Recognition: unknown
CBR Anisotropy in an Open Inflation, CDM Cosmogony
classification
🌌 astro-ph
gr-qchep-ph
keywords
openanisotropyinflationmodelappearsbackgroundcobecold
read the original 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 $\Omega_0 \sim$ 0.3 -- 0.4, the COBE normalized open model appears to be consistent with most observations.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.