Tabletop potentials for inflation from gravity
arXiv:2210.01828 · doi:10.1088/1475-7516/2023/03/023
Abstract
We show that a large class of modified gravity theories (MOG) with the Jordan-frame Lagrangian translate into scalar-field (scalaron) models with hilltop potentials in the Einstein frame. (A rare exception to this rule is provided by the Starobinsky model for which the corresponding scalaron potential is plateau-like for .) We find that MOG models featuring two distinct mass scales lead to scalaron potentials that have a flattened hilltop, or tabletop. Inflationary evolution in tabletop models agrees very well with CMB observations. Tabletop potentials therefore provide a new and compelling class of MOG-based inflationary models. By contrast, MOG models with a single mass scale generally correspond to steep hilltop potentials and fail to reproduce the CMB power spectrum. Inflationary evolution in hilltop/tabletop models can proceed in two alternative directions: towards the stable point at small describing the observable universe, or towards the asymptotic region at large . The MOG models which we examine have several new properties including the fact that gravity can become asymptotically vanishing, with , at infinite or large finite values of the scalar curvature . A universe evolving towards the asymptotically vanishing gravity region at large will either run into a 'Big-Rip' singularity, or inflate eternally.
35 pages, 11 figures, revised version, some clarifications and additional references, matches published version in JCAP
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