• Title of article

    Convergence of SPH and AMR simulations

  • Author/Authors

    David A. Hubber، نويسنده , , Sam A. E. G. Falle، نويسنده , , Simon P. Goodwin، نويسنده ,

  • Issue Information
    روزنامه با شماره پیاپی سال 2010
  • Pages
    4
  • From page
    429
  • To page
    432
  • Abstract
    We present the first results of a large suite of convergence tests between Adaptive Mesh Refinement (AMR) Finite Difference Hydrodynamics and Smoothed Particle Hydrodynamics (SPH) simulations of the non-linear thin shell instability and the Kelvin-Helmholtz instability. We find that the two methods converge in the limit of high resolution and accuracy. AMR and SPH simulations of the non-linear thin shell instability converge with each other with standard algorithms and parameters. The Kelvin-Helmholtz instability in SPH requires both an artificial conductivity term and a kernel with larger compact support and more neighbours (e.g. the quintic kernel) in order converge with AMR. For purely hydrodynamical problems, SPH simulations take an order of magnitude longer than the grid code when converged.
  • Keywords
    Hydrodynamics , methods: numerical
  • Journal title
    Proceedings of the International Astronomical Union
  • Serial Year
    2010
  • Journal title
    Proceedings of the International Astronomical Union
  • Record number

    667717