Bayesian constraints on inverse-tangent inflation with constant-EOS and dynamical reheating yield preferred kappa 0.5-0.6, Nk 40-60, and narrow ns-r region under consistency, linking early and late cosmology.
Cline,TASI Lectures on Early Universe Cosmology: Inflation, Baryogenesis and Dark Matter, arXiv:1807.08749 [hep-ph]
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Bayesian Constraints on Inverse-Tangent Inflation with Constant-EOS Reheating and a Dynamical Reheating Analysis
Bayesian constraints on inverse-tangent inflation with constant-EOS and dynamical reheating yield preferred kappa 0.5-0.6, Nk 40-60, and narrow ns-r region under consistency, linking early and late cosmology.