The Ricci Flow and the Early Universe

TL;DR

This paper proposes a novel framework where Ricci flow deforms quantum spacetime, naturally reproducing inflationary behavior and primordial perturbations without the need for inflaton fields or dark energy.

Contribution

It introduces a Ricci flow-based model of the early universe that explains inflation and primordial perturbations without inflaton or dark energy.

Findings

Ricci flow smooths out irregularities, leading to a homogeneous universe.

The model reproduces an inflationary de Sitter universe near the singularity.

Predicted scalar perturbation spectrum matches observations, tensor perturbations are too small to detect.

Abstract

A framework of quantum spacetime reference frame is proposed and reviewed, in which the quantum spacetime at the Gaussian approximation is deformed by the Ricci flow. At sufficient large scale, the Ricci flow not only smooths out local small irregularities making the universe a homogeneous and isotropic Friedmann-Robertson-Walker metric, but also develops a local singularity at the physical-time origin. Due to the phenomenological suppression of the non-Gaussian primordial perturbations, we assume the validity of the Ricci flow applying to the high curvature region near the local singularity of the early universe. The no-local-collapsing theorem of Perelman ensures the existence of a canonical neighborhood around the large curvature pinching point, which resembles a gradient shrinking Ricci soliton (GSRS) solution of the Ricci flow. Without any inflaton field, the GSRS naturally reproduces an exact inflationary deSitter universe near the singularity at the leading order. Without any rolling-down behavior of inflaton, the deviation from exact deSitter described by the "slow roll parameters" can be calculated by a small deviation from the singular flow-time via the Ricci flow, and the primordial perturbations can also be studied on the GSRS background, the power spectrum of the scalar perturbation agrees with present observations, and the one of the tensor perturbation is predicted too small to be detectable than the standard inflation. The previous treatment of the cosmological constant and the effective gravity are also briefly reviewed in the framework. So we argue that the Ricci flow provides us a possible unified view and treatment of the late epoch accelerating expansion and early epoch inflation of the universe without introducing dark energy or inflaton (dark energy of the second kind).