The invariant Twist of Magnetic Fields in the Relativistic Jets of Active Galactic Nuclei
Ioannis Contopoulos, Dimitris M. Christodoulou, Demosthenes Kazanas,, Denise C. Gabuzda

TL;DR
This paper proposes a new mechanism for the origin of cosmic magnetic fields in AGN jets, linking the magnetic field polarity to the accretion disk's rotation, supported by observational asymmetry data.
Contribution
It introduces a novel model where magnetic fields are generated near AGN accretion disks through azimuthal currents, explaining observed magnetic field asymmetries.
Findings
Observed asymmetry in AGN jet magnetic fields supports the model.
Probability of asymmetry occurring by chance is less than 1%.
Supports the hypothesis that AGN generate and seed cosmic magnetic fields.
Abstract
The origin of cosmic magnetic (B) fields remains an open question. It is generally believed that very weak primordial B fields are amplified by dynamo processes, but it appears unlikely that the amplification proceeds fast enough to account for the fields presently observed in galaxies and galaxy clusters. In an alternative scenario, cosmic B fields are generated near the inner edges of accretion disks in Active Galactic Nuclei (AGNs) by azimuthal electric currents due to the difference between the plasma electron and ion velocities that arises when the electrons are retarded by interactions with photons. While dynamo processes show no preference for the polarity of the (presumably random) seed field that they amplify, this alternative mechanism uniquely relates the polarity of the poloidal B field to the angular velocity of the accretion disk, resulting in a unique direction for the…
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