(Lovelock) inflation: explaining the ACT data and equivalence to Higgs-Gauss-Bonnet inflation
arXiv:2512.21167 · doi:10.1016/j.physletb.2026.140746
Abstract
We revisit the Starobinsky model of inflation in light of recent data from the Atacama Cosmology Telescope (ACT), which indicates a potential preference for a slightly larger scalar spectral index than predicted by the standard scenario. We demonstrate that a natural one-parameter generalization to a quadratic model in the Lovelock invariant ( is the Gauss--Bonnet term), can effectively resolve this minor tension. Scalar-tensor formulation of this theory yields an Einstein-frame Starobinsky-type scalar potential augmented by Gauss--Bonnet and derivative couplings, which modify the inflationary slow-roll dynamics. We show that a non-zero coupling for the Gauss-Bonnet term can shift along a trajectory that brings the predictions into better agreement with the ACT likelihood. We also find that gravity, in its scalar-tensor formulation, is equivalent to Higgs inflation coupled to the Gauss--Bonnet term, and belongs to the Horndeski/galileon class of modified gravities. This work establishes the quadratic gravity as a compelling and physically motivated extension that preserves the successes of Starobinsky inflation while improving its fit to modern precision cosmological data.
v1: 8 pages, 1 figure. v2: 10 pages, 1 figure, accepted to PLB
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