Endlessly flat scalar potentials and -attractors
arXiv:1607.00398 · doi:10.1016/j.physletb.2016.08.024
Abstract
We consider a minimally-coupled inflationary theory with a general scalar potential containing a stationary point of maximal order . We show that asymptotically flat potentials can be associated to stationary points of infinite order and discuss the relation of our approach to the theory of -attractors.
8 pages, 2 figures
References in corpus (14)
- Particle Physics Models of Inflation and the Cosmological Density Perturbation
- The Unity of Cosmological Attractors
- Particle physics models of inflation and curvaton scenarios
- MSSM flat direction inflation: slow roll, stability, fine tunning and reheating
- Multi-field Conformal Cosmological Attractors
- Cosmological Attractors and Initial Conditions for Inflation
- Planck, LHC, and -attractors
- Single-field -attractors
- On the geometrical interpretation of scale-invariant models of inflation
- Generalized Pole Inflation: Hilltop, Natural, and Chaotic Inflationary Attractors
- Pole Inflation - Shift Symmetry and Universal Corrections
- Inflationary quasi-scale invariant attractors
- Saddle point inflation from theory
- Implications of extreme flatness in a general f(R) theory
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