Magnetic reconnection as an Adler-Ohmic bifurcation: The topological origin of Bohm resistivity
Magnus F Ivarsen

TL;DR
This paper presents a topological phase transition model for magnetic reconnection, deriving Bohm resistivity from first principles and supported by data analysis, revealing a universal topological origin of anomalous resistivity in space plasmas.
Contribution
It introduces a novel topological phase transition framework for understanding Bohm resistivity, linking it to an Adler-Ohmic bifurcation and collective phase slippage.
Findings
Resistivity onset is a topological phase transition.
Data shows explosive phase space confinement during reconnection.
Bohm resistivity emerges as a universal topological property.
Abstract
The physical origin of 'anomalous' resistivity in magnetic reconnection remains one of the longest-standing problems in space plasma physics. While the empirical Bohm diffusion scaling () is widely invoked to explain fast reconnection rates, it lacks a rigorous derivation from first principles. Here, we derive this scaling by modeling the ensemble of electron gyro-axes in a magnetized plasma as an overdamped spintronic condensate governed by the Landau-Lifshitz-Gilbert equation. We demonstrate that the breakdown of the "frozen-in" condition is rigorously identified as an Adler-Ohmic bifurcation: a topological phase transition where electron gyro-axes lose synchronization with the mean magnetic field. Unlike stochastic turbulence models, this framework predicts a coherent, explosive onset of resistivity that naturally saturates at the Bohm limit. We support this thesis…
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Taxonomy
TopicsIonosphere and magnetosphere dynamics · Solar and Space Plasma Dynamics · Dust and Plasma Wave Phenomena
