English

Force Error Optimization in Smooth Particle Hydrodynamics

Astrophysics 2016-08-30 v2

Abstract

We discuss capability of Smooth Particle Hydrodynamics to represent adequately the dynamics of self-gravitating systems, in particular for what regards the quality of approximation of force fields in the motion equations. When cubic spline kernels are used, we find that a good estimate of the pressure field cannot be obtained in non uniform situations using the commonly adopted scheme of adapting the kernel sizes to include a fixed number of neighbours. We find that a fixed number of neighbours gives the best approximation of just the intensity of the force field, while the determination of the direction of the force requires a number of neighbours which strongly depends on the particle position.

Keywords

Cite

@article{arxiv.astro-ph/9611177,
  title  = {Force Error Optimization in Smooth Particle Hydrodynamics},
  author = {R. Capuzzo-Dolcetta and R. Di Lisio},
  journal= {arXiv preprint arXiv:astro-ph/9611177},
  year   = {2016}
}

Comments

17 pages, 13 figures, in 1 standard LaTex file and 13 postscript files