UHECR Acceleration in Dark Matter Filaments of Cosmological Structure Formation
Mikhail Malkov, Roald Sagdeev, and Patrick Diamond

TL;DR
This paper proposes a novel mechanism for accelerating protons to ultra-high energies (~10^21 eV) in dark matter filaments during cosmic structure formation, overcoming previous energy loss limits.
Contribution
It introduces a new acceleration process involving magnetic field compression and betatron acceleration in dark matter filaments, enabling protons to reach unprecedented energies.
Findings
Protons can be accelerated to 10^21 eV in dark matter filaments.
The mechanism surpasses photo-pion and synchrotron loss limits.
Pre-acceleration likely occurs in structure formation shocks.
Abstract
A mechanism for proton acceleration to ~10^21eV is suggested. It may operate in accretion flows onto thin dark matter filaments of cosmic structure formation. The flow compresses the ambient magnetic field to strongly increase and align it with the filament. Particles begin the acceleration by the ExB drift with the accretion flow. The energy gain in the drift regime is limited by the conservation of the adiabatic invariant p_perp^2/B. Upon approaching the filament, the drift turns into the gyro-motion around the filament so that the particle moves parallel to the azimuthal electric field. In this 'betatron' regime the acceleration speeds up to rapidly reach the electrodynamic limit for an accelerator with magnetic field and the orbit radius (Larmor radius). The periodic orbit becomes unstable and the particle slings out of the filament to the region of a weak…
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