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.
|Pages (from-to)||37 - 40|
|Number of pages||4|
|Journal||Astronomy & Astrophysics|
|Publication status||Published - 2009|