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Picogauss magnetic fields in voids from ultra-high energy cosmic rays

We argue that ultra-high energy cosmic rays emitted by galaxy clusters result in electric currents in filaments of the large-scale structure that are sufficient to generate magnetic fields in voids of the magnitude of ~1e-12 G and the coherence length of up to tens of Mpc. These fields satisfy both the lower and upper observational bounds on magnetic fields in voids without a need of any primordial component.

preprint2012arXivOpen access
M. S. PshirkovP. G. Tinyakov
astro-ph.COastro-ph.HE
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M. S. PshirkovP. G. Tinyakov

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