Simulations of turbulent reconnection in relativistic jets show energy-independent acceleration time in the Fermi regime matching theory up to a Larmor radius threshold set by current sheet thickness, then energy-dependent drift regime.
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Particle Acceleration Time due to Turbulent-Induced Magnetic Reconnection
Simulations of turbulent reconnection in relativistic jets show energy-independent acceleration time in the Fermi regime matching theory up to a Larmor radius threshold set by current sheet thickness, then energy-dependent drift regime.