Waterfall steps in single-field alpha-attractor potentials increase the effective number of e-folds, raising ns toward 1 and lowering r along the curve r = 3 alpha (1 - ns)^2.
Localized Steps toward ACT-Favored Inflation
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abstract
Recent ACT measurements favor a scalar spectral index larger than the Planck value, posing a challenge to many single-field slow-roll inflation models. We show that a smooth, localized step in the inflaton potential can shift the predicted scalar spectral index and tensor-to-scalar ratio by displacing the field value at which the CMB pivot scale exits the horizon. This mechanism can move monomial and, in particular, plateau-like attractor models toward the ACT-favored region, whereas the induced shift remains insufficient in natural inflation. We derive semi-analytical expressions for the step-induced remapping and quantify the associated effective e-fold shift, finding that it can be comparable to, and in some cases exceed, the shift allowed by conservative reheating uncertainties.
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astro-ph.CO 1years
2026 1verdicts
ACCEPT 1representative citing papers
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Waterfall-modulated $\alpha$-attractors
Waterfall steps in single-field alpha-attractor potentials increase the effective number of e-folds, raising ns toward 1 and lowering r along the curve r = 3 alpha (1 - ns)^2.