The Universe Around Us Turned Out to Be More Curved Than We Thought ✛ ✦

Original: "Backreaction and the Role of Spatial Curvature in the Cosmic Neighborhood"
arXiv:2605.05454v1 · 2026-05-06 · CC BY 4.0 · 1 min
The space around us isn’t a smooth sheet: it’s a bumpy blanket, and its contribution to expansion is 10% and isn’t weakening.

Under the influence of gravity, space dents like a stretched blanket: galaxies and their clusters create dips and bumps, and the main contribution to curvature comes from invisible dark matter (a discovery linked to Vera Rubin). Astronomers mapped local space using the motions of thousands of galaxies (from the Cosmicflows-4++ catalog, accounting for redshift and peculiar velocities) via computer simulations.

It turns out that curvature contributes roughly 10% to expansion and doesn’t taper off over distances up to a billion light-years. This contradicts the standard model, which, relying on the cosmic microwave background, assumes a smooth universe. Local bumps distort dark energy measurements by tens of percent — meaning we could be way off in our estimates. It’s astonishing that we live inside such a 'dent,' nested within an even larger void, like a cosmic matryoshka doll. Accounting for this relief will help refine the cosmic picture started by Edwin Hubble and Georges Lemaître.

Our universe resembles a matryoshka doll: we live inside a 'bubble' surrounded by a 'wall' of superclusters, which in turn is embedded in a giant void.

\Omega_M^{\mathcal{D}} + \Omega_\Lambda^{\mathcal{D}} + \Omega_R^{\mathcal{D}} + \Omega_Q^{\mathcal{D}} = 1
Ω_M — fraction of ordinary and dark matter, Ω_Λ — fraction of dark energy (cosmological constant), Ω_R — fraction of spatial curvature, Ω_Q — fraction of kinematic backreaction.
Scientists
Alan GuthAlexander FriedmannAndrei LindeGeorges LemaîtreJames PeeblesAdam Riess
Concepts
backreaction spatial curvature density contrast lambda cdm cosmological parameters curvature cosmic expansion energy reconstruction cosmological bounce cosmic chronometry spacetime emergence age of the universe hubble constant vacuum energy kilometer per second per megaparsec cosmology quantum cosmology universe matter density spacetime