Including time-dependent energy losses of primordial magnetic fields relaxes current bounds from reionization and UV luminosity data while 21cm cosmology could improve them.
Cosmology with inhomogeneous magnetic fields, phys, 2007
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Reionization, UV Luminosity and 21$\,$cm Sensitivity to Primordial Magnetic Fields: Impact of Energy Losses
Including time-dependent energy losses of primordial magnetic fields relaxes current bounds from reionization and UV luminosity data while 21cm cosmology could improve them.