English

Numerical Convergence in Smoothed Particle Hydrodynamics

Cosmology and Nongalactic Astrophysics 2015-06-23 v2

Abstract

We study the convergence properties of smoothed particle hydrodynamics (SPH) using numerical tests and simple analytic considerations. Our analysis shows that formal numerical convergence is possible in SPH only in the joint limit NN \rightarrow \infty, h0h \rightarrow 0, and NnbN_{nb} \rightarrow \infty, where NN is the total number of particles, hh is the smoothing length, and NnbN_{nb} is the number of neighbor particles within the smoothing volume used to compute smoothed estimates. Previous work has generally assumed that the conditions NN \rightarrow \infty and h0h \rightarrow 0 are sufficient to achieve convergence, while holding NnbN_{nb} fixed. We demonstrate that if NnbN_{nb} is held fixed as the resolution is increased, there will be a residual source of error that does not vanish as NN \rightarrow \infty and h0h \rightarrow 0. Formal numerical convergence in SPH is possible only if NnbN_{nb} is increased systematically as the resolution is improved. Using analytic arguments, we derive an optimal compromise scaling for NnbN_{nb} by requiring that this source of error balance that present in the smoothing procedure. For typical choices of the smoothing kernel, we find NnbN1/2N_{nb} \propto N^{1/2}. This means that if SPH is to be used as a numerically convergent method, the required computational cost does not scale with particle number as O(N)O(N), but rather as O(N1+δ)O(N^{1+\delta}), where δ1/2\delta \approx 1/2, with a weak dependence on the form of the smoothing kernel.

Keywords

Cite

@article{arxiv.1410.4222,
  title  = {Numerical Convergence in Smoothed Particle Hydrodynamics},
  author = {Qirong Zhu and Lars Hernquist and Yuexing Li},
  journal= {arXiv preprint arXiv:1410.4222},
  year   = {2015}
}

Comments

The revised version accepted in ApJ, with typos corrected and references added

R2 v1 2026-06-22T06:25:10.679Z