CBR anisotropy in an open inflation, CDM cosmogony

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.

inflation
cosmic background radiation: anisotropy
cosmological model
dark matter
numerical calculations: interpretation of experiments
bibliography

References(48)

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