English

The attractive behaviour of ultra-slow-roll inflation

Cosmology and Nongalactic Astrophysics 2018-09-19 v2 General Relativity and Quantum Cosmology High Energy Physics - Theory

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)V(\phi). 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 MPlV>VM_{\scriptscriptstyle{\mathrm{Pl}}} V''>|V'| (or for a field rolling up a concave potential with MPlV<VM_{\scriptscriptstyle{\mathrm{Pl}}} V''<-|V'|). In particular, when approaching a flat inflection point, ultra-slow roll is always stable and a large number of ee-folds may be realised in this regime. However, in ultra-slow roll, ϕ˙\dot{\phi} is not a unique function of ϕ\phi as it is in slow roll and dependence on initial conditions is retained. We confirm our analytical results with numerical examples.

Keywords

Cite

@article{arxiv.1806.09553,
  title  = {The attractive behaviour of ultra-slow-roll inflation},
  author = {Chris Pattison and Vincent Vennin and Hooshyar Assadullahi and David Wands},
  journal= {arXiv preprint arXiv:1806.09553},
  year   = {2018}
}

Comments

23 pages, 6 figures, matches version published in JCAP