On the problem of isotropization of cosmic microwave background radiation

Details On the problem of isotropization of cosmic microwave background radiation On the problem of isotropization of cosmic microwave background radiation

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...260...14g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 260, no. 1-2, p. 14-16.

Statistics

Computation

19

Perturbation Theory, Relic Radiation, Universe, Computational Astrophysics, Particle Theory

Scientific paper

An effect leading to a decrease of perturbations of microwave background radiation (MWB) after recombination epoch is investigated. Behavior of correlation functions for null geodesics flow enables one to evaluate the role of this effect based purely on geometrical and topological properties of the Universe. Possible anisotropy of MWB in open Friedmannian Universe is shown to be decreased due to this effect to a level far below present experimental accuracy.

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