Effect of chemistry on the compressibility and high-pressure structural evolution of the CaFe2O4-type aluminous silicate phase

IF 2.4 3区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Giacomo Criniti , Tiziana Boffa Ballaran , Alexander Kurnosov , Takayuki Ishii , Elena-Marie Rogmann , Konstantin Glazyrin , Timofey Fedotenko , Daniel J. Frost
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引用次数: 0

Abstract

Approximately 22–26 vol% of a basaltic phase assemblage at lower mantle conditions is comprised of a (Na,Mg,Fe2+)(Al,Si,Fe3+)2O4 phase with CaFe2O4-type (CF-type) structure. Previous experimental studies attempted to determine the equation of state of the CF-type phase but reported contrasting compressibility values, even for samples with the same composition. Therefore, the elastic properties of the CF-type phase remain, to date, largely unconstrained. Here, we conducted single-crystal X-ray diffraction (SCXRD) measurements in the diamond anvil cell (DAC) at high pressure and room temperature on three samples of CF-type phase with compositions Na0.90(1)Al1.03(2)Si1.00(2)O4 (NaCF), Na0.66(4)Mg0.28(4)Al1.22(3)Si0.78(3)O4 (MgCF) and Na0.62(2)Mg0.19(1)Fe2+0.17(1)Fe3+0.080(4)Al1.20(3)Si0.70(1)O4 (FeCF). A multi-sample loading approach was employed for most DAC runs, where two samples were loaded in the same sample chamber to reduce possible systematic deviations between datasets, thus enhancing internal consistency and corroborating data reproducibility. Experiments on the NaCF and MgCF samples were conducted up to ∼50 GPa, while the FeCF sample was compressed to ∼72 GPa to better characterize the effect of the spin crossover of octahedrally coordinated Fe3+. We found the isothermal bulk modulus (KT0) to increase with decreasing NaAlSiO4 content, accompanied by only a slight decrease in its pressure derivative (K'T0). Analysis of the crystal structures of the three samples at high pressure allowed compositional trends to be determined also for the interatomic bonds and polyhedral compressibility, as well as the distortion indices. These suggest an overall stiffening of the A site with increasing Mg2+ and Fe2+ content, as well of the two B sites with increasing Al3+ and Fe3+ content. Enhanced compressibility of the unit cell and octahedral B sites was observed between ∼26–42 GPa in the FeCF sample, suggesting a pressure-induced spin crossover of Fe3+, in agreement with some previous observations. Finally, trends in the elastic properties from experimental studies conducted along the NaAlSiO4-MgAl2O4 join are discussed and used as a proxy to evaluate the reliability of end-member properties for the CF-type phase employed in most recent mineral physical and thermodynamic databases. Our analysis suggests current mineral physical models might underestimate densities and overestimate bulk sound velocities of NaAlSiO4-rich CF-type phases with basaltic composition.

Abstract Image

化学对cafe2o4型硅酸铝相可压缩性及高压结构演化的影响
下地幔条件下玄武岩相组合约22-26 vol%由(Na,Mg,Fe2+)(Al,Si,Fe3+)2O4相组成,具有cafe2o4型(cf型)结构。先前的实验研究试图确定cf型相的状态方程,但报告了相反的压缩率值,即使是相同成分的样品。因此,迄今为止,cf型相的弹性特性在很大程度上是不受约束的。本文在金刚石顶孔(DAC)中对三种成分为Na0.90(1)Al1.03(2)Si1.00(2)O4 (NaCF)、Na0.66(4)Mg0.28(4)Al1.22(3)Si0.78(3)O4 (MgCF)和Na0.62(2)Mg0.19(1)Fe2+0.17(1)Fe3+0.080(4)Al1.20(3)Si0.70(1)O4 (FeCF)的cf型相样品进行了高压和室温下的单晶x射线衍射(SCXRD)测量。大多数DAC运行采用多样本加载方法,其中两个样本加载在同一个样本室中,以减少数据集之间可能的系统偏差,从而增强内部一致性和确证数据的可重复性。在NaCF和MgCF样品上进行了高达~ 50 GPa的实验,而FeCF样品被压缩到~ 72 GPa,以更好地表征八面体配位Fe3+自旋交叉的影响。我们发现等温体积模量(KT0)随着NaAlSiO4含量的降低而增加,而其压力导数(KT0)仅略有下降。对这三种样品在高压下的晶体结构进行分析,还可以确定原子间键和多面体可压缩性以及畸变指数的组成趋势。这表明随着Mg2+和Fe2+含量的增加,A位点整体变硬,随着Al3+和Fe3+含量的增加,两个B位点整体变硬。在FeCF样品中,在~ 26-42 GPa之间观察到单位细胞和八面体B位点的可压缩性增强,这表明Fe3+存在压力诱导的自旋交叉,与之前的一些观察结果一致。最后,讨论了沿NaAlSiO4-MgAl2O4连接处进行的实验研究的弹性特性趋势,并将其用作评估cf型相端元特性可靠性的代理,这些特性用于最新的矿物物理和热力学数据库中。我们的分析表明,目前的矿物物理模型可能低估了含有玄武岩成分的富含naalsio4的cf型相的密度和体声速。
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来源期刊
Physics of the Earth and Planetary Interiors
Physics of the Earth and Planetary Interiors 地学天文-地球化学与地球物理
CiteScore
5.00
自引率
4.30%
发文量
78
审稿时长
18.5 weeks
期刊介绍: Launched in 1968 to fill the need for an international journal in the field of planetary physics, geodesy and geophysics, Physics of the Earth and Planetary Interiors has now grown to become important reading matter for all geophysicists. It is the only journal to be entirely devoted to the physical and chemical processes of planetary interiors. Original research papers, review articles, short communications and book reviews are all published on a regular basis; and from time to time special issues of the journal are devoted to the publication of the proceedings of symposia and congresses which the editors feel will be of particular interest to the reader.
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