A limsup fast dynamo on $\mathbb{T}^3$

Fuente: arXiv
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Main Authors: Sorella, Massimo, Villringer, David
Format: Preprint
Published: 2025
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author Sorella, Massimo
Villringer, David
author_facet Sorella, Massimo
Villringer, David
contents We construct a time-dependent, incompressible, and uniformly-in-time Lipschitz continuous velocity field on $\mathbb{T}^3$ that produces exponential growth of the magnetic energy along a subsequence of times, for every positive value of the magnetic diffusivity. Because this growth is not uniform in time but occurs only along a diverging sequence of times, we refer to the resulting mechanism as a limsup fast dynamo. Our construction is based on suitably rescaled Arnold-Beltrami-Childress (ABC) flows, each supported on long time intervals. The analysis employs perturbation theory to establish continuity of the exponential growth rate with respect to both the initial data and the diffusivity parameter. This proves the weak form of the fast dynamo conjecture formulated by Childress and Gilbert on $\mathbb{T}^3$, but the considerably more challenging version proposed by Arnold on $\mathbb{T}^3$ remains an open problem.
format Preprint
id arxiv_https___arxiv_org_abs_2511_23024
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle A limsup fast dynamo on $\mathbb{T}^3$
Sorella, Massimo
Villringer, David
Analysis of PDEs
35Q35, 34L05, 47A55, 76E25, 47B12
We construct a time-dependent, incompressible, and uniformly-in-time Lipschitz continuous velocity field on $\mathbb{T}^3$ that produces exponential growth of the magnetic energy along a subsequence of times, for every positive value of the magnetic diffusivity. Because this growth is not uniform in time but occurs only along a diverging sequence of times, we refer to the resulting mechanism as a limsup fast dynamo. Our construction is based on suitably rescaled Arnold-Beltrami-Childress (ABC) flows, each supported on long time intervals. The analysis employs perturbation theory to establish continuity of the exponential growth rate with respect to both the initial data and the diffusivity parameter. This proves the weak form of the fast dynamo conjecture formulated by Childress and Gilbert on $\mathbb{T}^3$, but the considerably more challenging version proposed by Arnold on $\mathbb{T}^3$ remains an open problem.
title A limsup fast dynamo on $\mathbb{T}^3$
topic Analysis of PDEs
35Q35, 34L05, 47A55, 76E25, 47B12
url https://arxiv.org/abs/2511.23024