Improved limits on anisotropy and inhomogeneity from the cosmic background radiation

Details Improved limits on anisotropy and inhomogeneity from the cosmic background radiation Improved limits on anisotropy and inhomogeneity from the cosmic background radiation

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phrvd..51.5942m&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 51, Issue 10, 15 May 1995, pp.5942-5945

Other

32

Galaxy Groups, Clusters, And Superclusters, Large Scale Structure Of The Universe, Background Radiations

Scientific paper

Recently we presented limits on the deviation of the Universe from a Friedmann-Robertson-Walker form, which are implied directly by anisotropies in the cosmic background radiation, without assuming inflationary or other models of evolution. Here we weaken some of our previous assumptions, ensuring that all assumptions are in principle observational, and obtain improved limits.

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