Additions and Improvements to the FLASH Code for Simulating High Energy Density Physics Experiments

POSTER

Abstract

FLASH is an open source, finite-volume Eulerian, spatially adaptive, radiation hydrodynamics and magnetohydrodynamics code that incorporates capabilities for a broad range of physical processes, performs well on a wide range of computer architectures, and has a broad user base. Extensive capabilities have been added to FLASH to make it an open toolset for the academic high energy density physics community. We summarize these capabilities, with particular emphasis on recent additions and improvements, and present the results of several verification tests. We also describe several collaborations with the National Laboratories and the academic community in which FLASH has been used to simulate high energy density physics experiments.

*This work was supported in part by DOE NNSA ASC.

Authors

  • Donald Lamb

    • Flash Center for Computational Science, University of Chicago
    • University of Chicago Flash Center
    • Department of Astronomy and Astrophysics, University of Chicago
  • Christopher Daley

    • Flash Center for Computational Science, University of Chicago
  • Anshu Dubey

    • Flash Center for Computational Science, University of Chicago
  • Milad Fatenejad

    • Flash Center for Computational Science, University of Chicago
  • Norbert Flocke

    • Flash Center for Computational Science, University of Chicago
  • Carlo Graziani

    • Flash Center for Computational Science, University of Chicago
  • Dongwook Lee

    • Flash Center for Computational Science, University of Chicago
  • Petros Tzeferacos

    • Flash Center for Computational Science, University of Chicago
  • Klaus Weide

    • Flash Center for Computational Science, University of Chicago