Axion Electrodynamics in Strong Magnetic Backgrounds
arXiv:2203.14851 · doi:10.1088/1742-6596/2249/1/012021
Abstract
The overcritical regime of axion-electrodynamics (AED) is investigated. For magnetic fields larger than the characteristic scale linked to AED, quantum vacuum fluctuations due to axion-like fields can dominate over those associated with the electron-positron fields. This hypothetical regime of the dominance of AED over QED is predicted to induce strong birefringence and screening effects. We show that, if the magnetic field lines are curved, extraordinary photons could be canalized along the field direction. It is also shown that the running QED coupling depends on the magnetic field strength, and for certain energy regimes, it could be screened almost to zero, making the QED building blocks very weakly interacting between each other. The impact of this phenomenon on the radiation mechanism of pulsars is discussed.
arXiv comment9 pages, 5 figures
References in corpus (17)
- The ATNF Pulsar Catalogue
- The Low-Energy Frontier of Particle Physics
- A facility to Search for Hidden Particles at the CERN SPS: the SHiP physics case
- New experimental approaches in the search for axion-like particles
- Astrophysical Axion Bounds
- Particle Physics from Stars
- Birefringence and Dichroism of the QED Vacuum
- Photon Splitting in a Strong Magnetic Field: Recalculation and Comparison With Previous Calculations
- New Evidence for Proton Cyclotron Resonance in a Magnetar Strength Field from SGR 1806-20
- Axionic instabilities and new black hole solutions
- Renormalization flow of QED
- Expected characteristics of the subclass of Supernova Gamma-ray Bursts (S-GRBs)
- Electric field of a pointlike charge in a strong magnetic field and ground state of a hydrogenlike atom
- Modified Coulomb Law in a Strongly Magnetized Vacuum
- Coulomb field in a constant electromagnetic background
- Magnetic Field Effect in the Fine-Structure Constant and Electron Dynamical Mass
- Axion-modified photon propagator, Coulomb potential and Lamb-shift