Comparison of Dynamical Approximation Schemes for Non-Linear Gravitational Clustering

Details Comparison of Dynamical Approximation Schemes for Non-Linear Gravitational Clustering Comparison of Dynamical Approximation Schemes for Non-Linear Gravitational Clustering

1994-02-23

arxiv.org/abs/astro-ph/9402057v1

Astrophys.J.426:L19-L22,1994

Astronomy and Astrophysics

Astrophysics

8 pp., plain TeX. ApJ Letters, in press. Contact melott@kusmos.phsx.ukans.edu for Figures

Scientific paper

10.1086/187329

I report on controlled comparison of gravitational approximation schemes linear/lognormal/adhesion/frozen-flow/Zel'dovich(ZA) and ZA's second--order generalization. In the last two cases we also created new versions of the approximation by truncation, i.e., by finding an optimum smoothing window (see text) for the initial conditions. The Zel'dovich approximation, with optimized initial smoothing, worked extremely well. Its second-order generalization was slightly better. The success of our best-choice was a result of the treatment of the phases of nonlinear Fourier components. The adhesion approximation produced the most accurate nonlinear power spectrum and density distribution, but its phase errors suggest mass condensations were moved somewhat incorrectly. Due to its better reproduction of the mass density distribution function and power spectrum, adhesion might be preferred for some uses. We recommend either n-body simulations or our modified versions of ZA, depending on the purpose. Modified ZA can rapidly generate large numbers of realizations of model universes with good accuracy down to galaxy group (or smaller) mass scales.

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