Oscillating Inflation with a non-minimally coupled scalar field
arXiv:hep-th/9909106 · doi:10.1103/PhysRevD.61.027301
Abstract
The oscillating inflation model recently proposed by Damour and Mukhanov is investigated with a non-minimal coupling. Numerical study confirms an inflationary behavior and the density perturbation is obtained. A successful inflation requires the gravity-dilaton coupling to be small.
9 pages, 1 figure, to be published in PRD
Cited by in corpus (15)
- Extended Theories of Gravity
- Dynamical and Gravitational Instability of Oscillating-Field Dark Energy and Dark Matter
- Imperfect fluid description of modified gravities
- Cosmological perturbations in coherent oscillating scalar field models
- A crucial ingredient of inflation
- Steep Inflation followed by Born-Infeld Reheating
- The false vacuum bubble nucleation due to a nonminimally coupled scalar field
- Tachyon Inflation in Teleparallel Gravity
- Non-Gaussianities of Single Field Inflation with Non-minimal Coupling
- Energy conditions and classical scalar fields
- Can the Big Bang Singularity be avoided by a single scalar field?
- Warm inflation with an oscillatory inflaton in the non-minimal kinetic coupling model
- Inflation in Weyl Scaling Invariant Gravity with Extensions
- Quasilocal mass in scalar-tensor gravity: spherical symmetry
- Consistency of Anisotropic Inflation during Rapid Oscillations with Planck 2015 Data