Picogauss magnetic fields in voids from ultra-high energy cosmic rays
M. S. Pshirkov, P. G. Tinyakov

TL;DR
This paper proposes that ultra-high energy cosmic rays from galaxy clusters can generate magnetic fields in cosmic voids, reaching observable magnitudes without primordial origins, aligning with current observational bounds.
Contribution
It introduces a novel mechanism linking cosmic rays to magnetic field generation in voids, explaining observed field strengths without primordial assumptions.
Findings
Magnetic fields in voids can reach ~10^-12 G
Coherence lengths of magnetic fields can be tens of Mpc
The mechanism aligns with observational bounds
Abstract
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.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Solar and Space Plasma Dynamics
