The microwave background anisotropy and the homogeneity of the universe

Details The microwave background anisotropy and the homogeneity of the universe The microwave background anisotropy and the homogeneity of the universe

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..890m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Dec. 1984, p. 890-895) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Nov.-Dec

Astronomy and Astrophysics

Astronomy

Background Radiation, Cosmology, Relic Radiation, Universe, Anisotropy, Homogeneity, Perturbation

Scientific paper

The background radiation fluctuations due to scalar type cosmological perturbations are calculated using relativistic potential gauge. The observational upper limit of the quadrupole anisotropy of the background radiation restricts the characteristic scale of perturbations which are larger than the transparency region. The sizes of perturbations with amplitude of the order of unity must be at least forty-five times as large as the observational horizon.

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