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. © ESO 2009.
The power spectrum of the cosmic microwave background Kolmogorov maps: Possible clue to correlation of voids / Gurzadyan, V. G.; Kashin, A. L.; Khachatryan, H. G.; Kocharyan, A. A.; Poghosian, E.; Vetrugno, D.; Yegorian, G.. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 0004-6361. - 506:3(2009), pp. L37-L40. [10.1051/0004-6361/200913141]
The power spectrum of the cosmic microwave background Kolmogorov maps: Possible clue to correlation of voids
Vetrugno D.;
2009-01-01
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. © ESO 2009.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione
