首页> 外文会议>Advances in Computational Methods in Sciences and Engineering 2005 vol.4B; Lecture Series on Computer and Computational Sciences; vol.4B >Water Under the Extreme Conditions of Planetary Interiors: Symmetric Hydrogen Bonding in the Superionic Phase
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Water Under the Extreme Conditions of Planetary Interiors: Symmetric Hydrogen Bonding in the Superionic Phase

机译:行星内部极端条件下的水:超离子相中的对称氢键

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The predicted superionic phase of water is investigated via ab initio molecular dynamics at densities of 2.0-3.0 g/cc (34 -115 GPa) along the 2000K isotherm. We find that extremely rapid (superionic) diifusion of protons occurs in a fluid phase at pressures between 34 and 58 GPa. A transition to a stable body-centered cubic (bcc) O lattice with superionic proton conductivity is observed between 70 and 75 GPa, a much higher pressure than suggested in prior work. We find that all molecular species at pressures greater than 75 GPa are too short lived to be classified as bound states. Above 95 GPa, a transient network phase is found characterized by symmetric O-H hydrogen bonding with nearly 50% covalent character.
机译:通过从头算分子动力学沿着2000K等温线以2.0-3.0 g / cc(34 -115 GPa)的密度研究水的预测超离子相。我们发现质子在34 GPa和58 GPa之间的压力下发生了非常快速的(超离子)扩散。观察到在70至75 GPa之间过渡到具有超离子质子传导性的稳定的体心立方(bcc)O晶格,这比以前的工作所建议的压力高得多。我们发现,压力大于75 GPa的所有分子种类寿命都太短,无法归类为束缚态。高于95 GPa,发现过渡网络相的特征是对称的O-H氢键具有近50%的共价特性。

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