Abstract
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.
| Original language | English |
|---|---|
| Article number | 048 |
| Journal | Journal of Cosmology and Astroparticle Physics |
| Volume | 2018 |
| Issue number | 8 |
| DOIs | |
| Publication status | Published - 31 Aug 2018 |
| Externally published | Yes |
Keywords
- ination
- physics of the early universe
Fingerprint
Dive into the research topics of 'The attractive behaviour of ultra-slow-roll inflation'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver