The power spectrum of the cosmic microwave background Kolmogorov maps: possible clue to correlation of voids

TL;DR

This study analyzes the power spectrum of Kolmogorov stochasticity maps derived from WMAP's CMB data to explore potential correlations among cosmic voids, providing insights into large-scale structure formation.

Contribution

It introduces the use of Kolmogorov maps for CMB analysis to detect void correlations, a novel approach linking stochasticity parameters to matter distribution.

Findings

Power spectrum reveals possible void correlations.

Some features differ from simulated maps.

Method shows potential despite resolution limits.

Abstract

The power spectrum is obtained for the Kolmogorov stochasticity parameter map for WMAP's cosmic microwave background (CMB) radiation temperature datasets. The interest for CMB Kolmogorov map is that it can carry direct information about voids in the matter distribution, so that the correlations in the distribution of voids have to be reflected in the power spectrum. Although limited by the angular resolution of the WMAP, this analysis shows the possibility of acquiring this crucial information via CMB maps. Even the already obtained behavior, some of which is absent in the simulated maps, can influence the development of views on the void correlations at the large-scale web formation.