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The attractive behaviour of ultra-slow-roll inflation

  • University of Portsmouth
  • Astroparticule and Cosmol APC

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

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 originaleAnglais
Numéro d'article048
journalJournal of Cosmology and Astroparticle Physics
Volume2018
Numéro de publication8
Les DOIs
étatPublié - 31 août 2018
Modification externeOui

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