Axion driven cosmic magneto-genesis during the QCD crossover
Francesco Miniati, Gianluca Gregori, Brian Reville, Subir Sarkar

TL;DR
This paper proposes a novel mechanism where axions induce magnetic fields during the QCD crossover, potentially explaining cosmic magnetism and offering testable predictions through gamma-ray and gravitational wave observations.
Contribution
It introduces a new axion-driven magnetogenesis mechanism during the QCD crossover, linking axion physics with early universe magnetic field generation.
Findings
Magnetic field strength estimated at ~10^{-13} G today
Magnetic fields generated on subhorizon scales (~20 pc)
Potential observational tests via gamma-ray and gravitational wave data
Abstract
We propose a mechanism for the generation of a magnetic field in the early universe during the QCD crossover assuming that dark matter is made of axions. Thermoelectric fields arise at pressure gradients in the primordial plasma due to the difference in charge, energy density and equation of state between the quark and lepton components. The axion field is coupled to the EM field, so when its spatial gradient is misaligned with the thermoelectric field, an electric current is driven. Due to the finite resistivity of the plasma an electric field appears that is generally rotational. For a QCD axion mass consistent with observational constraints and a conventional efficiency for turbulent dynamo amplification --- driven by the same pressure gradients responsible for the thermoelectric fields --- a magnetic field is generated on subhorizon scales. After significant Alfv\'enic unwinding it…
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