Large-scale inhomogeneities in the universe and fluctuation spectra

Details Large-scale inhomogeneities in the universe and fluctuation spectra Large-scale inhomogeneities in the universe and fluctuation spectra

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..659g&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, Aug. 1991, p. 659-670. In Russian.

Statistics

Computation

1

Anisotropic Media, Background Radiation, Galactic Clusters, Interstellar Matter, Spectral Energy Distribution, Universe, Computational Astrophysics, Density Distribution, Power Spectra, Relic Radiation

Scientific paper

The requirements for the matter density fluctuation spectrum from the standpoint of the conformity of predicted and observed characteristics of the large-scale structure of the universe are analyzed. A spectrum is found for which the calculated correlation functions of galaxies and their clusters, large-scale galactic fluxes, and great attractor models are consistent with the observed quantities, and which agrees with present-day constraints on background radiation anisotropy.

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