Magnetohydrodynamic simulation comparisons of cylindrical implosion experiments for Rayleigh Taylor instability

POSTER

Abstract

The Rayleigh-Taylor (RT) hydrodynamic instability degrade the performance of inertial confinement fusion (ICF) experiments. During both the acceleration and deceleration phases of the implosion, the RT instability grows and mixes materials at the interfaces. Mitigating the RT instability enables ICF implosions to achieve hot spot pressures necessary to reach ignition conditions with respect to the Lawson criterion. The current approach is to reduce seeds and match Atwood numbers to reduce instability growth. An alternate approach would be the application of magnetic fields. Here we present computational design efforts using radiation-hydrodynamic codes with magnetohydrodynamic capabilities (FLASH) to study RT inhibition under the influence of magnetic fields on a cylindrical imploding target. Since ablative stabilization has the strongest impact on the inhibition of RT, the key design challenge for cylindrical experiments is achieving relevant temperatures in the fill material. We explore ideas for validation experiments.

*The software used in this work was developed in part by the DOE NNSA ASC- and DOE Office of Science ASCR-supported Flash Center for Computational Science at the University of Chicago.

Authors

  • Nomita Vazirani

    • Los Alamos National Lab
  • J. Kline

    • Los Alamos National Laboratory
    • Los Alamos National Lab
  • K.A. Flippo

    • Los Alamos National Laboratory
    • LANL
    • Los Alamos National Lab
  • Sasikumar Palaniyappan

    • Los Alamos National Laboratory
    • Los Alamos National Laboratory, Los Alamos, NM 87545
    • Los Alamos National Lab
  • J.P. Sauppe

    • Los Alamos National Laboratory
    • Los Alamos National Lab
  • Scott England

    • Virginia Tech
  • Wayne Scales

    • Virginia Tech