COBE-DMR-normalisation for Cosmological Constant Dominated Cold Dark Matter Models

Details COBE-DMR-normalisation for Cosmological Constant Dominated Cold Dark Matter Models COBE-DMR-normalisation for Cosmological Constant Dominated Cold Dark Matter Models

1995-02-06

arxiv.org/abs/astro-ph/9502035v1

Astronomy and Astrophysics

Astrophysics

uuencoded file containing 6 postscript files (10 pgs text, 4 figures, 1 table)

Scientific paper

The two-year COBE-DMR 53 and 90 GHz sky maps are used to determine the normalization of inflationary, cosmological constant dominated, cold dark matter models. Although the COBE-DMR data prefer a nearly critical value for the total density, low-density models with Omega_0 > 0.15 can not be rejected at a confidence level > 95%. We compare theoretical predictions for various large scale statistics, computed for a range of values of Omega_0 and h=0.5, or 0.8, to various measures of structure in the universe.

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