Halo magnetic fields at z=0 converge across primordial and astrophysical seeds via dynamo action, but IGM magnetization and coherence lengths retain seed memory and SN-only injection underproduces γ-ray lower limits.
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Magnetogenesis by galactic processes: impact on circumgalactic and intergalactic fields
Halo magnetic fields at z=0 converge across primordial and astrophysical seeds via dynamo action, but IGM magnetization and coherence lengths retain seed memory and SN-only injection underproduces γ-ray lower limits.