Torchio Raffaella, Occelli Florent, Mathon Olivier, Sollier Arnaud, Lescoute Emilien, Videau Laurent, Vinci Tommaso, Benuzzi-Mounaix Alessandra, Headspith Jon, Helsby William, Bland Simon, Eakins Daniel, Chapman David, Pascarelli Sakura, Loubeyre Paul
CEA, DAM, DIF, F-91297, Arpajon, France.
ESRF-The European Synchrotron 71, Avenue des Martyrs Grenoble, France.
Sci Rep. 2016 Jun 1;6:26402. doi: 10.1038/srep26402.
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.
了解行星内部状态的热致密物质(WDM)是科学研究的一个新前沿领域。目前几乎没有在原子水平探测WDM状态的实验数据来检验当前模型,而且迄今为止所进行的实验在质量上也很有限。在此,我们报告一项原理验证实验,该实验使研究人员能够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条件下所能达到的水平。我们使用单个100皮秒的同步加速器X射线脉冲,通过K边吸收光谱法测量了WDM铁的纳秒级寿命平衡态。在如此极端的条件下,首次清晰地观察到了铁的结构和电子变化。扩展X射线吸收精细结构(EXAFS)振荡的幅度在高达500吉帕和17000 K时仍然存在,这表明存在持久的局部有序。此外,吸收起始能量位移值与理论计算存在差异,因此这种比较应有助于完善模型中使用的近似值。