Dark matter and generation of galactic magnetic fields
Zurab Berezhiani, A.D. Dolgov, I.I. Tkachev

TL;DR
This paper proposes a novel mechanism where feeble long-range interactions between dark matter and electrons generate galactic magnetic fields during galaxy formation, potentially explaining observed magnetic phenomena.
Contribution
It introduces a new scenario linking dark matter properties to the generation of galactic magnetic fields through electron interactions at cosmological epochs.
Findings
Dark matter-electron interactions can produce sufficient electric currents in protogalaxies.
Generated magnetic fields can be amplified by dynamo processes to match observations.
Angular momentum transfer may alter dark matter profiles, affecting galaxy core structures.
Abstract
A new scenario for creation of galactic magnetic fields is proposed which is operative at the cosmological epoch of the galaxy formation, and which relies on unconventional properties of dark matter. Namely, it requires existence of feeble but long range interaction between the dark matter particles and electrons. In particular, millicharged dark matter particles or mirror particles with the photon kinetic mixing to the usual photon can be considered. We show that in rotating protogalaxies circular electric currents can be generated by the interactions of free electrons with dark matter particles in the halo, while the impact of such interactions on galactic protons is considerably weaker. The induced currents may be strong enough to create the observed magnetic fields on the galaxy scales with the help of moderate dynamo amplification. In addition, the angular momentum transfer from…
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