Observational constraints on the cosmological expansion rate and spatial curvature

TL;DR

This paper uses observational data to test the standard cosmological model, constraining dark energy dynamics and spatial curvature, generally supporting flatness but allowing some room for deviations.

Contribution

It provides updated observational constraints on dynamical dark energy models and spatial curvature, exploring alternatives to the standard flat Lambda-CDM model.

Findings

Data favor the standard flat Lambda-CDM model.

Some data combinations show mild preference for spatial curvature.

Constraints allow for mild dynamical dark energy.

Abstract

Observations conducted over the last few decades show that the expansion of the Universe is accelerating. In the standard model of cosmology, this accelerated expansion is attributed to a dark energy in the form of a cosmological constant. It is conceivable, however, for the dark energy to exhibit mild dynamics (so that its energy density changes with time rather than having a constant value), or for the accelerated expansion of the Universe to be caused by some mechanism other than dark energy. In this work I will investigate both of these possibilities by using observational data to place constraints on the parameters of simple models of dynamical dark energy as well as cosmological models without dark energy. I find that these data favor the standard model while leaving some room for dynamical dark energy. The standard model also holds that the Universe is flat on large spatial scales. The same observational data used to test dark energy dynamics can be used to constrain the large-scale curvature of the Universe, and these data generally favor spatial flatness, with some mild preference for spatial curvature in some data combinations.