Fundamental differences between SPH and grid methods

Oscar Agertz, Ben Moore, Joachim Stadel, Doug Potter, Francesco Miniati, Justin Read, Lucio Mayer, Artur Gawryszczak, Andrey Kravtsov, Åke Nordlund, Frazer Pearce, Vicent Quilis, Douglas Rudd, Volker Springel, James McLellan Stone, Elizabeth Tasker, Romain Teyssier, James Wadsley, Rolf Walder

Research output: Contribution to journalArticle

431 Scopus citations

Abstract

We have carried out a comparison study of hydrodynamical codes by investigating their performance in modelling interacting multiphase fluids. The two commonly used techniques of grid and smoothed particle hydrodynamics (SPH) show striking differences in their ability to model processes that are fundamentally important across many areas of astrophysics. Whilst Eulerian grid based methods are able to resolve and treat important dynamical instabilities, such as Kelvin-Helmholtz or Rayleigh-Taylor, these processes are poorly or not at all resolved by existing SPH techniques. We show that the reason for this is that SPH, at least in its standard implementation, introduces spurious pressure forces on particles in regions where there are steep density gradients. This results in a boundary gap of the size of an SPH smoothing kernel radius over which interactions are severely damped.

Original languageEnglish (US)
Pages (from-to)963-978
Number of pages16
JournalMonthly Notices of the Royal Astronomical Society
Volume380
Issue number3
DOIs
StatePublished - Sep 2007

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Galaxies: evolution
  • Galaxies: formation
  • Galaxies: general
  • Hydrodynamics
  • ISM: clouds
  • Instabilities
  • Methods: numerical
  • Turbulence

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    Agertz, O., Moore, B., Stadel, J., Potter, D., Miniati, F., Read, J., Mayer, L., Gawryszczak, A., Kravtsov, A., Nordlund, Å., Pearce, F., Quilis, V., Rudd, D., Springel, V., Stone, J. M., Tasker, E., Teyssier, R., Wadsley, J., & Walder, R. (2007). Fundamental differences between SPH and grid methods. Monthly Notices of the Royal Astronomical Society, 380(3), 963-978. https://doi.org/10.1111/j.1365-2966.2007.12183.x