Cosmic background radiation anisotropies from cosmic structures - Models based on the Tolman solution

Details Cosmic background radiation anisotropies from cosmic structures - Models based on the Tolman solution Cosmic background radiation anisotropies from cosmic structures - Models based on the Tolman solution

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...388..225p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 388, April 1, 1992, p. 225-233.

Astronomy and Astrophysics

Astrophysics

52

Anisotropy, Astronomical Models, Galactic Clusters, Relic Radiation, Einstein Equations, Gravitational Effects, Red Shift

Scientific paper

Anisotropies of the Cosmic Background Radiation resulting from second-order gravitational effects in structures like voids, the Great Attractor, and clusters of galaxies are investigated. Spherically symmetric models of the structures are based on the Tolman solution of Einstein equations. Predicted anisotropies of the order of 10 exp -7 to 10 exp -6 are below the sensitivity of present observations.

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