Résumé
It is often claimed that the ultra-slow-roll regime of inflation, where the dynamics of the inflaton field are friction dominated, is a non-attractor and/or transient. In this work we carry out a phase-space analysis of ultra-slow roll in an arbitrary potential, V(φ). We show that while standard slow roll is always a dynamical attractor whenever it is a self-consistent approximation, ultra-slow roll is stable for an inflaton field rolling down a convex potential with MPl V′′>|V′| (or for a field rolling up a concave potential with MPl V′′<-|V′|). In particular, when approaching a flat inflection point, ultra-slow roll is always stable and a large number of \efolds may be realised in this regime. However, in ultra-slow roll, is not a unique function of φ as it is in slow roll and dependence on initial conditions is retained. We confirm our analytical results with numerical examples.
| langue originale | Anglais |
|---|---|
| Numéro d'article | 048 |
| journal | Journal of Cosmology and Astroparticle Physics |
| Volume | 2018 |
| Numéro de publication | 8 |
| Les DOIs | |
| état | Publié - 31 août 2018 |
| Modification externe | Oui |
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