Braneworld inflation with effective α-attractor potential
arXiv:1807.07443 · doi:10.1103/PhysRevD.99.103523
Abstract
In this paper, we study inflation with α-attractor potential in the RS braneworlds where high energy corrections to the Friedmann equation facilitate slow roll. In this scenario, we numerically investigate the inflationary parameters and show that the high energy brane corrections have significant effect on the parameter α, namely, the lower values of the parameter are preferred by observation in this limit. We find that the sub-Planckian values of the field displacement can be achieved by suitably constraining the brane tension.
arXiv comment12 pages, 5 figures, Minor corrections the revised version, to appear in PRD
References in corpus (42)
- Planck 2015 results. XIII. Cosmological parameters
- A Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- The Hierarchy Problem and New Dimensions at a Millimeter
- Dynamics of dark energy
- Cosmological Tracking Solutions
- The Einstein Equations on the 3-Brane World
- Non-conventional cosmology from a brane-universe
- Brane cosmological evolution in a bulk with cosmological constant
- BICEP2 / Keck Array VI: Improved Constraints On Cosmology and Foregrounds When Adding 95 GHz Data From Keck Array
- Quintessential inflation
- Cosmological Expansion in the Presence of an Extra Dimension
- Cosmology of One Extra Dimension with Localized Gravity
- Chaotic inflation on the brane
- BICEP2 / Keck Array x: Constraints on Primordial Gravitational Waves using Planck, WMAP, and New BICEP2/Keck Observations through the 2015 Season
- Minimal Supergravity Models of Inflation
- The Four-Year COBE Normalization and Large-Scale Structure
- Brane-world cosmology
- A universal attractor for inflation at strong coupling
- Gravitational waves from inflation on the brane
- Relic Gravity Waves from Braneworld Inflation
- Steep inflation: ending braneworld inflation by gravitational particle production
- Dark energy, -attractors, and large-scale structure surveys
- Quintessential Inflation with -attractors
- Four-year COBE normalization of inflationary cosmologies
- Quintessential Inflation on the Brane and the Relic Gravity Wave Background
- Emergent scale symmetry: Connecting inflation and dark energy
- Instant Preheating in Quintessential Inflation with -Attractors
- Unification of inflation and dark energy {\it à la} quintessential inflation
- The Curvaton Hypothesis and the eta-problem of Quintessential Inflation, with and without Branes
- Higher Order Corrections in Minimal Supergravity Models of Inflation
- Constraints on braneworld inflation from CMB anisotropies
- Universality and Thouless energy in the supersymmetric Sachdev-Ye-Kitaev Model
- Mirage effects on the brane
- Dark energy from -attractors: phenomenology and observational constraints
- Inflaton potential reconstruction in the braneworld scenario
- Random Potentials and Cosmological Attractors
- Preinflationary dynamics of attractor in loop quantum cosmology
- Sourcing Dark Matter and Dark Energy from -attractors
- Inflationary generalized Chaplygin gas and dark energy in the light of the Planck and BICEP2 experiments
- Observational constraints on the generalized attractor model
- Dark energy and possible alternatives
Cited by in corpus (9)
- Sound from extra dimension: quasinormal modes of thick brane
- Baryogenesis in the paradigm of quintessential inflation
- What is needed of a scalar field if it is to unify inflation and late time acceleration ?
- Quasinormal modes and echoes of a double braneworld
- -attractor from superconformal E-models in brane inflation
- Characteristic modes of thick brane model: resonances and quasinormal modes
- Emergence of cosmological scaling behavior in asymptotic regime
- Graviscalar quasinormal modes and asymptotic tails of a thick brane
- Helical phase inflation and its observational constraints