Inflationary dynamics of kinetically-coupled gauge fields
arXiv:1411.5362 · doi:10.1088/1475-7516/2015/04/029
Abstract
We investigate the inflationary dynamics of two kinetically-coupled massless gauge fields with time-varying kinetic-term coefficients. Ensuring that the system does not have strongly coupled regimes shrinks the parameter space. Also, we further restrict ourselves to systems that can be quantized using the standard creation, annihilation operator algebra. This second constraint limits us to scenarios where the system can be diagonalized into the sum of two decoupled, massless, vector fields with a varying kinetic-term coefficient. Such a system might be interesting for magnetogenesis because of how the strong coupling problem generalizes. We explore this idea by assuming that one of the gauge fields is the Standard Model field and that the other dark gauge field has no particles charged under its gauge group. We consider whether it would be possible to transfer a magnetic field from the dark sector, generated perhaps before the coupling was turned on, to the visible sector. We also investigate whether the simple existence of the mixing provides more opportunities to generate magnetic fields. We find that neither possibility works efficiently, consistent with the well-known difficulties in inflationary magnetogenesis.
arXiv comment17 pages, 0 figures. Matches JCAP version
References in corpus (28)
- Astrophysical magnetic fields and nonlinear dynamo theory
- Evidence for strong extragalactic magnetic fields from Fermi observations of TeV blazars
- Cosmological Magnetic Fields: Their Generation, Evolution and Observation
- The intergalactic magnetic field constrained by Fermi/LAT observations of the TeV blazar 1ES 0229+200
- EGMF Constraints from Simultaneous GeV-TeV Observations of Blazars
- Lower limit on the strength and filling factor of extragalactic magnetic fields
- Generation of Large-Scale Magnetic Fields in Single-Field Inflation
- Magnetic fields from inflation?
- Instability of anisotropic cosmological solutions supported by vector fields
- The First Magnetic Fields
- The anisotropic power spectrum and bispectrum in the f(phi) F^2 mechanism
- Cosmological Magnetic Fields from Inflation and Backreaction
- Observable non-gaussianity from gauge field production in slow roll inflation, and a challenging connection with magnetogenesis
- Magnetic fields in the early universe
- Instability of the ACW model, and problems with massive vectors during inflation
- Inflationary Magnetogenesis without the Strong Coupling Problem
- Vector theories in cosmology
- Signatures of anisotropic sources in the squeezed-limit bispectrum of the cosmic microwave background
- Inflationary Magnetogenesis without the Strong Coupling Problem II: Constraints from CMB anisotropies and B-modes
- Vector Curvaton without Instabilities
- Higher order statistics of curvature perturbations in IFF model and its Planck constraints
- Consistency relation for cosmic magnetic fields
- On the non-Gaussian correlation of the primordial curvature perturbation with vector fields
- Critical constraint on inflationary magnetogenesis
- A scenario for inflationary magnetogenesis without strong coupling problem
- Constraints on Gauge Field Production during Inflation
- Probing correlations of early magnetic fields using mu-distortion
- Inflationary susceptibilities, duality and large-scale magnetic fields generation
Cited by in corpus (12)
- Consistent generation of magnetic fields in axion inflation models
- Pre-reheating Magnetogenesis in the Kinetic Coupling Model
- Stable solutions of inflation driven by vector fields
- Constraints on Primordial Magnetic Fields from Inflation
- Primordial perturbations from dilaton-induced gauge fields
- Inflationary magnetogenesis, derivative couplings and relativistic Van der Waals interactions
- Inflationary magnetogenesis in the perturbative regime
- Large-scale gauge spectra and pseudoscalar couplings
- Statistical anisotropy from inflationary magnetogenesis
- Spectator Higgs, large-scale gauge fields and the non-minimal coupling to gravity
- Effective horizons, junction conditions and large-scale magnetism
- Squeezed relic photons beyond the horizon