A non-Friedmannian model of the universe

Details A non-Friedmannian model of the universe A non-Friedmannian model of the universe

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988baicz..39..185m&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 39, May 1988, p. 185-188.

Mathematics

Logic

2

Astronomical Models, Relic Radiation, Universe, Anisotropy, Galactic Structure, Hubble Constant

Scientific paper

An inhomogeneous nonstandard model of the visible part of the universe (Meszaros, 1983) is presented in which the inhomogeneities are considered to be a property of Tolman's background. The anisotropy effects observed in the Hubble flow and cosmic background radiation are interpreted as perturbative inhomogeneities on the homogeneous Friedmannian background in standard cosmological models. This non-Friedmannian model assumes that the observable part of the universe is inside a giant but finite anticollapsing spherical body called the M-Galaxy.

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