Glass-like universe: Real-space correlation properties of standard cosmological models

After reviewing the basic relevant properties of stationary stochastic processes (SSP), defining basic terms and quantities, we discuss the properties of the so-called Harrison-Zeldovich like spectra. These correlations, usually characterized exclusively in k space [i.e., in terms of power spectra $P(k)],$ are a fundamental feature of all current standard cosmological models. Examining them in real space we note their characteristics to be a negative power law tail ξ(r)~-r^-4, and a sub-Poissonian normalized variance in spheres σ²(R)~R^-4lnR. We note in particular that this latter behavior is at the limit of the most rapid decay (~R^-4) of this quantity possible for any stochastic distribution (continuous or discrete). This very particular characteristic is usually obscured in cosmology by the use of Gaussian spheres. In a simple classification of all SSP into three categories, we highlight with the name ``superhomogeneous'' the properties of the class to which models such as this, with $P(0)=0,$ belong. In statistical physics language they are well described as glass-like. They have neither ``scale-invariant'' features, in the sense of critical phenomena, nor fractal properties. We illustrate their properties with some simple examples, in particular that of a ``shuffled'' lattice.