Gravitational clustering in a D-dimensional universe

We consider the problem of gravitational clustering in a D-dimensional expanding universe and derive scaling relations connecting the exact mean two-point correlation function with the linear mean correlation function, in the quasilinear and nonlinear regimes, using the standard paradigms of scale-invariant radial collapse and stable clustering. We show that the existence of scaling laws is a generic feature of gravitational clustering in an expanding background, in all dimensions except D52 and comment on the special nature of the two-dimensional ~2D! case. The D-dimensional scaling laws derived here reduce, in the three-dimensional case, to scaling relations obtained earlier from N-body simulations. Finally, we consider the case of clustering of two-dimensional particles in a 2D expanding background, governed by a force 2GM /R , and show that the correlation function does not grow ~to first order! until much after the recollapse of any shell.