arXiv · astro-ph/0105189
Numerical Analyses of Weakly Nonlinear Velocity-Density Coupling
Abstract
We study evolution of various statistical quantities of smoothed cosmic density and velocity fields using N-body simulations. The parameter $C\equiv /( <δ^2>)$ characterizes nonlinear coupling of these two fields and determines behavior of bulk velocity dispersion as a function of local density contrast. It is found that this parameter depends strongly on the smoothing scale even in quasi-linear regimes where the skewness parameter $S_3$ is nearly constant and close to the predicted value by the second-order perturbation theory. We also analyze weakly nonlinear effects caused by an adaptive smoothing known as the gather approach.
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Naoki Seto, Naoshi Sugiyama. 2001-05-11. Numerical Analyses of Weakly Nonlinear Velocity-Density Coupling. https://doi.org/10.1086/322285
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