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A transport-like approach to turbulence-mediated magnetic reconnection

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arxiv 2312.06945 v1 pith:75FKNQU3 submitted 2023-12-12 physics.plasm-ph astro-ph.HE

Nuno F. Loureiro This is my paper · ORCID
classification physics.plasm-phastro-ph.HE
keywords reconnectionapproachmagnetictimescaletransport-likearguearisecases
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A transport-like framework for the study of magnetic reconnection mediated by self-driven turbulence is proposed, based on timescale separation between the reconnection time and the characteristic timescale of the turbulent fluctuations which arise in the reconnection layer. We argue that the mean fields remain on MHD scales even in collisionless cases. These observations provide theoretical justification for an efficient computational approach to this problem, which we discuss.

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Cited by 1 Pith paper

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  1. Effective resistivity in relativistic reconnection: a prescription based on fully kinetic simulations

    astro-ph.HE 2025-01 conditional novelty 5.0 of 10

    An empirical effective resistivity eta = alpha B0 |J|^p / (|J|^(p+1) + (e n c)^(p+1)) is fit to PIC simulations of relativistic pair-plasma reconnection and reproduces nonideal electric fields, but the proposed guide-...

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