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TRANSFORMATION OF STISHOVITE TO A DENSER PHASE AT LOWER-MANTLE PRESSURES

机译:在较低地幔压力下钛辉石转变成密度阶段

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WHETHER stishovite, the highest-pressure polymorph of SiO2 known from natural samples, transforms to a denser structure at higher pressures has long been of interest. A suggested transition from rutile to the CaCl2 structure driven by a vibrational-mode instability(1) was supported by the observation of a frequency decrease (softening) of a Raman mode with increasing pressure(2). Subsequent X-ray diffraction measurements provided evidence(3) for stability of the CaCl2 phase near 100 GPa. Electronic-structure calculations predict, however, that the transition occurs at much lower pressure, where a shear modulus vanishes and before the Raman mode softens completely(4). Here we use in situ Raman spectroscopy and a new theoretical model to investigate the high-pressure behaviour of stishovite. At 50 GPa, the pressure dependence of the soft B-1g mode abruptly changes and the E(g) mode splits, as predicted for transformation to the CaCl2 structure. Our results demonstrate that any free silica in the deep mantle (below 1,200-1,500 km) will exist in the CaCl2 structure at considerably lower pressures than previously thought(3). [References: 30]
机译:然而,从天然样品中已知的最高压力的SiO2多晶型的辉石,在较高的压力下转变为致密的结构早已引起人们的关注。观察到随着压力增加拉曼模式的频率降低(软化),支持了由振动模式不稳定性驱动的金红石型向CaCl2结构的转变(1)。随后的X射线衍射测量为CaCl2相在100 GPa附近的稳定性提供了证据(3)。然而,电子结构计算预测该转变发生在低得多的压力下,在该压力下剪切模量消失并且在拉曼模式完全软化之前(4)。在这里,我们使用原位拉曼光谱和一个新的理论模型来研究stishovite的高压行为。在50 GPa时,软B-1g模式的压力依赖性突然改变,并且E(g)模式分裂,正如预测的转变为CaCl2结构一样。我们的结果表明,在深层地幔中(1200-1500 km以下)的任何游离二氧化硅将以比以前认为的低得多的压力存在于CaCl2结构中(3)。 [参考:30]

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