Minimal Extensions of the $α$-Starobinsky Model: Reconciling ACT DR6 and Reheating Constraints

Abstract: The latest combined data from the Atacama Cosmology Telescope (ACT) DR6, Planck, and DESI yields a scalar spectral index $n_s = 0.9743 \pm 0.0034$, which lies approximately $2σ$ above the prediction of the standard $α$-Starobinsky inflation model. To address this tension, we propose two minimal extensions that preserve the model's plateau structure and attractor properties: a multiplicative exponential modification and an additive polynomial deformation, both governed by a single small perturbative parameter $δ&gt;0$. We analytically derive the slow-roll parameters and inflationary observables up to second order in $δ$ and integrate them with reheating dynamics via the consistency equation. It is shown that the $δ$ term effectively shifts $n_s$ into the $1σ$ confidence region of the joint P-ACT-LB-BK18 dataset without violating the tensor-to-scalar ratio bound ($r &lt; 0.038$). The viable parameter space at $1σ$ requires $α\lesssim 35$ with $δ\sim \mathcal{O}(10<sup>{-2})$ for the exponential model, while the additive model requires $δ\sim \mathcal{O}(10<sup>{-3})$ for $p=1$ and $δ\sim \mathcal{O}(10<sup>{-4})$ for $p=2$. For the e-folding range $N_k \in [50, 65]$, the relevant reheating equation of state is $0&lt;ω<em>{\mathrm{re}}\le1$. All viable scenarios yield a reheating temperature $T</em>{\mathrm{re}} \sim 10<sup>9$ GeV, which is safely above the Big Bang Nucleosynthesis (BBN) bound and below the gravitino overproduction limit.