Three-form cosmology

Abstract

Cosmology of self-interacting three-forms is investigated. The minimally coupled canonical theory can naturally generate a variety of isotropic background dynamics, including scaling, possibly transient acceleration and phantom crossing. An intuitive picture of the cosmological dynamics is presented employing an effective potential. Numerical solutions and analytical approximations are provided for scenarios which are potentially important for inflation or dark energy.

6 pages, 2 figures; V2: typos corrected, refs added, to appear in PLB

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Cited by in corpus (59)

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• Generalized hybrid metric-Palatini gravity
• Inflation from N-Forms and its stability
• Non-Gaussianity and statistical anisotropy from vector field populated inflationary models
• Coupled quintessence with a $\Lambda$CDM background: removing the ${\sigma }_8$ tension
• Gauge-flation trajectories in Chromo-Natural Inflation
• Dynamics of dark energy models and centre manifolds
• Cosmology for quadratic gravity in generalized Weyl geometry
• Coupled three-form dark energy
• Constraining anisotropic models of the early Universe with WMAP9 data
• Interacting 3-form dark energy models: distinguishing interactions and avoiding the Little Sibling of the Big Rip
• Stable solutions of inflation driven by vector fields
• Wormhole geometries supported by three-form fields
• Revisiting the Stability of Quadratic Poincaré Gauge Gravity
• Linear perturbations in vector inflation and stability issues
• Stability of the 3-form field during inflation
• Cosmic infinity: A dynamical system approach
• Statistical Anisotropy and the Vector Curvaton Paradigm
• Traversable Wormhole in Einstein 3-Form Theory With Self-Interacting Potential
• The dark side of the torsion: Dark Energy from propagating torsion
• Reheating in 3-form inflation
• Inflation in a two 3-form fields scenario
• Regular Black Hole Interior Spacetime Supported by Three-Form Field
• Three-form inflation and non-Gaussianity
• On cosmic inflation in vector field theories
• 3-form inflation in Randall-Sundrum II
• Three-magnetic fields
• Quantum behavior of the "Little Sibling" of the Big Rip induced by a three-form field
• Disformal vectors and anisotropies on a warped brane
• Non-Gaussianity in multiple three-form field inflation
• Arbitrarily coupled $p-$forms in cosmological backgrounds
• Anisotropic inflation with coupled $\mathbf{p}$-forms
• Perfect fluid in Lagrangian formulation due to generalized three-form field
• Perturbations and non-Gaussianities in three-form inflationary magnetogenesis
• Black hole and naked singularity geometries supported by three-form fields
• A power-law coupled three-form dark energy model
• Rotating traversable wormhole geometries in the presence of three-form fields
• Doubly-boosted vector cosmologies from disformal metrics
• Cosmology with a Continuous Tower of Scalar Fields
• Coupled Quintessence scalar field model in light of observational datasets
• The anisotropy of a three- and a one-form
• A coupled generalized three-form dark energy model
• Transient dark energy, cosmological constant boundary crossing and dark energy $w(z)$ data fits
• Screening three-form fields
• Inflation with antisymmetric tensor field: new candidates
• Gravitational lensing by traversable wormholes supported by three-form fields
• Quantum Yang-Mills Condensate Dark Energy Models
• Inflation using a triplet of Antisymmetric tensor fields
• Cosmological correlation functions in scalar and vector inflationary models
• Scalar and vector modes in inflation with antisymmetric tensor field
• Non-canonical 3-form dark energy
• Generalized Three-Form Field
• Aspects of time evolution in $p$-form field theories
• Hamiltonian formalism and constraint analysis of three-form matter models coupled with general relativity
• Vector wormholes as conduits for matter interaction
• New effective theories of gravitation and their phenomenological consequences
• Scaling solutions in three-form cosmology