Planck Limits on Non-canonical Generalizations of Large-field Inflation Models
arXiv:1609.08959 · doi:10.1088/1475-7516/2017/04/006
Abstract
In this paper, we consider two case examples of Dirac-Born-Infeld (DBI) generalizations of canonical large-field inflation models, characterized by a reduced sound speed, . The reduced speed of sound lowers the tensor-scalar ratio, improving the fit of the models to the data, but increases the equilateral-mode non-Gaussianity, , which the latest results from the Planck satellite constrain by a new upper bound. We examine constraints on these models in light of the most recent Planck and BICEP/Keck results, and find that they have a greatly decreased window of viability. The upper bound on corresponds to a lower bound on the sound speed and a corresponding lower bound on the tensor-scalar ratio of , so that near-future Cosmic Microwave Background observations may be capable of ruling out entire classes of DBI inflation models. The result is, however, not universal: infrared-type DBI inflation models, where the speed of sound increases with time, are not subject to the bound.
arXiv comment20 pages, 4 figures (v2: references added, version to appear in JCAP)
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