Point field models for the galaxy point pattern. Modelling the singularity of the two-point correlation function

There is empirical evidence that the two-point correlation function of the galaxy distribution follows, for small scales, reasonably well a power-law expression $\xi (r)\propto r^{-\gamma }$ with $\gamma$ between 1.5 and 1.9. Nevertheless, most of the point field models suggested in the literature do not have this property. This paper presents a new class of models, which is produced by modifying point fields commonly used in cosmology to mimic the galaxy distribution, but where $\gamma =2$ is too large. The points are independently and randomly shifted, leading to the desired reduction of the value of $\gamma$.