Primordial large-scale electromagnetic fields from Gravitoelectromagnetic Inflation
arXiv:0811.0993 · doi:10.1016/j.physletb.2009.03.027
Abstract
We investigate the origin and evolution of primordial electric and magnetic fields in the early universe, when the expansion is governed by a cosmological constant . Using the gravitoelectromagnetic inflationary formalism with , we obtain the power of spectrums for large-scale magnetic fields and the inflaton field fluctuations during inflation. A very important fact is that our formalism is {\em naturally non-conformally invariant}.
Accepted for publication in Physics Letters B
References in corpus (9)
- Magnetic field production during preheating at the electroweak scale
- Generation of Cosmological Seed Magnetic Fields from Inflation with Cutoff
- Effects of a Primordial Magnetic Field on Low and High Multipoles of the CMB
- Inflation-Produced Magnetic Fields in Nonlinear Electrodynamics
- Inflation-Produced Magnetic Fields in R^n F^2 and I F^2 models
- Scaling laws in decaying helical hydromagnetic turbulence
- The interrelation between the generation of large-scale electric fields and that of large-scale magnetic fields during inflation
- Property of the spectrum of large-scale magnetic fields from inflation
- An exact solution of the five-dimensional Einstein equations with four-dimensional de Sitter-like expansion