Reionization, UV Luminosity and 21, cm Sensitivity to Primordial Magnetic Fields: Impact of Energy Losses
This work re-examines constraints on primordial magnetic fields (PMFs) by consistently modeling their energy losses through ambipolar diffusion and decaying turbulence during cosmic evolution from recombination to reionization. The study uses detailed cosmological equations to link PMF parameters to observable effects on the Intergalactic Medium and structure formation.