64 / 2020-03-09 21:42:17
Ramp compressed Iron at Super-Earth interior conditions
laser shock-loaded,high pressure,iron,Equation of state,Super-Earth
摘要待审
Liang Sun / Laser Fusion Research Center, China Academy of Engineering Physics (CAEP), Mianyang,621900,P. R. China
Xiaoxi Duan / Laser Fusion Research Center, China Academy of Engineering Physics (CAEP), Mianyang,621900,P. R. China
Liping Peng / Laser Fusion Research Center, China Academy of Engineering Physics (CAEP), Mianyang,621900,P. R. China
Yulong Li / Laser Fusion Research Center, China Academy of Engineering Physics (CAEP), Mianyang,621900,P. R. China
Youjun Zhang / Sichuan University, Chengdu, P.R. China
Toshimori Sekine / Center for High Pressure Science and Technology Advanced Research (HPSTAR), Shanghai, 201203, P. R. China
Zhebin Wang / Laser Fusion Research Center, China Academy of Engineering Physics (CAEP), Mianyang,621900,P. R. China
Jiamin Yang / Laser Fusion Research Center, China Academy of Engineering Physics (CAEP), Mianyang,621900,P. R. China
Shaoen Jiang / Laser Fusion Research Center, China Academy of Engineering Physics (CAEP), Mianyang,621900,P. R. China
Recent investigations of the mass-radius relationship of solid exoplanets indicate they consist of iron, silicates, water, and carbon compounds. The accurate equation of state (EOS) at Super-Earth interior conditions is fundamental to evaluate the composition and interior structure. The conditions in these rocky Super-Earths interiors reach 1-4 TPa and ~10^4K and cannot be easily achieved by a single shock or quasi-isentropic compression in laboratory experiments.
Here we developed laser shock and ramp compression techniques to perform a series of experiments on Fe-LiF targets initially shocked and then ramped using shaped laser pulses in the high-powered laser facility of China. In the present experiments, the initial shock pressure was nearly 300 GPa to provide high temperature for achieving interiors conditions. The peak ramp pressures were more than 1 TPa, comparable to that predicted at the center of Super-Earths. By the Lagrangian sound-speed analysis for the measured VISAR data, we determined pressure, density and sound speed along the isentropic path at these extreme condition. Our EOS data were also compared with the previous ones to know the effects of the initial shock pressure and temperature. Finally, our results provide directly-measured key physical properties of iron at the extreme high pressure and temperature, which can be used to model the physics and chemistry of iron and to understand the structures and dynamics of the cores of Super-Earths.
重要日期
  • 会议日期

    05月25日

    2020

    05月29日

    2020

  • 02月29日 2020

    初稿截稿日期

  • 05月29日 2020

    注册截止日期

承办单位
中国工程物理研究院流体物理研究所
中国工程物理研究院激光聚变研究中心
历届会议
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