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arXiv 1502.07381cond-mat.mtrl-sci
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高压下稳定的过氧化镁

Stable magnesium peroxide at high pressure

Sergey S. Lobanov, Qiang Zhu, Nicholas Holtgrewe, Clemens Prescher, Vitali B. Prakapenka, Artem R. Oganov, Alexander F. Goncharov

摘要:

岩石行星被认为是由Mg和O的化合物组成的,因为它们是最丰富的元素之一,但对其稳定相的了解可能是不完整的。已知MgO对非常高的压力非常稳定,并且在地球下地幔的还原条件下具有化学惰性。然而,在“冰冷的”气体巨星以及系外行星中,氧可能是一种更丰富的成分(参考文献1,2)。在这里,使用同步加速器X射线衍射在激光加热的金刚石对顶砧单元,我们表明,MgO和氧气反应在94 GPa以上的压力和T = 2150 K与理论预测的I4/mcm MgO 2的形成(参考文献3)。拉曼光谱检测的过氧化物离子(O22-)的合成材料中的存在,以及在回收的标本。同样,能量色散X射线光谱证实,回收的样品具有比纯MgO更高的氧含量。我们的发现表明,在高氧化条件下,MgO 2可能取代MgO的岩石地幔和岩石行星的核心。

英文摘要:

Rocky planets are thought to comprise compounds of Mg and O as these are among the most abundant elements, but knowledge of their stable phases may be incomplete. MgO is known to be remarkably stable to very high pressure and chemically inert under reduced condition of the Earth's lower mantle. However, in 'icy' gas giants as well as in exoplanets oxygen may be a more abundant constituent (Ref. 1,2). Here, using synchrotron x-ray diffraction in laser-heated diamond anvil cells, we show that MgO and oxygen react at pressures above 94 GPa and T = 2150 K with the formation of the theoretically predicted I4/mcm MgO2 (Ref.3). Raman spectroscopy detects the presence of a peroxide ion (O22-) in the synthesized material as well as in the recovered specimen. Likewise, energy-dispersive x-ray spectroscopy confirms that the recovered sample has higher oxygen content than pure MgO. Our finding suggests that MgO2 may substitute MgO in rocky mantles and rocky planetary cores under highly oxidizing conditions.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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