,这涉及至少两种竞争机制,即仅在八面体位点取代Si,或同时在Mg和Mg上耦合取代。硅站点。由于存在氧空位,因此空位机制有望显着降低K-0。可以通过考虑高温下有利于空位机理以及高压下有利于偶合机理来解释本研究中进行的所有压缩曲线。这些趋势与以前的报告非常吻合。对于与下地幔有关的(Mg,Fe)(Si,A1)O-3钙钛矿组成,先前的两个报告和我们关于MORB型钙钛矿相的新数据集彼此吻合,K-0值在先前研究表明,纯MgSiO3相为260和270 GPa,而K-0 = 253 GPa。在这些化合物中,Al3 +和Fe3 +阳离子的偶联取代导致良好的晶体化学约束。因此,在先前的一些研究中观察到的无铁Al-Pv的低K-0值可能与地幔钙钛矿无关。某些问题可能只存在于670 km不连续点以下的地幔区域,那里的压力仍处于中等水平,因此可能最多允许2%的氧空位。但是,很明显,使用低K-0值推断到更大的深度是不合理的。 (c)2007 Elsevier B.V.保留所有权利。

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