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LiteBIRD and CMB-S4 Sensitivities to Reheating in Plateau Models of Inflation
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abstract
We study the sensitivity of LiteBIRD and CMB-S4 to the reheating temperature and the inflaton coupling in three types of plateau-potential models of inflation, namely mutated hilltop inflation, radion gauge inflation, and $\alpha$-attractor T models. We first find relations between model parameters and CMB observables in all models. We then perform Monte Carlo Markov Chain based forecasts to quantify the information gain on the reheating temperature, the inflaton coupling, and the scale of inflation that can be achieved with LiteBIRD and CMB-S4, assuming a fiducial tensor-to-scalar ratio $\bar{r} \sim 0.02$ and neglecting foreground contamination of the B-mode polarization spectrum. We compare the results of the forecasts to those obtained from a recently proposed simple analytic method. We find that both LiteBIRD and CMB-S4 can simultaneously constrain the scale of inflation and the reheating temperature in all three types of models. They can for the first time obtain both an upper and lower bound on the latter, comprising the first ever measurement of the big bang temperature. In the mutated hilltop inflation and radion gauge inflation models this can be translated into a measurement of the inflaton coupling in parts of the parameter space. Constraining this microphysical parameter will help to understand how these models of inflation may be embedded into a more fundamental theory of particle physics.
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Cited by 3 Pith papers
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ACT DR6 Insights on the Inflationary Attractor models and Reheating
With ACT DR6 combined data, E-type alpha-attractors allow matter-like reheating, but T-type alpha-attractors require a stiff post-inflationary equation of state around w_phi=0.44 or higher.
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Constraining Reheating Temperature, Inflaton-SM Coupling and Dark Matter Mass in Light of ACT DR6 Observations
Using ACT DR6 plus Planck, BICEP/Keck and DESI data, the authors update bounds on alpha-attractor reheating temperature, inflaton-SM couplings, and gravitationally produced dark matter mass.
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Perturbative analysis of the reheating dynamics of $\alpha$-attractors
Reheating temperatures, e-folds, and inflaton masses in alpha-attractor models are computed via perturbative decay formulas, showing how they vary with the spectral index n_s and Yukawa coupling y.
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