How much of the inflaton potential do we see?
Wessel Valkenburg

TL;DR
This paper analyzes the observable part of the inflaton potential using recent constraints, emphasizing a conservative approach that avoids assumptions about unobservable inflation phases, leading to broader applicability.
Contribution
It introduces a method focusing solely on the observable inflaton potential, contrasting with prior extrapolation-based approaches, thus providing more conservative and model-independent constraints.
Findings
Significant differences from previous extrapolation methods
Broader applicability to various inflation models
No assumptions about invisible e-folds of inflation
Abstract
We discuss the latest constraints on a Taylor-expanded scalar inflaton potential, obtained focusing on its observable part only. This is in contrast with other works in which an extrapolation of the potential is applied using the slow-roll hierarchy. We find significant differences. The results discussed here apply to a broader range of models, since no assumption about the invisible e-folds of inflation has to be made, thereby remaining conservative.
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Taxonomy
TopicsAdvanced Thermodynamics and Statistical Mechanics · Stellar, planetary, and galactic studies · Photoreceptor and optogenetics research
