A 3D, Parallel, Solution-Adaptive Model for Radiative Shocks

ORAL

Abstract

In this talk, a radiation hydrodynamics code for simulating radiative shocks will be described. The high-level validation problem for the code is one in which a 1 ns, 4 kJ laser pulse irradiates a Be disk, driving a shock into a Xe-filled plastic tube. The radiative precursor to the shock heats the wall of the tube, so that the there is a complex interaction among the shock driven by the ablated material from the wall, the laser driven shock, and the Be-Xe interface. The code is three-dimensional, solution-adaptive, and parallel. The radiation transport model in the current code is based on gray diffusion; work is underway to support higher-fidelity radiation transport models. The methodology used in the code and preliminary results of simulations will be presented.

*This work was supported in part by the US DOE NNSA under the Predictive Science Academic Alliance Program by grant DE-FC52-08NA28616.

Authors

  • Kenneth Powell

    • Center for Radiative Shock Hydrodynamics, University of Michigan
  • Paul Drake

    • University of Michigan
    • U of Michigan
    • Center for Radiative Shock Hydrodynamics, University of Michigan
  • James Holloway

    • Center for Radiative Shock Hydrodynamics, University of Michigan
  • Bart Van der Holst

    • Center for Radiative Shock Hydrodynamics, University of Michigan
  • Smadar Karni

    • Center for Radiative Shock Hydrodynamics, University of Michigan
  • William Martin

    • Center for Radiative Shock Hydrodynamics, University of Michigan
  • Eric Myra

    • Center for Radiative Shock Hydrodynamics, University of Michigan
    • University of Michigan
  • Igor Sokolov

    • Center for Radiative Shock Hydrodynamics, University of Michigan
    • University of Michigan
  • Quentin Stout

    • Center for Radiative Shock Hydrodynamics, University of Michigan
  • G. Toth

    • Center for Radiative Shock Hydrodynamics, University of Michigan