Journal
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Volume -, Issue 8, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2018/08/048
Keywords
inflation; physics of the early universe
Funding
- U.K. Science and Technology Facilities Council grant [ST/N000668/1]
- European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant [750491]
- STFC [ST/N000668/1] Funding Source: UKRI
- Marie Curie Actions (MSCA) [750491] Funding Source: Marie Curie Actions (MSCA)
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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 (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 MP1V '' > vertical bar V'vertical bar (or for a field rolling up a concave potential with MP1V '' < -vertical bar V'vertical bar). In particular, when approaching a flat inflection point, ultra-slow roll is always stable and a large number of e-folds may be realised in this regime. However, in ultra-slow roll, phi is not a unique function of phi as it is in slow roll and dependence on initial conditions is retained. We confirm our analytical results with numerical examples.
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