# Particle acceleration and fast magnetic reconnection

**Authors:** Allen H. Boozer

arXiv: 1902.10860 · 2020-01-29

## TL;DR

This paper explores the mathematical basis of fast magnetic reconnection in three-dimensional magnetic fields, emphasizing the exponential sensitivity to non-ideal effects and the role of Alfvénic physics in energy transfer.

## Contribution

It provides a theoretical framework showing how exponential sensitivity leads to fast reconnection in 3D magnetic fields, extending classical 2D theories.

## Key findings

- Fast magnetic reconnection occurs on a timescale logarithmic in non-ideality.
- Energy transfer during reconnection is governed by Alfvénic physics, not resistive effects.
- Weak non-ideality conserves magnetic helicity but enables subtle energy transfer mechanisms.

## Abstract

Mathematics demonstrates that an ideally evolving magnetic field has an exponentially increasing sensitivity to non-ideal effects for all but truly exceptional evolutions. On a time scale that depends only logarithmically on the magnitude of non-ideality, an evolving magnetic field will generally reach a state of fast magnetic reconnection. The effects of fast magnetic reconnection proceed at a rate determined by Alfv\'enic, not resistive, physics. The best known of these effects are associated with the transfer of magnetic field energy to the plasma and the conservation of magnetic helicity, which limits the energy transfer. As will be shown, weak non-ideality implies helicity conservation in regions bounded by magnetic surfaces or rigid perfect conductors. But, weak non-ideality makes the rapid transfer of energy subtle. This transfer can be understood by the drive for Alfv\'en waves and two other effects, which are present even in an ideal evolution, an effective parallel electric field $\mathcal{E}_{||}$, which can accelerate particles despite the particle acceleration due to the true parallel electric field $E_{||}$ being negligible, and a coefficient $\nu_K$, which gives a rate for exponentiation of the kinetic energy of particle motion along the magnetic field. Classical theories of reconnection are two-dimensional and exclude the exponentially increasing sensitivity that is robustly present for magnetic fields in three-dimensional space.

## Full text

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## References

31 references — full list in the complete paper: https://tomesphere.com/paper/1902.10860/full.md

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Source: https://tomesphere.com/paper/1902.10860