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Constraints on attractor models of inflation and reheating from Planck, BICEP/Keck, ACT DR6, and SPT-3G data

John Ellis*

Marcos A. G. Garcia†

Keith A. Olive‡

Sarunas Verner§

  • Theoretical Particle Physics and Cosmology Group, Department of Physics, King’s College London, London WC2R 2LS, United Kingdom and Theoretical Physics Department, CERN, CH-1211 Geneva 23, Switzerland

  • William I. Fine Theoretical Physics Institute, School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA

  • Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637, USA

  • *Contact author: John.Ellis@cern.ch
  • †Contact author: marcos.garcia@fisica.unam.mx
  • ‡Contact author: olive@umn.edu
  • §Contact author: verner@uchicago.edu

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 ns and tensor-to-scalar ratio r 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 (α-Starobinsky) and T-model potentials. The observational constraints accommodate E-models with α≲25, with the canonical Starobinsky model (α=1) predicting ns=0.958–0.963 for reheating temperatures between 100−1010  GeV, 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 ns values (0.956–0.961), in some tension with Planck 2018 data, and we find an upper limit of α≲11 in these models. We extend our analysis to generalized α-attractors with monomial potentials V(φ)∝φk near the minimum, demonstrating that models with k≥6 naturally predict ns≃0.965–0.968 for typical number of e-folds, in better agreement with the ACT DR6 data. We also consider deformed E- and T-models, which allow significantly higher values of ns for low values of α≃1.

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