With the advent of high-quality surveys in cosmology the full three-point correlation function will be a valuable statistic for describing structure formation models. It contains information on cosmological parameters and detailed halo properties that cannot be extracted from the two-point correlation function. We use the halo clustering model to analytically calculate the three-point correlati...

A simple kinematically consistent expression for the longitudinal two-point correlation function related to both the integral length scale and the Taylor microscale is obtained. On the inner scale, in a region of width inversely proportional to the turbulent Reynolds number, the function has the appropriate curvature at the origin. The expression for two-point correlation is related to the nonl...

Critical opalescence is a characteristic experimental signature of a second order phase transition in solid state physics. A new, experimentally accessible measure of opacity and of attenuation length in heavy ion reactions is suggested, as a combination of HBT radii and nuclear modification factors. This opacity is maximal when √ sNN , the system size and centrality correspond to the critical ...

The next generation of galaxy surveys will provide highly accurate measurements the large-scale structure Universe, allowing for more stringent tests gravity on cosmological scales. Higher order statistics are a valuable tool to study non-Gaussianities in matter field and break degeneracies between modified other physical or nuisance parameters. However, understanding from first principles beha...