English

A new insight into the consistency of smoothed particle hydrodynamics

Computational Physics 2019-04-09 v2 Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies Fluid Dynamics

Abstract

In this paper the problem of consistency of smoothed particle hydrodynamics (SPH) is solved. A novel error analysis is developed in nn-dimensional space using the Poisson summation formula, which enables the treatment of the kernel and particle approximation errors in combined fashion. New consistency integral relations are derived for the particle approximation which correspond to the cosine Fourier transform of the classically known consistency conditions for the kernel approximation. The functional dependence of the error bounds on the SPH interpolation parameters, namely the smoothing length hh and the number of particles within the kernel support N{\cal{N}} is demonstrated explicitly from which consistency conditions are seen to follow naturally. As N{\cal{N}}\to\infty, the particle approximation converges to the kernel approximation independently of hh provided that the particle mass scales with hh as mhβm\propto h^{\beta}, with β>n\beta >n. This implies that as h0h\to 0, the joint limit m0m\to 0, N{\cal{N}}\to\infty, and NN\to\infty is necessary for complete convergence to the continuum, where NN is the total number of particles. The analysis also reveals the presence of a dominant error term of the form (lnN)n/N(\ln {\cal{N}})^{n}/{\cal{N}}, which tends asymptotically to 1/N1/{\cal{N}} when N1{\cal{N}}\gg 1, as it has long been conjectured based on the similarity between the SPH and the quasi-Monte Carlo estimates.

Keywords

Cite

@article{arxiv.1608.05883,
  title  = {A new insight into the consistency of smoothed particle hydrodynamics},
  author = {Leonardo Di G. Sigalotti and Otto Rendón and Jaime Klapp and Carlos A. Vargas and Kilver Campos},
  journal= {arXiv preprint arXiv:1608.05883},
  year   = {2019}
}

Comments

27 pages. v2: Matches published version