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Backreaction and the Role of Spatial Curvature in the Cosmic Neighborhood

  • Authors: Marco Galoppo, Thomas Buchert, Pierre Mourier

Marco Galoppo et al 2026 The Astrophysical Journal Letters 1002 .

  • Provider: AAS Journals

Caption: Figure 1.

Expansion rate (Θ/3, top-left panel), shear scalar amplitude (﹩\sqrt{2{\sigma }^{2}}﹩, top-right panel), matter density (ρ, bottom-left panel), and spatial scalar curvature (﹩{ \mathcal R }﹩, bottom-right panel) on the supergalactic plane as functions of the supergalactic comoving-distance coordinates SGX, SGY, from the CF4++ reconstruction. In all panels, the white cross marker at the center indicates the observer’s position.

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