Including time-dependent energy losses of primordial magnetic fields relaxes current bounds from reionization and UV luminosity data while 21cm cosmology could improve them.
Probing the primordial Universe with 21cm line from cosmic dawn/epoch of reionization.Publ
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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.