COBE-DMR-normalised Open Inflation, CDM Cosmogony

Details COBE-DMR-normalised Open Inflation, CDM Cosmogony COBE-DMR-normalised Open Inflation, CDM Cosmogony

1995-02-06

arxiv.org/abs/astro-ph/9502034v1

Astrophys.J.444:L65-L68,1995

Astronomy and Astrophysics

Astrophysics

uuencoded file containing 6 postscript files (11 pgs text, 4 figures, 1 table)

Scientific paper

10.1086/187861

Fourier analysis on a cut sky of the two-year COBE DMR 53 and 90 GHz sky maps (in galactic coordinates) is used to determine the normalisation of an open inflation model based on the cold dark matter scenario. The normalised model is compared to measures of large-scale structure in the universe. Although the DMR data alone does not provide sufficient discriminative power to prefer a particular value of the mass density parameter, the open model appears to be reasonably consistent with observations when Omega_0 ~ 0.3 - 0.4 and merits further study.

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