Inflation in light of ACT/SPT: a new perspective from Weyl gravity

TL;DR

This paper introduces a Weyl gravity-based inflationary model that naturally aligns with recent ACT and SPT measurements, providing a new perspective on primordial scalar perturbations and scale invariance.

Contribution

It proposes a novel inflation scenario using Weyl scale-invariant gravity with exponential curvature extensions, matching observational constraints.

Findings

Predicted spectral index n_s~0.97-0.975 consistent with ACT/SPT

Weyl gravity provides a natural framework for inflation

Imprints of primordial symmetry in the cosmic microwave background

Abstract

Recent measurements from the Atacama Cosmology Telescope (ACT) and the South Pole Telescope (SPT) have placed the strictest constraints on the primordial scalar perturbation spectrum, reporting a spectral index of $n_s\sim0.967-0.98$ at 95% confidence level. This result indicates a stronger scale invariance of the scalar perturbation than earlier estimates, posing challenges for numerous inflation models. In this work, we propose a novel inflationary scenario based on Weyl scale-invariant gravity, where the quadratic curvature establishes the scale invariance of the scalar spectrum, while the higher-order extensions imprint the observed slight deviation. Specifically, the exponential curvature extensions are introduced to suppress the mass divergence of the inflaton. We find such scenario naturally yields leading-order predictions of $n_s\simeq1-3/(2N)\sim0.97-0.975$ or $n_s\simeq1-5/(3N)\sim0.967-0.972$ for various models, in excellent agreement with the ACT/SPT constraints. This result builds a concrete bridge between theoretical and observational scale invariance, implying an enduring cosmic echo of the primordial symmetry.