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地球核心中面心立方铁中的间隙氢原子。

Interstitial hydrogen atoms in face-centered cubic iron in the Earth's core.

作者信息

Ikuta Daijo, Ohtani Eiji, Sano-Furukawa Asami, Shibazaki Yuki, Terasaki Hidenori, Yuan Liang, Hattori Takanori

机构信息

Department of Earth Science, Tohoku University, Sendai, Miyagi, 980-8578, Japan.

Materials and Life Science Division, Japan Proton Accelerator Research Complex (J-PARC) Center, Japan Atomic Energy Agency, Naka, Ibaraki, 319-1195, Japan.

出版信息

Sci Rep. 2019 May 8;9(1):7108. doi: 10.1038/s41598-019-43601-z.

DOI:10.1038/s41598-019-43601-z
PMID:31068634
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6506596/
Abstract

Hydrogen is likely one of the light elements in the Earth's core. Despite its importance, no direct observation has been made of hydrogen in an iron lattice at high pressure. We made the first direct determination of site occupancy and volume of interstitial hydrogen in a face-centered cubic (fcc) iron lattice up to 12 GPa and 1200 K using the in situ neutron diffraction method. The transition temperatures from the body-centered cubic and the double-hexagonal close-packed phases to the fcc phase were higher than reported previously. At pressures <5 GPa, the hydrogen content in the fcc iron hydride lattice (x) was small at x < 0.3, but increased to x > 0.8 with increasing pressure. Hydrogen atoms occupy both octahedral (O) and tetrahedral (T) sites; typically 0.870(±0.047) in O-sites and 0.057(±0.035) in T-sites at 12 GPa and 1200 K. The fcc lattice expanded approximately linearly at a rate of 2.22(±0.36) Å per hydrogen atom, which is higher than previously estimated (1.9 Å/H). The lattice expansion by hydrogen dissolution was negligibly dependent on pressure. The large lattice expansion by interstitial hydrogen reduced the estimated hydrogen content in the Earth's core that accounted for the density deficit of the core. The revised analyses indicate that whole core may contain hydrogen of 80(±31) times of the ocean mass with 79(±30) and 0.8(±0.3) ocean mass for the outer and inner cores, respectively.

摘要

氢可能是地球核心中的轻元素之一。尽管其很重要,但尚未在高压下的铁晶格中对氢进行直接观测。我们使用原位中子衍射方法首次直接测定了面心立方(fcc)铁晶格中间隙氢的占位和体积,压力高达12 GPa,温度高达1200 K。从体心立方相和双六方密堆积相到fcc相的转变温度高于先前报道的值。在压力<5 GPa时,fcc氢化铁晶格中的氢含量(x)在x < 0.3时较小,但随着压力增加,氢含量增加到x > 0.8。氢原子占据八面体(O)和四面体(T)位置;在12 GPa和1200 K时,通常O位置为0.870(±0.047),T位置为0.057(±0.035)。fcc晶格以每个氢原子2.22(±0.36)Å的速率近似线性膨胀,这高于先前估计的值(1.9 Å/H)。氢溶解引起的晶格膨胀对压力的依赖性可忽略不计。间隙氢引起的大晶格膨胀降低了对地球核心中氢含量的估计,而该估计是用于解释核心密度亏缺的。修订后的分析表明,整个地核可能含有相当于海洋质量80(±31)倍的氢,其中外核和内核分别含有79(±30)倍和0.8(±0.3)倍的海洋质量。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0f89/6506596/fba16c61332a/41598_2019_43601_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0f89/6506596/bc3d547348e7/41598_2019_43601_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0f89/6506596/9f79e91b106f/41598_2019_43601_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0f89/6506596/3be3429534a2/41598_2019_43601_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0f89/6506596/266444065152/41598_2019_43601_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0f89/6506596/fba16c61332a/41598_2019_43601_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0f89/6506596/bc3d547348e7/41598_2019_43601_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0f89/6506596/9f79e91b106f/41598_2019_43601_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0f89/6506596/3be3429534a2/41598_2019_43601_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0f89/6506596/266444065152/41598_2019_43601_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0f89/6506596/fba16c61332a/41598_2019_43601_Fig5_HTML.jpg

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本文引用的文献

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New iron hydrides under high pressure.高压下的新型铁氢化物
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