CBR Anisotropy in an Open Inflation, CDM Cosmogony
arXiv:astro-ph/9406069 · doi:10.1086/187558
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 $Ω_0 \sim$ 0.3 -- 0.4, the COBE normalized open model appears to be consistent with most observations.
(12 pages, plain TeX; 3 figures available upon request from the authors), IASSNS-HEP-94/39, PUPT-1470, POP-568, CfPA-TH-94-27, UTAP-185