Primordial black holes and magnetic fields in conformal neutrino mass models
arXiv:2505.08011 · doi:10.1088/1475-7516/2025/10/064
Abstract
Sufficiently strong and long-lasting first-order phase transitions can produce primordial black holes (PBHs) that contribute substantially to the dark matter abundance of the Universe, and can produce large-scale primordial magnetic fields. We study these mechanisms in a generic class of conformal models that also explain active neutrino oscillation data via the type-I seesaw mechanism. We find that phase transitions that occur at seesaw scales between GeV and GeV produce gravitational wave signals (from the dynamics of the phase transition and from the decay of cosmic string loops) at LISA/ET that can be correlated with microlensing signals of PBHs at the Roman Space Telescope, while scales near GeV can be correlated with Hawking evaporation signals at future gamma-ray telescopes. LISA can probe the entire range of PBH masses between and if PBHs fully account for the dark matter abundance. For Z' masses between 5 TeV and 100 TeV, and TeV right-handed neutrinos, helical magnetic fields can be produced with magnitudes - G and coherence lengths - Mpc, above current blazar lower bounds.
25 pages, 10 figures, 3 tables. Corrected bug in magnetic field code. Corresponding parameter space changed
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