English

A numerical comparison of theories of violent relaxation

Astrophysics 2009-11-10 v3

Abstract

Using N-body simulations with a large set of massless test particles we compare the predictions of two theories of violent relaxation, the well known Lynden-Bell theory and the more recent theory by Nakamura. We derive ``weaken'' versions of both theories in which we use the whole equilibrium coarse-grained distribution function as a constraint instead of the total energy constraint. We use these weaken theories to construct expressions for the conditional probability Ki(τ)K_i(\tau) that a test particle initially at the phase-space coordinate τ\tau would end-up in the ii'th macro-cell at equilibrium. We show that the logarithm of the ratio Rij(τ)Ki(τ)/Kj(τ)R_{ij}(\tau) \equiv K_i(\tau)/K_j(\tau) is directly proportional to the initial phase-space density f0(τ)f_0(\tau) for the Lynden-Bell theory and inversely proportional to f0(τ)f_0(\tau) for the Nakamura theory. We then measure Rij(τ)R_{ij}(\tau) using a set of N-body simulations of a system undergoing a gravitational collapse to check the validity of the two theories of violent relaxation. We find that both theories are at odds with the numerical results, qualitatively and quantitatively.

Keywords

Cite

@article{arxiv.astro-ph/0501619,
  title  = {A numerical comparison of theories of violent relaxation},
  author = {I. Arad and P. H. Johansson},
  journal= {arXiv preprint arXiv:astro-ph/0501619},
  year   = {2009}
}

Comments

Replaced with a revised version, which is now accepted to MNRAS. LaTeX, 12 pages, 6 figures