Non-Gaussianity of the Cosmic Baryon Fluid: Log-Poisson Hierarchy Model

Details Non-Gaussianity of the Cosmic Baryon Fluid: Log-Poisson Hierarchy Model Non-Gaussianity of the Cosmic Baryon Fluid: Log-Poisson Hierarchy Model

2007-07-18

arxiv.org/abs/0707.2620v1

Astronomy and Astrophysics

Astrophysics

19 pages, 8 figures, accepted by ApJ

Scientific paper

10.1086/523684

In the nonlinear regime of cosmic clustering, the mass density field of the cosmic baryon fluid is highly non-Gaussian. It shows different dynamical behavior from collisionless dark matter. Nevertheless, the evolved field of baryon fluid is scale-covariant in the range from the Jeans length to a few ten h^{-1} Mpc, in which the dynamical equations and initial perturbations are scale free. We show that in the scale-free range, the non-Gaussian features of the cosmic baryon fluid, governed by the Navier-Stokes equation in an expanding universe, can be well described by a log-Poisson hierarchical cascade. The log-Poisson scheme is a random multiplicative process (RMP), which causes non-Gaussianity and intermittency even when the original field is Gaussian. The log-Poisson RMP contains two dimensionless parameters: $\beta$ for the intermittency and $\gamma$ for the most singular structure. All the predictions given by the log-Poisson RMP model, including the hierarchical relation, the order dependence of the intermittent exponent, the moments, and the scale-scale correlation, are in good agreement with the results given by hydrodynamic simulations of the standard cold dark matter model. The intermittent parameter $\beta$ decreases slightly at low redshift and indicates that the density field of baryon fluid contains more singular structures at lower redshifts. The applicability of the model is addressed.

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