Inflation using a triplet of Antisymmetric tensor fields
arXiv:2212.13508 · doi:10.1140/epjc/s10052-023-11932-x
Abstract
We study an inflation model driven by a triplet of antisymmetric tensor fields, with minimal and nonminimal couplings to gravity. First, we show that the presence of a triplet of antisymmetric tensor fields can provide inherent background isotropy in the stress-energy tensor contrary to the past studies using an antisymmetric tensor field. Inflation is supported in the presence of non-minimal couplings with gravity. We perform the slow roll analysis and also analyse perturbations to the antisymmetric tensor field as well as the tensor modes of perturbed metric. The speed of gravitational waves manifested from the tensor perturbations is tuned to . We also study the evolution of the gravitational waves, calculate their power spectrum and tensor spectral index.
arXiv comment23 pages, 5 figures
References in corpus (44)
- Planck 2018 results. X. Constraints on inflation
- Cosmological perturbations
- Bounds on Slow Roll and the de Sitter Swampland
- Inflationary cosmology in modified gravity theories
- Vector Inflation
- The Nature of Primordial Fluctuations from Anisotropic Inflation
- Ghost instabilities of cosmological models with vector fields nonminimally coupled to the curvature
- Anisotropic Power-law Inflation
- The zoo plot meets the swampland: mutual (in)consistency of single-field inflation, string conjectures, and cosmological data
- Multiple field inflation
- Inflation from N-Forms and its stability
- Further refining the de Sitter swampland conjecture
- P-nflation: generating cosmic Inflation with p-forms
- Inflation with General Initial Conditions for Scalar Perturbations
- Three-form cosmology
- Anisotropic Non-Gaussianity from a Two-Form Field
- The inflationary universe in F(R) gravity with antisymmetric tensor fields and their suppression during the universe evolution
- Kerr/CFT Correspondence in the Low Energy Limit of Heterotic String Theory
- dS Vacua and the Swampland
- Stable solutions of inflation driven by vector fields
- Inflation with an antisymmetric tensor field
- Primordial bispectrum from inflation with background gauge fields
- Footprint of Two-Form Field: Statistical Anisotropy in Primordial Gravitational Waves
- Three-form inflation and non-Gaussianity
- On cosmic inflation in vector field theories
- Interferometer Constraints on the Inflationary Field Content
- The cosmology of the nonsymmetric theory of gravitation
- Instabilities in Horndeski Yang-Mills inflation
- Relaxing inflation models with non-minimal coupling: A general study
- Cuscuton Inflation
- Inflation with multiple vector fields and non-Gaussianities
- Inflation in mimetic gravity
- Observational constraints on assisted k-inflation
- Inflationary model in minimally modified gravity theories
- Hubble multi-scalar inflation
- Dynamics of inflation with mutually orthogonal vector fields in a closed universe
- Vector inflation by kinetic coupled gravity
- Vector Field and Inflation
- Exploring the inflation of gravity
- Avoiding instabilities in antisymmetric tensor field driven inflation
- Gravitational waves from inflation with antisymmetric tensor field
- Inflation with antisymmetric tensor field: new candidates
- Dark Energy with a Triplet of Classical U(1) Fields
- Analysis of Vector-Inflation Models Using Dynamical Systems