Gradient models of the axion-photon coupling
arXiv:1201.3009 · doi:10.1140/epjc/s10052-012-1895-3
Abstract
We establish an extended version of the Einstein - Maxwell - axion model by introducing into the Lagrangian cross-terms, which contain the gradient four-vector of the pseudoscalar (axion) field in convolution with the Maxwell tensor. The gradient model of the axion-photon coupling is applied to cosmology: we analyze the Bianchi-I type Universe with an initial magnetic field, electric field induced by the axion-photon interaction, cosmological constant and dark matter, which is described in terms of the pseudoscalar (axion) field. Analytical, qualitative and numerical results are presented in detail for two distinguished epochs: first, for the early Universe with magnetic field domination; second, for the stage of late-time accelerated expansion.
26 pages, 5 figures, accepted for publication in The European Physical Journal C
References in corpus (19)
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Bose-Einstein Condensation of Dark Matter Axions
- New PVLAS results and limits on magnetically induced optical rotation and ellipticity in vacuum
- Inflation and late-time cosmic acceleration in non-minimal Maxwell- gravity and the generation of large-scale magnetic fields
- Axion cold dark matter in non-standard cosmologies
- Q & A Experiment to Search for Vacuum Dichroism, Pseudoscalar-Photon Interaction and Millicharged Fermions
- The BMV experiment : a novel apparatus to study the propagation of light in a transverse magnetic field
- From Equivalence Principles to Cosmology: Cosmic Polarization Rotation, CMB Observation, Neutrino Number Asymmetry, Lorentz Invariance and CPT
- Non-minimal coupling of photons and axions
- Non-minimal Einstein-Yang-Mills-Higgs theory: Associated, color and color-acoustic metrics for the Wu-Yang monopole model
- Effective metrics in the non-minimal Einstein-Yang-Mills-Higgs theory
- Cosmic Polarization Rotation, Cosmological Models, and the Detectability of Primordial Gravitational Waves
- Equivalence principle and electromagnetic field: no birefringence, no dilaton, and no axion
- Non-minimal pp-wave Einstein-Yang-Mills-Higgs model: color cross-effects induced by curvature
- Class of Einstein-Maxwell-Dilaton-Axion Space-Times
- Magnetic relaxation in the Bianchi-I universe
- Asymptotic singular behaviour of inhomogeneous cosmologies in Einstein-Maxwell-dilaton-axion theory
- Pseudoscalar-photon Interactions, Axions, Non-Minimal Extensions, and Their Empirical Constraints from Observations
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- Supermassive Neutron Stars in Axion Gravity
- Rotating Neutron Stars in F(R) Gravity with Axions
- Gravity with an Axion-like Particle: Dynamics, Gravity Waves, Late and Early-time Phenomenology
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- Axion electrodynamics and dark matter fingerprints in the terrestrial magnetic and electric fields
- The Einstein-Maxwell-aether-axion theory: Dynamo-optical anomaly in the electromagnetic response
- Electrodynamics of a Cosmic Dark Fluid
- Axion-induced oscillations of cooperative electric field in a cosmic magneto-active plasma
- Electromagnetic waves in an axion-active relativistic plasma non-minimally coupled to gravity
- Einstein-Maxwell-axion theory: Dyon solution with regular electric field
- Neutron Stars in f(R)-Gravity and Its Extension with a Scalar Axion Field
- Electrodynamic phenomena induced by a dark fluid: Analogs of pyromagnetic, piezoelectric, and striction effects
- Extended axion electrodynamics: Anomalous dynamo-optical response induced by gravitational pp-waves
- Magneto-electro-statics of axionically active systems: Induced field restructuring in magnetic stars