The galaxy power spectrum take on spatial curvature and cosmic concordance
Sunny Vagnozzi, Eleonora Di Valentino, Stefano Gariazzo, Alessandro, Melchiorri, Olga Mena, Joseph Silk

TL;DR
This paper uses full-shape galaxy power spectrum data to constrain the Universe's spatial curvature, finding it to be flat within sub-percent precision and highlighting the importance of such measurements in cosmology.
Contribution
It introduces the use of full-shape galaxy power spectrum measurements to break degeneracies and constrain spatial curvature, providing results consistent with a flat universe.
Findings
Constrained spatial curvature to Omega_K=0.0023 ± 0.0028.
Found consistency with a flat universe within sub-percent precision.
Identified tension between Planck and galaxy power spectrum data under curved universe assumptions.
Abstract
The concordance of the CDM cosmological model in light of current observations has been the subject of an intense debate in recent months. The 2018 Planck Cosmic Microwave Background (CMB) temperature anisotropy power spectrum measurements appear at face value to favour a spatially closed Universe with curvature parameter . This preference disappears if Baryon Acoustic Oscillation (BAO) measurements are combined with Planck data to break the geometrical degeneracy, although the reliability of this combination has been questioned due to the strong tension present between the two datasets when assuming a curved Universe. Here, we approach this issue from yet another point of view, using measurements of the full-shape (FS) galaxy power spectrum, , from the Baryon Oscillation Spectroscopic Survey DR12 CMASS sample. By combining Planck data with FS measurements, we…
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