Averaging, renormalization group and criticality in cosmology

TL;DR

This paper explores the application of real-space Renormalization Group methods to cosmology, linking RG flow to Ricci-Hamilton equations and discussing implications for criticality and manifold deformation.

Contribution

It establishes a novel connection between RG flow and Ricci-Hamilton equations, providing a physical interpretation relevant to cosmological averaging problems.

Findings

RG flow described by Ricci-Hamilton equations

Connection between manifold deformation and Thurston's conjecture

Discussion of criticality in cosmological models

Abstract

Several problems in physics, in particular the averaging problem in gravity, can be described in a formalism derived from the real-space Renormalization Group (RG) methods. It is shown that the RG flow is provided by the Ricci-Hamilton equations which are thereby provided with a {\it physical} interpretation. The connection between a manifold deformation according to these equations and Thurston's conjecture is exhibited. The significance of criticality which naturally appears in this framework is briefly discussed. This article summarizes also recent work with M. Carfora. Moreover, a report on some work in progress is given and some open issues in the averaging problem pointed out.