Shell-to-shell transfer analysis in decaying MHD turbulence demonstrates direct non-local inverse energy transfer from the integral scale, resulting in multiplicative growth of large-scale magnetic energy, confined within helical sectors when net helicity is zero.
Revisiting constraints on primordial magnetic fields from spectral distortions of cosmic microwave background
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Maximally helical primordial U(1)_Y magnetic fields can generate both intergalactic magnetic fields and baryon asymmetry; non-helical fields may work if Higgs dynamics compensate helicity loss to ≲10^{-9-10} precision during electroweak crossover.
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Revisiting constraints on magnetogenesis from baryon asymmetry
Maximally helical primordial U(1)_Y magnetic fields can generate both intergalactic magnetic fields and baryon asymmetry; non-helical fields may work if Higgs dynamics compensate helicity loss to ≲10^{-9-10} precision during electroweak crossover.