Primordial Magnetic Fields from Dark Energy

Abstract

Evidences indicate that the dark energy constitutes about two thirds of the critical density of the universe. If the dark energy is an evolving pseudo scalar field that couples to electromagnetism, a cosmic magnetic seed field can be produced via spinoidal instability during the formation of large-scale structures.

Discussion on back reaction is added to match the published version

References in corpus (9)

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Cited by in corpus (19)

• Evolution of Primordial Magnetic Fields from Phase Transitions
• Opening up the QCD axion window
• Gravitational wave probes of axion-like particles
• Helical Magnetic Fields from Inflation
• Magnetic Helicity Generation from the Cosmic Axion Field
• Evolution of inflation-generated magnetic field through phase transitions
• Magnetic field generation from non-equilibrium phase transitions
• Coupling Quintessence to Inflation in Supergravity
• Large scale magnetogenesis from a non-equilibrium phase transition in the radiation dominated era
• Constraining Evolution of Quintessence with CMB and SNIa Data
• Bound on the time variation of the fine structure constant driven by quintessence
• Evolution of primordial magnetic fields in mean-field approximation
• The Dynamical Mixing of Light and Pseudoscalar Fields
• Nonequilibrium dynamics of moving mirrors in quantum fields: Influence functional and Langevin equation
• Electrodynamics of a Cosmic Dark Fluid
• Vacuum fluctuations in an ancestor vacuum: A possible dark energy candidate
• Cosmological Ohm's law and dynamics of non-minimal electromagnetism
• Nonlinear axion electrodynamics: Axionically induced electric flares in the early magnetized universe
• Density perturbation and cosmological evolution in the presence of magnetic field in $f(R)$ gravity models