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

2025/08/13 by Zhu, Yigan, Gao, Qing, Gong, Yungui +1 · 9 citations
#Cosmology and Nongalactic Astrophysics (astro-ph.CO) #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc)

paper · doi:10.48550/arxiv.2508.09707

Abstract

Recent analyses combining Atacama Cosmology Telescope (ACT) data with other cosmological datasets report a higher scalar spectral index ns, creating tension with a wide range of inflationary models. Since a Gauss-Bonnet term with a coupling function ξ(ϕ) = 3λ/[4V(ϕ)] leaves ns nearly unchanged (up to a field rescaling) while reducing the tensor-to-scalar ratio r by a factor (1-λ), so choosing (1-λ) 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.

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