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Incommensurate atomic density waves in the high-pressure IVb phase of barium

机译:钡的高压IVb相中的原子密度波不相称

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摘要

The host–guest structures of elements at high pressure discovered a decade ago still leave many open questions due to the lack of precise models based on full exploitation of the diffraction data. This concerns in particular Ba IV, which is stable in the range 12–45 GPa. With the example of phase Ba IVb, which is characterized here for the first time, a systematic analysis is presented of possible host–guest structure models based on high-quality single-crystal diffraction data obtained with synchrotron radiation at six different pressures between 16.5 and 19.6 GPa. It is shown that a new incommensurately modulated (IM) structure model better fits the experimental data. Unlike the composite models which are commonly reported for the Ba IV phases, the IM model reveals a density wave and its pressure-dependent evolution. The crucial role played by the selected model in the interpretation of structure evolution under pressure is discussed. The findings give a new experimental basis for a better understanding of the nature of host–guest structures.
机译:十年前发现的高压元素的主客体结构由于缺乏充分利用衍射数据的精确模型而仍然存在许多悬而未决的问题。这尤其涉及Ba IV,Ba IV在12–45 GPa范围内稳定。以首次表征的Ba IVb相为例,系统地分析了可能的主客体结构模型,这些模型基于高质量的单晶衍射数据,这些数据是通过在66.5至16.5之间的六个不同压力下用同步加速器辐射获得的。 19.6 GPa。结果表明,一个新的不相称调制(IM)结构模型更好地拟合了实验数据。与通常报道的Ba IV相的复合模型不同,IM模型揭示了密度波及其与压力有关的演化。讨论了所选模型在解释受压结构演化中的关键作用。这些发现为更好地理解宿主-客体结构的性质提供了新的实验基础。

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