CBR Anisotropy in an Open Inflation, CDM Cosmogony
Astrophysics
2009-10-22 v1 General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
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 0.3 -- 0.4, the COBE normalized open model appears to be consistent with most observations.
Cite
@article{arxiv.astro-ph/9406069,
title = {CBR Anisotropy in an Open Inflation, CDM Cosmogony},
author = {Marc Kamionkowski and Bharat Ratra and David N. Spergel and Naoshi Sugiyama},
journal= {arXiv preprint arXiv:astro-ph/9406069},
year = {2009}
}
Comments
(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