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arXiv · 1904.06135

Cosmological constraints from cosmic homogeneity

Pierros Ntelis·Adam James Hawken·Stephanie Escoffier·Anne Ealet·Andre Tilquin
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Abstract

In this paper, we study the normalised characteristic scale of transition to cosmic homogeneity, $\mathcal{R}_H/d_V$, as a cosmological probe. We use a compilation of SDSS galaxy samples, comprising more than $10^6$ galaxies in the redshift range $0.17 \leq z \leq 2.2$ within the largest comoving volume to date, $\sim 8 h^{-3}\mathrm{Gpc}^3$. We show that these samples can be described by a single bias model as a function of redshift. By combining our measurements with prior Cosmic Microwave Background and Lensing information from the Planck satellite, we constrain the total matter density ratio of the universe, $\Omega_m = 0.363 \pm 0.025$, and the Dark Energy density ratio, $\Omega_{\Lambda} = 0.649 \pm 0.021$, improving the values from Planck alone by 31% and 28%, respectively. Our results are compatible with a flat $\Lambda$CDM model. These results show the complementarity of the normalised homogeneity scale with other cosmological probes and open new roads to cosmometry.

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Pierros Ntelis, Adam James Hawken, Stephanie Escoffier, Anne Ealet, Andre Tilquin. 2019-04-12. Cosmological constraints from cosmic homogeneity. https://arxiv.org/abs/1904.06135

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