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Published February 1, 2013 | Accepted Version + Published
Journal Article Open

A general class of Lagrangian smoothed particle hydrodynamics methods and implications for fluid mixing problems

Abstract

Various formulations of smoothed particle hydrodynamics (SPH) have been proposed, intended to resolve certain difficulties in the treatment of fluid mixing instabilities. Most have involved changes to the algorithm which either introduces artificial correction terms or violates what is arguably the greatest advantage of SPH over other methods: manifest conservation of energy, entropy, momentum and angular momentum. Here, we show how a class of alternative SPH equations of motion (EOM) can be derived self-consistently from a discrete particle Lagrangian – guaranteeing manifest conservation – in a manner which tremendously improves treatment of these instabilities and contact discontinuities. Saitoh & Makino recently noted that the volume element used to discretize the EOM does not need to explicitly invoke the mass density (as in the 'standard' approach); we show how this insight, and the resulting degree of freedom, can be incorporated into the rigorous Lagrangian formulation that retains ideal conservation properties and includes the '∇h' terms that account for variable smoothing lengths. We derive a general EOM for any choice of volume element (particle 'weights') and method of determining smoothing lengths. We then specify this to a 'pressure–entropy formulation' which resolves problems in the traditional treatment of fluid interfaces. Implementing this in a new version of the GADGET code, we show it leads to good performance in mixing experiments (e.g. Kelvin–Helmholtz and 'blob' tests). And conservation is maintained even in strong shock/blastwave tests, where formulations without manifest conservation produce large errors. This also improves the treatment of subsonic turbulence and lessens the need for large kernel particle numbers. The code changes are trivial and entail no additional numerical expense. This provides a general framework for self-consistent derivation of different 'flavours' of SPH.

Additional Information

© 2012 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2012 October 12. Received 2012 October 12; in original form 2012 June 11. We thank Dusan Keres and Lars Hernquist for helpful discussions, and Oscar Agertz, Andrey Kravtsov, Robert Feldmann and Nick Gnedin for contributions motivating this work. We also thank Justin Read, Volker Springel, Eliot Quataert, Claudio Dalla Vecchia and the anonymous referee for useful comments and suggestions, and thank Andreas Bauer for sharing the implementation of the turbulent driving routine. Support for PFH was provided by NASA through Einstein Postdoctoral Fellowship Award Number PF1-120083 issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the NASA under contract NAS8-03060.

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Accepted Version - 1206.5006.pdf

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Additional details

Created:
August 19, 2023
Modified:
October 20, 2023