216 / 2023-04-15 20:54:25
Development of X-ray fluorescence holography under high pressure
x-ray fluorescence holography,high pressure,SrTiO3
摘要录用
Xinhui Zhan / Hiroshima Univercity
Naoki Ishimatsu / Hiroshima University
Koji Kimura / Nagoya Institute of Technology
Tomoko Sato / Hiroshima University
Naohisa Happo / Hiroshima City University
Naomi Kawamura / SPring-8
Kotaro Higashi / SPring-8
Ritsuko Eguchi / Okayama University
Yoshihiro Kubozono / Okayama University
Hiroo Tajiri / SPring-8
Toru Shinmei / Ehime University
Tetsuo Irifune / Ehime University
Shinya Hosokawa / Kumamoto University
Halubai Sekhar / Nagoya Institute of Technology
Tomohiro Matsushita / Nara Institute of Science and Technology
Koichi Hayashi / Nagoya Institute of Technology
X-ray fluorescence holography (XFH) is an atomic structure determination technique that utilizes fluorescing atoms as a wave source or a monitor of the interference field within a crystal sample. [1] Because it provides three-dimensional atomic images around a specified element within a range of up to a few nm in real space, XFH is used for medium-range local structural analysis. However, XFH has not been measured under high pressure yet. In this work, we combined the XFH with the diamond anvil cell (DAC) to study the local structures around Sr atom in a single-crystalline SrTiO3 at high pressure. The experiment of XFH was carried out at BL39XU of SPring-8 using the normal mode setup. A symmetry DAC with a wide window has been newly designed, and the window allowed us to collect the XFH patterns from the sample irradiated through a beryllium gasket. The most serious difficulty to be solved under high pressure is the scattered X-rays from the diamond anvils and gasket, which are superimposed on the XFH image from the sample. We have demonstrated that nano polycrystalline diamond is a good material for the anvil that does not generate the background scattering.[2] As a result, Kossel lines of SrTiO3 were successfully observed. Furthermore, the position of the Kossel line gradually moved as a pressure dependence of the XFH image. Bragg scattering from the beryllium gasket remained as background signal of our XFH images, however, methods to remove the Bragg scattering are discussed in the poster presentation.

 
重要日期
  • 会议日期

    06月05日

    2023

    06月09日

    2023

  • 04月30日 2023

    提前注册日期

  • 05月01日 2023

    摘要截稿日期

  • 05月01日 2023

    摘要录用通知日期

  • 05月01日 2023

    初稿截稿日期

  • 05月31日 2023

    注册截止日期

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北京师范大学天文系
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Matter and Radiation at Extremes期刊
中国工程物理研究院流体物理研究所
北京应用物理与计算数学研究所
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