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Probing local and electronic structure in Warm Dense Matter: single pulse synchrotron x-ray absorption spectroscopy on shocked Fe

机译:探测热致密物质中的局部和电子结构:冲击铁上的单脉冲同步加速器X射线吸收光谱

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摘要

Understanding Warm Dense Matter (WDM), the state of planetary interiors, is a new frontier in scientific research. There exists very little experimental data probing WDM states at the atomic level to test current models and those performed up to now are limited in quality. Here, we report a proof-of-principle experiment that makes microscopic investigations of materials under dynamic compression easily accessible to users and with data quality close to that achievable at ambient. Using a single 100 ps synchrotron x-ray pulse, we have measured, by K-edge absorption spectroscopy, ns-lived equilibrium states of WDM Fe. Structural and electronic changes in Fe are clearly observed for the first time at such extreme conditions. The amplitude of the EXAFS oscillations persists up to 500 GPa and 17000 K, suggesting an enduring local order. Moreover, a discrepancy exists with respect to theoretical calculations in the value of the energy shift of the absorption onset and so this comparison should help to refine the approximations used in models.
机译:了解温暖致密物质(WDM)是行星内部的状态,是科学研究的新领域。几乎没有在原子级别上探测WDM状态以测试当前模型的实验数据,并且迄今为止执行的实验质量有限。在这里,我们报告了一项原理验证实验,该实验使用户可以轻松地对动态压缩下的材料进行微观研究,并且数据质量接近在环境下可获得的数据质量。使用单个100 ps同步加速器X射线脉冲,我们通过K边吸收光谱法测量了WDM Fe的ns寿命平衡态。在这种极端条件下,首次可以清楚地观察到铁的结构和电子变化。 EXAFS振荡的振幅持续高达500 GPa和17000 K,表明存在持久的局部有序性。此外,在理论计算上存在吸收起始能量位移值的差异,因此这种比较应有助于完善模型中使用的近似值。

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