84 / 2023-04-13 09:58:30
Role of hot electrons in mitigating ablative Rayleigh-Taylor instability
Hot electrons,ablative Rayleigh-Taylor instability,hydrodynamic instability
Abstract Accepted
Jun Li / Institute of Applied Physics and Computational Mathematics
Rui Yan / University of Science and Technology of China
赵 斌 / 南京工程学院
Jian Zheng / university of science and technology of china
Huasen Zhang / Institute of Applied Physics and Computational mathematics
Xiyun Lu / University of Science and Technology of China
In laser-driven inertial confinement fusion (ICF) specifically with high laser intensities, energetic (hot) electrons (HEs) can be generated via laser-plasma instabilities. HEs can significantly impact the target performance by modifying the implosion hydrodynamics. In this work, the effects of moderate-energy (about 20 to 40 keV) HEs on the evolution of ablative Rayleigh–Taylor instability (ARTI) are studied through numerical simulations with a multigroup diffusion model in which the HE population is treated as a high-energy group launched from the boundary. With HEs present, it is found that ARTI linear growth rates are reduced even though the acceleration of the implosion shell is enhanced by HEs. The reduction in the linear growth rate is owing to the increase in the ablation velocity and the density scale length, and this stabilization effect is greater in the shorter-wavelength modes and/or higher-energy HE cases. The ARTI linear growth does not get mitigated monotonically as the HE number density increases for a given fixed HE kinetic energy. The latest results showing that HEs can stabilize the highly nonlinear growth of multimode ARTI are also presented.
Important Date
  • Conference Date

    Jun 05

    2023

    to

    Jun 09

    2023

  • Apr 30 2023

    Early Bird Registration

  • May 01 2023

    Abstract Submission Deadline

  • May 01 2023

    Abstract Notification of Acceptance

  • May 01 2023

    Draft paper submission deadline

  • May 31 2023

    Registration deadline

Sponsored By
Science and Technology on Plasma Physics Laboratory
Department of Astronomy, Beijing Normal University
Organized By
Matter and Radiation at Extremes
Institute of Fluid Physics, China Academy of Engineering Physics, China
Institute of Applied Physics and Computational Mathematics, Beijing, China
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