Minimizing the tensor-to-scalar ratio in single-field inflation models

Abstract

We revisit a class of simple single-field inflation models and demonstrate that they can readily produce a negligible tensor/scalar ratio $r$. Motivated by recent work suggesting the need to introduce higher order operators to stabilise unregulated potentials, as well as by work indicating that such terms can have significant effects on observable predictions, we explicitly construct corrected versions of the quadratic hilltop potential that are motivated by an effective field theory expansion. We employ Markov Chain Monte Carlo (MCMC) methods and optimization techniques to sample viable models and minimize $r$. We find that such potentials can readily lower $r$ values below projected CMB-S4 sensitivity, while still remaining within observable constraints on $n_s$. Furthermore, we find that the minimum $r$ reached for each order of the expansion considered is well-described by a power law $r_{min}(q)\propto q^{-B}$ before asymptoting to a value of $r_{min}\sim 10^{-11}$, where $q$ is the order to which the expansion of $V(\varphi )$ is carried out.

Updated to match published version

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Cited by in corpus (8)

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• Matching current observational constraints with nonminimally coupled dark energy
• Robustness of dark energy phenomenology across different parameterizations
• Non-minimal coupling in light of ACT
• Inflationary attractors and radiative corrections in light of ACT data
• The Spectre of Underdetermination in Modern Cosmology
• Mutated hilltop inflation in light of Planck/ACT observations
• Probing single-field inflation: predictions, constraints, and theoretical viewpoints