• DOI:10.1088/1475-7516/2016/06/051
• Corpus ID: 67760137

Constraints on single-field inflation

@article{Pirtskhalava2015ConstraintsOS,
  title={Constraints on single-field inflation},
  author={David Pirtskhalava and Luca Santoni and Enrico Trincherini},
  journal={Journal of Cosmology and Astroparticle Physics},
  year={2015},
  volume={2016},
  pages={051 - 051}
}

• D. Pirtskhalava, Luca Santoni, E. Trincherini
• Published 5 November 2015
• Computer Science
• Journal of Cosmology and Astroparticle Physics

Many alternatives to canonical slow-roll inflation have been proposed over the years, one of the main motivations being to have a model, capable of generating observable values of non-Gaussianity. In this work, we (re-)explore the physical implications of a great majority of such models within a single, effective field theory framework (including novel models with large non-Gaussianity discussed for the first time below). The constraints we apply—both theoretical and experimental—are found to be rather robust, determined to a great extent by just three parameters: the coefficients of the quadratic EFT operators (δN)2 and δNδE, and the slow-roll parameter ε. This allows to significantly limit the majority of single-field alternatives to canonical slow-roll inflation. While the existing data still leaves some room for most of the considered models, the situation would change dramatically if the current upper limit on the tensor-to-scalar ratio decreased down to r < 10−2. Apart from inflationary models driven by plateau-like potentials, the single-field model that would have a chance of surviving this bound is the recently proposed slow-roll inflation with weakly-broken galileon symmetry. In contrast to canonical slow-roll inflation, the latter model can support r < 10−2 even if driven by a convex potential, as well as generate observable values for the amplitude of non-Gaussianity.