English

The Lyth Bound of Inflation with a Tilt

High Energy Physics - Theory 2015-01-09 v2 Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Phenomenology

Abstract

We provide strong evidence for universality of the inflationary field range: given an accurate measurement of (ns,r)(n_s,r), one can infer Δϕ\Delta \phi in a model-independent way in the sub-Planckian regime for a range of universality classes of inflationary models. Both the tensor-to-scalar ratio as well as the spectral tilt are essential for the field range. Given the Planck constraints on nsn_s, the Lyth bound is strengthened by two orders of magnitude: whereas the original bound gives a sub-Planckian field range for r2103r \lesssim 2 \cdot 10^{-3}, we find that n=0.96n=0.96 brings this down to r2105r \lesssim 2 \cdot 10^{-5}.

Keywords

Cite

@article{arxiv.1408.6839,
  title  = {The Lyth Bound of Inflation with a Tilt},
  author = {Juan Garcia-Bellido and Diederik Roest and Marco Scalisi and Ivonne Zavala},
  journal= {arXiv preprint arXiv:1408.6839},
  year   = {2015}
}

Comments

5 pages, 3 figures. v2: refs added, PRD version