Logarithmically enhanced hyperbolic square-root deformation of Starobinsky inflation
arXiv:2603.14743
Abstract
We propose an enhanced hyperbolic square-root (HSQRT) deformation of the Starobinsky model in the context of gravity. The original HSQRT construction provided a globally regular modification of inflation, curing the strong-coupling singularity at negative curvatures while preserving the exponential slow-roll plateau at large positive curvatures. Motivated by recent cosmological data (ACT DR6 and DESI), we introduce a structurally minimal, rational-logarithmic enhancement. This enhancement modifies the deep UV asymptotic regime while preserving global tachyon-free stability, ghost freedom, and the recovery of general relativity at low curvatures. In the Einstein frame, the scalaron dynamics is described by a globally defined, Padé-regulated effective potential, , which exhibits the inverse-power asymptotic form at high curvatures, , with the strength of the deviation from the baseline HSQRT geometry governed by dimensionless parameter . We derive analytic expansions for the slow-roll observables, yielding a leading-order spectral index and a tensor-to-scalar ratio . For standard e-fold durations (), this model drives the spectral index directly into the newly favored observational window () and predicts an exceptionally small spectral running , establishing a viable target for next-generation CMB observatories.
20 pages, 8 figures