Gravitational energy as dark energy: Concordance of cosmological tests

TL;DR

This paper suggests that a new averaging approach to inhomogeneous matter distribution could explain cosmic acceleration without dark energy, fitting multiple cosmological observations with consistent parameters.

Contribution

It introduces a novel solution to averaging inhomogeneous matter, providing an alternative explanation for cosmic acceleration compatible with key cosmological tests.

Findings

Parameters fit CMB angular scale and BAO measurements

Hubble constant aligns with independent measurements

Universe age estimated at 14.7 billion years

Abstract

We provide preliminary quantitative evidence that a new solution to averaging the observed inhomogeneous structure of matter in the universe [gr-qc/0702082, arxiv:0709.0732], may lead to an observationally viable cosmology without exotic dark energy. We find parameters which simultaneously satisfy three independent tests: the match to the angular scale of the sound horizon detected in the cosmic microwave background anisotropy spectrum; the effective comoving baryon acoustic oscillation scale detected in galaxy clustering statistics; and type Ia supernova luminosity distances. Independently of the supernova data, concordance is obtained for a value of the Hubble constant which agrees with the measurement of the Hubble Key team of Sandage et al [astro-ph/0603647]. Best-fit parameters include a global average Hubble constant H_0 = 61.7 (+1.2/-1.1) km/s/Mpc, a present epoch void volume fraction of f_{v0} = 0.76 (+0.12/-0.09), and an age of the universe of 14.7 (+0.7/-0.5) billion years as measured by observers in galaxies. The mass ratio of non-baryonic dark matter to baryonic matter is 3.1 (+2.5/-2.4), computed with a baryon-to-photon ratio that concords with primordial lithium abundances.