Curvature acceleration in strong Alfvénic turbulence saturates due to diminishing energy exchange efficiency, producing particle distributions f(p) ∝ p^{-3} (non-relativistic) and f(γ) ∝ γ^{-3} (ultrarelativistic).
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The paper reviews electron transport in tangled magnetic fields, including creation via turbulence, modulation by instabilities, trapping, cross-field diffusion, and energization.
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Distributions of particles accelerated by strong Alfv\'enic turbulence
Curvature acceleration in strong Alfvénic turbulence saturates due to diminishing energy exchange efficiency, producing particle distributions f(p) ∝ p^{-3} (non-relativistic) and f(γ) ∝ γ^{-3} (ultrarelativistic).
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Transport of electrons in tangled magnetic fields
The paper reviews electron transport in tangled magnetic fields, including creation via turbulence, modulation by instabilities, trapping, cross-field diffusion, and energization.