October 1, 1994Open Access
Cosmic background radiation anisotropy in an open inflation, cold dark matter cosmogony
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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 ₀ 0. 3 -- 0. 4, the COBE normalized open model appears to be consistent with most observations.