Gauge-flation and Cosmic No-Hair Conjecture
arXiv:1109.5573 · doi:10.1088/1475-7516/2012/01/016
Abstract
Gauge-flation, inflation from non-Abelian gauge fields, was introduced in [1,2]. In this work, we study the cosmic no-hair conjecture in gauge-flation. Starting from Bianchi-type I cosmology and through analytic and numeric studies we demonstrate that the isotropic FLRW inflation is an attractor of the dynamics of the theory and that the anisotropies are damped within a few e-folds, in accord with the cosmic no-hair conjecture.
24 pages, 18 figures
References in corpus (11)
- Inflationary Universe with Anisotropic Hair
- Vector Inflation
- Instability of anisotropic cosmological solutions supported by vector fields
- The Nature of Primordial Fluctuations from Anisotropic Inflation
- Scalar-Scalar, Scalar-Tensor, and Tensor-Tensor Correlators from Anisotropic Inflation
- Anisotropic Power-law Inflation
- Instability of the ACW model, and problems with massive vectors during inflation
- Imprints of anisotropic inflation on the cosmic microwave background
- Anisotropic Inflation from Charged Scalar Fields
- Inflation with stable anisotropic hair: is it cosmologically viable?
- Particle Production of Vector Fields: Scale Invariance is Attractive
Cited by in corpus (48)
- Gauge Fields and Inflation
- Revisiting Cosmic No-Hair Theorem for Inflationary Settings
- Inflation with stable anisotropic hair: is it cosmologically viable?
- Inflation with Multi-Vector-Hair: The Fate of Anisotropy
- Chiral Primordial Gravitational Waves from Dilaton Induced Delayed Chromo-natural Inflation
- Gauge-flation Vs Chromo-Natural Inflation
- Parity-violating CMB correlators with non-decaying statistical anisotropy
- Gauge-flation confronted with Planck
- δN Formalism in Anisotropic Inflation and Large Anisotropic Bispectrum and Trispectrum
- Low-Energy Effective Field Theory for Chromo-Natural Inflation
- Generalized SU(2) Proca Theory
- Chiral Gravity Waves and Leptogenesis in Inflationary Models with non-Abelian Gauge Fields
- Chromo-Natural Model in Anisotropic Background
- Initial conditions for Inflation in an FRW Universe
- Stable solutions of inflation driven by vector fields
- Curvature Perturbations in Anisotropic Inflation with Symmetry Breaking
- Parity Violating Statistical Anisotropy
- Chromo-Natural Inflation in the Axiverse
- On the stability and causality of scalar-vector theories
- Primordial Anisotropies in Gauged Hybrid Inflation
- Dynamical analysis of cosmological models with non-Abelian gauge vector fields
- Stability analysis of inflation with an SU(2) gauge field
- Non-Abelian -term dark energy and inflation
- Light propagation in inhomogeneous and anisotropic cosmologies
- How attractive is the isotropic attractor solution of axion-SU(2) inflation?
- Inflationary Dynamics with a Non-Abelian Gauge Field
- Anisotropic Einstein Yang-Mills Higgs Dark Energy
- Leptogenesis in Inflationary models with Non-Abelian Gauge Fields
- Massive Gauge-flation
- Constant-roll inflation in the generalized SU(2) Proca theory
- The isotropic attractor solution of axion-SU(2) inflation: Universal isotropization in Bianchi type-I geometry
- Dark Fermions and Spontaneous violation in -axion Inflation
- Anisotropic Massive Gauge-flation
- An Hamilton-Jacobi formulation of anisotropic inflation
- Anisotropic Scalar Field Dark Energy with a Disformally Coupled Yang-Mills Field
- Dynamics of inflation with mutually orthogonal vector fields in a closed universe
- Scale and shape dependent non-Gaussianity in the presence of inflationary vector fields
- Cosmic No-hair Conjecture and Inflation with an SU(3) Gauge Field
- Particle-like solutions in the generalized SU(2) Proca theory
- Anisotropic inflation in non-minimal kinetic coupling model
- Chromo-natural inflation supported by enhanced friction from Horndeski gravity
- Anisotropic warm inflation
- Inflationary buildup of a vector field condensate and its cosmological consequences
- \bf Formalism and Anisotropic Chaotic Inflation Power Spectrum
- How does SU()-natural inflation isotropize the universe?
- Induced Cosmological Anisotropies and CMB Anomalies by a non-Abelian Gauge-Gravity Interaction
- Active galaxies can make axionic dark energy
- Tensor Adiabatic Modes and Consistency Relations with Primordial Axion-Gauge Fields