Scaling Relations for Collision-less Dark Matter Turbulence
Akika Nakamichi, Masahiro Morikawa

TL;DR
This paper proposes that collision-less dark matter behaves like a turbulent fluid, deriving scaling laws that explain various cosmic observations and suggesting a universal energy flow rate in dark matter structures.
Contribution
It introduces the concept of dark turbulence in collision-less dark matter and derives scaling laws from Navier-Stokes equations applicable to cosmic structures.
Findings
Consistent scaling relations for dark matter systems are explained by dark turbulence.
Derived a universal energy flow rate of 0.3 cm^2/sec^3 in cosmic structures.
Application of turbulence theory to observations like velocity dispersion and power spectra.
Abstract
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: , which may be understood as the speed of the…
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