The Significance of the Cosmic Virial Theorem

Abstract

We discuss the development and physics of the cosmic virial theorem and its traditional application as an indicator of the cosmic mean density. The standard result that the density must be sub-critical relies on the assumption that the galaxy three-point correlation function accurately describes the mass distribution around a typical pair of galaxies. To challenge this assumption, we develop a simple model of this mass distribution based on the extension of galactic halos. In such a model, one sees clearly the importance of the local mass distribution around pairs to the prediction of the galaxy pair-wise velocity dispersion. The model provides insight into the mechanics of the theorem and demonstrates that a flat universe is {\it consistent} with the observations. More generally, we conclude that the relative pair-wise velocity dispersion probes the mass clustered around galaxies and that the observations, viewed in this light, indicate a lower bound of $\sim 300\; h^{-1}$kpc on the radius of galactic halos.