The Generalized Poisson distribution and a model of clustering from   Poisson initial conditions
  This paper presents a new derivation of the Generalized Poisson distribution. This distribution provides a good fit to the evolved, counts-in-cells distribution measured in numerical simulations of hierarchical clustering from Poisson initial conditions. This new derivation can be used to construct a useful analytic model of the evolution of clustering measured in these simulations. The model is consistent with the assumption that, as the universe expands and the comoving sizes of regions change as a result of gravitational instability, the number of such expanding and contracting regions is conserved. The model neglects the influence of external tides on the evolution of such regions. Indeed, in the context of this model, the GPD can be thought of as arising from a simple variant of the well-studied spherical collapse model, in which tidal effects are also neglected. The model can be understood as a simple generalization of the excursion set model which is used to estimate the number density of collapsed, virialized halos. The generalization allows one to describe the spatial distribution of the halos and the mass simultaneously, so the extent to which these halos are biased tracers of the underlying matter distribution is easy to estimate. 
Ravi K. Sheth (MPI Astrophysik)