Particle Acceleration and Fractional Transport in Turbulent Reconnection
Heinz Isliker, Theophilos Pisokas, Loukas Vlahos, Anastasios, Anastasiadis

TL;DR
This paper investigates particle acceleration in turbulent reconnection environments with multiple current sheets, demonstrating that fractional transport equations better model energy distributions than classical Fokker-Planck equations due to Levy flight behavior.
Contribution
It introduces a fractional transport equation approach to accurately model particle acceleration in turbulent reconnection, accounting for Levy flights in energy space.
Findings
Power-law energy distributions with index 1-2 are achieved.
Classical Fokker-Planck equations fail to reproduce simulation results.
Fractional transport equations successfully model the energy distributions.
Abstract
We consider a large scale environment of turbulent reconnection that is fragmented into a number of randomly distributed Unstable Current Sheets (UCS), and we statistically analyze the acceleration of particles within this environment. We address two important cases of acceleration mechanisms when the particles interact with the UCS: (a) electric field acceleration, and (b) acceleration through reflection at contracting islands. Electrons and ions are accelerated very efficiently, attaining an energy distribution of power-law shape with an index , depending on the acceleration mechanism. The transport coefficients in energy space are estimated from the test-particle simulation data, and we show that the classical Fokker-Planck (FP) equation fails to reproduce the simulation results when the transport coefficients are inserted into it and it is solved numerically. The cause for this…
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