Radiation backreaction in axion electrodynamics
Andras Patkos

TL;DR
This paper analyzes energy conservation in axion-electrodynamics, identifies energy transfer mechanisms, and quantifies axion damping in magnetic fields, with implications for axion cosmology.
Contribution
It provides a Hamiltonian formulation of energy transfer in axion-electrodynamics and quantifies axion damping times in magnetic backgrounds.
Findings
Energy transfer term identified in the Hamiltonian framework.
Axion-to-light Primakoff process analyzed in static magnetic fields.
Axion damping time comparable to the Universe's age in certain mass ranges.
Abstract
Energy-momentum conservation of classical axion-electrodynamics is carefully analyzed in the Hamiltonian formulation of the theory. The term responsible for the energy transfer between the electromagnetic and the axion sectors is identified. As a special application the axion-to-light Primakoff-process in the background of a static magnetic field is worked out and the radiative self-damping of the axion oscillations is characterized quantitatively. The damping time turns out comparable to the age of the Universe in the preferred axion mass range.
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