- Open Access
Constraints on attractor models of inflation and reheating from , BICEP/Keck, ACT DR6, and SPT-3G data
Phys. Rev. D 113, 063571 – Published 30 March, 2026
DOI: https://doi.org/10.1103/d35r-7bn8
Abstract
We analyze the latest cosmic microwave background (CMB) constraints on the scalar spectral index and tensor-to-scalar ratio from Planck 2018, BICEP/Keck 2018, the Atacama Cosmology Telescope Data Release 6 (ACT DR6), and the South Pole Telescope (SPT-3G) data, focusing on their implications for attractor models of inflation. We compare systematically observational bounds with theoretical predictions for both E-model (-Starobinsky) and T-model potentials. The observational constraints accommodate E-models with , with the canonical Starobinsky model () predicting for reheating temperatures between , in good agreement with Planck 2018 data and within the 95% CL region determined by the Planck-ACT-SPT combination, but below the 95% confidence region of the Planck-ACT-DESI combination. Higher reheating temperatures from near-instantaneous reheating improve the compatibility. T-models predict slightly lower values (0.956–0.961), in some tension with Planck 2018 data, and we find an upper limit of in these models. We extend our analysis to generalized -attractors with monomial potentials near the minimum, demonstrating that models with naturally predict for typical number of -folds, in better agreement with the ACT DR6 data. We also consider deformed E- and T-models, which allow significantly higher values of for low values of .
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