Virialisation-induced curvature as a physical explanation for dark energy
Boudewijn F. Roukema, Jan J. Ostrowski, Thomas Buchert

TL;DR
This paper proposes that the effects attributed to dark energy in cosmology can be explained by virialisation-induced curvature, challenging the need for a cosmological constant and suggesting a correction to the standard matter-dominated model.
Contribution
It introduces a general-relativistic correction based on virialisation to the Einstein de Sitter model, offering an alternative explanation for dark energy phenomena.
Findings
Virialisation fraction increases around redshift 1-3, coinciding with the rise of Omega_Lambda.
The virialisation-corrected Einstein de Sitter model matches the distance modulus of LambdaCDM over 0<z<3.
Effective matter density at present is inferred to be approximately 0.26.
Abstract
The geometry of the dark energy and cold dark matter dominated cosmological model (LambdaCDM) is commonly assumed to be given by a Friedmann-Lemaitre-Robertson-Walker (FLRW) metric, i.e. it assumes homogeneity in the comoving spatial section. The homogeneity assumption fails most strongly at (i) small distance scales and (ii) recent epochs, implying that the FLRW approximation is most likely to fail at these scales. We use the virialisation fraction to quantify (i) and (ii), which approximately coincide with each other on the observational past light cone. For increasing time, the virialisation fraction increases above 10% at about the same redshift (sim 1-3) at which Omega_Lambda grows above 10% (approx 1.8). Thus, instead of non-zero Omega_Lambda, we propose an approximate, general-relativistic correction to the matter-dominated (Omega_m =1, Omega_Lambda=0), homogeneous metric…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
