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Cosmic background radiation anisotropy in an open inflation, cold dark matter cosmogony
1994
Astrophysical Journal
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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 $\Omega_0 \sim$ 0.3 -- 0.4, the COBE normalized open model appears to be consistent with most observations.
doi:10.1086/187558
fatcat:sorh3555ije4lovayzilw5krjm