Generation of large-scale magnetic fields from inflation in teleparallelism
arXiv:1208.0665 · doi:10.1088/1475-7516/2012/10/058
Abstract
We explore the generation of large-scale magnetic fields from inflation in teleparallelism, in which the gravitational theory is described by the torsion scalar instead of the scalar curvature in general relativity. In particular, we examine the case that the conformal invariance of the electromagnetic field during inflation is broken by a non-minimal gravitational coupling between the torsion scalar and the electromagnetic field. It is shown that for a power-law type coupling, the magnetic field on 1 Mpc scale with its strength of G at the present time can be generated.
18 pages, no figure, version accepted for publication in JCAP
References in corpus (36)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Dark torsion as the cosmic speed-up
- Modified teleparallel gravity: inflation without inflaton
- Einstein's Other Gravity and the Acceleration of the Universe
- On Born-Infeld Gravity in Weitzenbock spacetime
- Generation of Large-Scale Magnetic Fields in Single-Field Inflation
- Magnetic fields from inflation?
- Modified gravity models of dark energy
- models with phantom divide line crossing
- Inflation and late-time cosmic acceleration in non-minimal Maxwell- gravity and the generation of large-scale magnetic fields
- Inflationary cosmology and the late-time accelerated expansion of the universe in non-minimal Yang-Mills- gravity and non-minimal vector- gravity
- Large-scale magnetic fields in the inflationary universe
- Cosmological Magnetic Field: a fossil of density perturbations in the early universe
- The phenomenological approach to modeling the dark energy
- Universal upper limit on inflation energy scale from cosmic magnetic field
- Effects of a Primordial Magnetic Field on Low and High Multipoles of the CMB
- Faraday Rotation Limits on a Primordial Magnetic Field from WMAP Five-Year Data
- Inflation-Produced Magnetic Fields in Nonlinear Electrodynamics
- Inflation-Produced Magnetic Fields in R^n F^2 and I F^2 models
- Primordial Magnetic Field Limits from Cosmic Microwave Background Bispectrum of Magnetic Passive Scalar Modes
- Can Gravity Probe B usefully constrain torsion gravity theories?
- Generalized dark gravity
- Primordial magnetic fields and nonlinear electrodynamics
- Cosmological magnetic fields from nonlinear effects
- Large-scale magnetic fields from inflation due to Chern-Simons-like effective interaction
- The interrelation between the generation of large-scale electric fields and that of large-scale magnetic fields during inflation
- Primordial magnetic fields from second-order cosmological perturbations: Tight coupling approximation
- Property of the spectrum of large-scale magnetic fields from inflation
- Cosmological Structure Formation Creates Large-Scale Magnetic Fields
- Constraints on the Primordial Magnetic Field from
- Constraining primordial magnetic fields with CMB polarization experiments
- Slow decay of magnetic fields in open Friedmann universes