CBR Anisotropy in an Open Inflation, CDM Cosmogony
Marc Kamionkowski, Bharat Ratra, David N. Spergel, Naoshi Sugiyama
Abstract
We compute the cosmic background radiation anisotropy, produced by energy-density fluctuations generated during an early epoch of inflation, in an open cosmological model based on the cold dark matter scenario. At Ω0 0.3 -- 0.4, the COBE normalized open model appears to be consistent with most observations.
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