Observational Constraints on Open Inflation Models
arXiv:astro-ph/9608177 · doi:10.1103/PhysRevLett.77.4704
Abstract
We discuss observational constraints on models of open inflation. Current data from large-scale structure and the cosmic microwave background prefer models with blue spectra and/or Omega_0 >= 0.3--0.5. Models with minimal anisotropy at large angles are strongly preferred.
4 pages, RevTeX, with 2 postscript figures included. Second Figure corrected