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首页> 外文期刊>Geophysical Research Letters >Structural Transitions in MgSiO3 Glasses and Melts at the Core-Mantle Boundary Observed via Inelastic X-ray Scattering
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Structural Transitions in MgSiO3 Glasses and Melts at the Core-Mantle Boundary Observed via Inelastic X-ray Scattering

机译:Mgsio3眼镜中的结构转变并通过非弹性X射线散射观察到的芯罩边界处的熔体

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摘要

The structural adaptation in MgSiO3 melts under compression up to 130 GPa is the key to revealing the origins of the pronounced negative buoyancy of the melts at the core-mantle boundary (CMB). A full understanding of the melt densification requires study of the pressure-induced changes in the bonding configuration around oxygen at the CMB, which has proven to be difficult to measure. Here, the experimental breakthrough in O K-edge inelastic X-ray scattering enables collection of the spectra of MgSiO3 glasses up to 130 GPa, along with ab initio molecular dynamics simulations, revealing the electronic bonding transitions around heavily compressed oxygen. The spectral results indicate the emergence of denser network structures around oxygen, stemming from contractions in the Mg-O and O-O distances associated with flexible topological and short-range rearrangements around Si. The results unveil the electronic structure and thus the nature of densification in dense partial melts at the CMB.
机译:Mgsio3在压缩下熔化的结构适应高达130GPa是揭示核心 - 地幔边界(CMB)处的熔体的发音负浮力的起源的关键。全面了解熔融致密化需要研究CMB在CMB上氧气周围的粘合构型的压力诱导的变化,这已经证明难以测量。这里,O k边缘无弹性X射线散射的实验突破使得能够收集高达130GPa的MgSiO3玻璃的光谱,以及AB Initio分子动力学模拟,揭示了围绕重压氧气的电子键合转变。光谱结果表明氧气周围的密度网络结构的出现,源于与Si周围的柔性拓扑和短距离排列相关的Mg-O和O-O距离中的收缩。结果揭示了电子结构,从而揭示了CMB致密局部熔体的致密化性质。

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