English

Vlasov-Poisson in 1D: waterbags

Astrophysics of Galaxies 2014-04-22 v1 Cosmology and Nongalactic Astrophysics

Abstract

We revisit in one dimension the waterbag method to solve numerically Vlasov-Poisson equations. In this approach, the phase-space distribution function f(x,v)f(x,v) is initially sampled by an ensemble of patches, the waterbags, where ff is assumed to be constant. As a consequence of Liouville theorem it is only needed to follow the evolution of the border of these waterbags, which can be done by employing an orientated, self-adaptive polygon tracing isocontours of ff. This method, which is entropy conserving in essence, is very accurate and can trace very well non linear instabilities as illustrated by specific examples. As an application of the method, we generate an ensemble of single waterbag simulations with decreasing thickness, to perform a convergence study to the cold case. Our measurements show that the system relaxes to a steady state where the gravitational potential profile is a power-law of slowly varying index β\beta, with β\beta close to 3/23/2 as found in the literature. However, detailed analysis of the properties of the gravitational potential shows that at the center, β>1.54\beta > 1.54. Moreover, our measurements are consistent with the value β=8/5=1.6\beta=8/5=1.6 that can be analytically derived by assuming that the average of the phase-space density per energy level obtained at crossing times is conserved during the mixing phase. These results are incompatible with the logarithmic slope of the projected density profile β20.47\beta-2 \simeq -0.47 obtained recently by Schulz et al. (2013) using a NN-body technique. This sheds again strong doubts on the capability of NN-body techniques to converge to the correct steady state expected in the continuous limit.

Keywords

Cite

@article{arxiv.1404.5175,
  title  = {Vlasov-Poisson in 1D: waterbags},
  author = {Stéphane Colombi and Jihad Touma},
  journal= {arXiv preprint arXiv:1404.5175},
  year   = {2014}
}

Comments

MNRAS, in press (Appendices B to J as supplementary material)