Scaling Relations for Collision-less Dark Matter Turbulence

Details Scaling Relations for Collision-less Dark Matter Turbulence Scaling Relations for Collision-less Dark Matter Turbulence

2008-05-02

arxiv.org/abs/0805.0172v3

JCAP 1001:011,2010

Astronomy and Astrophysics

Astrophysics

26 pages, 6 figures

Scientific paper

10.1088/1475-7516/2010/01/011

Many scaling relations are observed for self-gravitating systems in the universe. We explore the consistent understanding of them from a simple principle based on the proposal that the collision-less dark matter fluid terns into a turbulent state, i.e. dark turbulence, after crossing the caustic surface in the non-linear stage. The dark turbulence will not eddy dominant reflecting the collision-less property. After deriving Kolmogorov scaling laws from Navier-Stokes equation by the method similar to the one for Smoluchowski coagulation equation, we apply this to several observations such as the scale-dependent velocity dispersion, mass-luminosity ratio, magnetic fields, and mass-angular momentum relation, power spectrum of density fluctuations. They all point the concordant value for the constant energy flow per mass: $0.3 cm^2/sec^3$, which may be understood as the speed of the hierarchical coalescence process in the cosmic structure formation.

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