Constraining hybrid inflation models with WMAP three-year results
arXiv:astro-ph/0610074 · doi:10.1103/PhysRevD.75.027302
Abstract
We reconsider the original model of quadratic hybrid inflation in light of the WMAP three-year results and study the possibility of obtaining a spectral index of primordial density perturbations, , smaller than one from this model. The original hybrid inflation model naturally predicts in the false vacuum dominated regime but it is also possible to have when the quadratic term dominates. We therefore investigate whether there is also an intermediate regime compatible with the latest constraints, where the scalar field value during the last 50 e-folds of inflation is less than the Planck scale.
7 pages, 10 figures. V2: References added
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