Minimal Extensions of the alpha-Starobinsky Model: Reconciling ACT DR6 and Reheating Constraints
Nehla Shobcha, Norma Sidik Risdianto, Romy Hanang Setya Budhi
astro-ph.CO, gr-qc, hep-ph
Submitted: 2026-06-23
Comments: 8 pages, 2 Figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Reheating in Inflationary Cosmology: Theory and Applications
- Reheating after Inflation
- Thermal Production of Gravitinos
- Refined Predictions for Starobinsky Inflation and Post-inflationary Constraints in Light of ACT
- How long before the end of inflation were observable perturbations produced?
- Reheating and relic gravitational waves as remedies for degeneracies of non-canonical natural inflation
- Inflation Dynamics and Reheating
- Nonperturbative Dynamics Of Reheating After Inflation: A Review
- Perturbative analysis of the reheating dynamics of $\alpha$-attractors
- Planck 2018 results. VI. Cosmological parameters
- Planck 2018 results. X. Constraints on inflation
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- Bounds on very low reheating scenarios after Planck
- Starobinsky-like Inflationary Models as Avatars of No-Scale Supergravity
- Polynomial $\alpha$-attractors
- $\alpha$-attractor inflation: Models and predictions
- No-Scale Inflation
- Starobinsky Inflation: From Non-SUSY To SUGRA Realizations
- Unified No-Scale Attractors
- Cosmological Attractors from $\alpha$-Scale Supergravity
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