Turbulence model of the cosmic structure
  The Kolmogorov approach to turbulence is applied to the Burgers turbulence in
the stochastic adhesion model of large-scale structure formation. As the
perturbative approach to this model is unreliable, here is proposed a new,
non-perturbative approach, based on a suitable formulation of Kolmogorov's
scaling laws. This approach suggests that the power-law exponent of the matter
density two-point correlation function is in the range 1--1.33, but it also
suggests that the adhesion model neglects important aspects of the
gravitational dynamics.
