Scalar Field Assisted Gravity Inflation
arXiv:1803.10748 · doi:10.1142/S0219887818501372
Abstract
In this paper we investigate the inflationary dynamics of an gravity in the presence of a canonical scalar field. We specifically choose the cosmological evolution to be a quasi-de Sitter evolution and also the gravity is assumed to be a modified version of the gravity. We investigate which scalar field potential can produce the quasi-de Sitter evolution for the choice of the gravity we made, and also we study in detail the inflationary dynamics of the resulting theory. As we demonstrate, the spectral index is identical to the one corresponding to the ordinary gravity, while the scalar-to-tensor ratio is found to be smaller than the inflation one consequently, compatibility with both the Planck 2015 and BICEP2/Keck-Array data is achieved.
References in corpus (19)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Modified Gravity and Cosmology
- Extended Theories of Gravity
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- The Standard Model Higgs boson as the inflaton
- Particle Physics Models of Inflation and the Cosmological Density Perturbation
- Universality Class in Conformal Inflation
- Superconformal Inflationary -Attractors
- BICEP2 / Keck Array VI: Improved Constraints On Cosmology and Foregrounds When Adding 95 GHz Data From Keck Array
- Inflationary Cosmology
- Minimal Supergravity Models of Inflation
- f(R) gravity theory and CMBR constraints
- A bird's eye view of f(R)-gravity
- Gauge-ready formulation of the cosmological kinetic theory in generalized gravity theories
- Singular Inflationary Universe from Gravity
- Inflationary spectra in generalized gravity: Unified forms
- Inflationary -attractors from Gravity
- Viable Mimetic Completion of Unified Inflation-Dark Energy Evolution in Modified Gravity
- Singular Cosmology Unifying Early and Late-time Acceleration with Matter and Radiation Domination Era
Cited by in corpus (5)
- Effects of Spatial Curvature on the Gravity Phase Space: no Inflationary Attractor?
- Swampland dS conjecture in Mimetic gravity
- Autonomous Dynamical System Description of de Sitter Evolution in Scalar Assisted Gravity
- Inflation in mimetic gravity
- Intermediate Coupling Regime in Dilatonic Inflationary Universe