Abstract:Année de publication : 1999
We present results of the investigations of the statistical properties of a joint density and velocity divergence probability distribution function (PDF) in the mildly non-linear regime. For that purpose we use both perturbation theory results (complete as possible up to third order terms), obtained analytically for a Gaussian filter and extended for a top-hat filter, and numerical simulations. {In particular we derive the quantitative and qualitative predictions for constrained averages and constrained dispersions -- which describe the nonlinearities and the stochasticity properties beyond the linear regime -- and compare them against numerical simulations. We find overall a good agreement with scaling relations for the $\Omega$-dependence of these quantities satisfactory reproduced.} {Finally, guided by our analytical and numerical results, we construct a robust phenomenological description of the joint PDF in a closed analytic form. The good agreement of our formula with results of N-body simulations for a number of cosmological parameters provides a sound validation of the presented approach. } {Our results} provide a basis for a potentially powerful tool with which it is possible to analyze galaxy survey data in order to test the gravitational instability paradigm beyond the linear regime and put useful {constraints} on cosmological parameters.
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