Fully developed relativistic turbulence

We use a simple model consisting of energy-momentum tensor conservation and Maxwell-Cattaneo equation for its viscous part to study nonlinear phenomena in real relativistic fluid. focus on new types behavior without nonrelativistic equivalents, such as an entropy cascade driven by fluctuations the degrees freedom theory. write down von K\'arm\'an--Howarth equations this kind turbulence consider correlations corresponding fully developed turbulence.