The cosmological principle is not in the sky
Chan-Gyung Park, Hwasu Hyun, Hyerim Noh, Jai-chan Hwang

TL;DR
This study tests the assumption of large-scale homogeneity in the universe using galaxy data and finds significant deviations from homogeneity, challenging the foundational cosmological principle.
Contribution
It provides the first direct observational test showing the universe's large-scale structure is not homogeneous, questioning a core assumption of modern cosmology.
Findings
Galaxy counts show larger dispersions than random models up to 300 Mpc/h.
Average galaxy counts are outside the expected range for homogeneity.
Mock galaxy data from simulations are also inconsistent with homogeneity at large scales.
Abstract
The homogeneity of matter distribution at large scales, known as the cosmological principle, is a central assumption in the standard cosmological model. The case is testable though, thus no longer needs to be a principle. Here we perform a test for spatial homogeneity using the Sloan Digital Sky Survey Luminous Red Galaxies (LRG) sample by counting galaxies within a specified volume with the radius scale varying up to 300 Mpc/h. We directly confront the large-scale structure data with the definition of spatial homogeneity by comparing the averages and dispersions of galaxy number counts with allowed ranges of the random distribution with homogeneity. The LRG sample shows significantly larger dispersions of number counts than the random catalogues up to 300 Mpc/h scale, and even the average is located far outside the range allowed in the random distribution; the deviations are…
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