Diffusive Shock Acceleration and Turbulent Reconnection
Christian Garrel, Loukas Vlahos, Heinz Isliker, Theophilos Pisokas

TL;DR
This paper explores how turbulent reconnection (TR) enhances particle acceleration near shocks, showing that TR can significantly outperform traditional diffusive shock acceleration (DSA) in efficiency and maximum energy achieved.
Contribution
It demonstrates that the combination of DSA and TR leads to faster acceleration and higher energy particles, highlighting the synergy between these mechanisms in shock environments.
Findings
TR accelerates particles as efficiently as DSA in large systems
The combined DSA and TR mechanism shortens acceleration time by an order of magnitude
Maximum particle energy is increased by two orders of magnitude with DSA/TR synergy
Abstract
Diffusive Shock Acceleration (DSA) cannot efficiently accelerate particles without the presence of self-consistently generated or pre-existing strong turbulence () in the vicinity of the shock. The problem we address in this article is: if large amplitude magnetic disturbances are present upstream and downstream of a shock then Turbulent Reconnection (TR) will set in and will participate not only in the elastic scattering of particles but also in their heating and acceleration. We demonstrate that large amplitude magnetic disturbances and Unstable Current Sheets (UCS), spontaneously formed in the strong turbulence in the vicinity of a shock, can accelerate particles as efficiently as DSA in {\bf large scale systems and on long time scales}. We start our analysis with "elastic" scatterers upstream and downstream and estimate the energy distribution of particles…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
