Including time-dependent energy losses of primordial magnetic fields relaxes current bounds from reionization and UV luminosity data while 21cm cosmology could improve them.
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A Z2-symmetric SM extension with vector-like fermions and an inert scalar doublet generates neutrino masses radiatively, accounts for (g-2)e,μ anomalies, and yields the observed DM relic abundance while satisfying LFV, direct detection, BBN, and CMB bounds.
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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.
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Neutrino masses, anomalous magnetic moments and dark matter with vector-like fermions and an inert scalar doublet
A Z2-symmetric SM extension with vector-like fermions and an inert scalar doublet generates neutrino masses radiatively, accounts for (g-2)e,μ anomalies, and yields the observed DM relic abundance while satisfying LFV, direct detection, BBN, and CMB bounds.