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The Lyth Bound of Inflation with a Tilt

Published 28 Aug 2014 in hep-th, astro-ph.CO, gr-qc, and hep-ph | (1408.6839v2)

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 r≲2⋅10<sup>−3r \lesssim 2 \cdot 10<sup>{-3}, we find that n=0.96n=0.96 brings this down to r≲2⋅10<sup>−5r \lesssim 2 \cdot 10<sup>{-5}.

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