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Large-scale structure formation can be modeled as a nonlinear process thattransfers energy from the largest scales to successively smaller scales untilit is dissipated, in analogy with Kolmogorov's cascade model of incompressibleturbulence. However, cosmic turbulence is very compressible, and vorticityplays a secondary role in it. The simplest model of cosmic turbulence is theadhesion model, which can be studied perturbatively or adapting to itKolmogorov's non-perturbative approach to incompressible turbulence. Thisapproach leads to observationally testable predictions, e.g., to the power-lawexponent of the matter density two-point correlation function.

Turbulence models of gravitational clustering