Inflationary Models with Gauss-Bonnet Coupling in Light of ACT Observations

TL;DR

This paper explores how Gauss-Bonnet couplings in inflationary models can reduce the tensor-to-scalar ratio, helping models align with recent ACT observations and resolve existing tensions in cosmological data.

Contribution

It introduces a specific Gauss-Bonnet coupling mechanism that effectively lowers the tensor-to-scalar ratio in various inflationary models, improving their compatibility with current CMB constraints.

Findings

Gauss-Bonnet coupling reduces tensor-to-scalar ratio $r$ by a factor $(1- ext{lambda})$

Broad regions of parameter space in inflation models become consistent with ACT data

Gauss-Bonnet couplings help reconcile inflation models with recent cosmological observations

Abstract

Recent analyses combining Atacama Cosmology Telescope (ACT) data with other cosmological datasets report a higher scalar spectral index $n_s$, creating tension with a wide range of inflationary models. Since a Gauss-Bonnet term with a coupling function $\xi(\phi) = 3\lambda/[4V(\phi)]$ leaves $n_s$ nearly unchanged (up to a field rescaling) while reducing the tensor-to-scalar ratio $r$ by a factor $(1-\lambda)$, so choosing $(1-\lambda)$ sufficiently small effectively removes $r$ as a limiting observable, making it easier for inflationary models to satisfy the latest observational constraints and alleviating this tension. Applying this mechanism to chaotic inflation, E-models, T-models, and hilltop inflation, we find that broad regions of parameter space become consistent with the latest ACT-based CMB constraints. These results demonstrate that Gauss-Bonnet couplings can help bring a broad class of inflationary models into agreement with current CMB measurements.