A fractal version of the Onsager's conjecture: the $\beta-$model
Luigi De Rosa, Silja Haffter

TL;DR
This paper establishes a mathematical link between fractal models of turbulence and energy conservation, showing that the dimension of singularities determines whether energy is conserved in solutions of the Euler equations, aligning with the Onsager conjecture.
Contribution
It provides a rigorous mathematical statement connecting the fractal dimension of singularities with energy conservation in Euler solutions, extending Onsager's conjecture to fractal turbulence models.
Findings
Energy conservation holds if the Minkowski dimension of singularities is less than 2+3θ.
Non-conservative solutions have singularities concentrated on sets with dimension at least 2+3θ.
Results align with the fractal $eta$-model and previous mathematical findings.
Abstract
Intermittency phenomena are known to be among the main reasons why Kolmogorov's theory of fully developed Turbulence is not in accordance with several experimental results. This is why some \emph{fractal} statistical models have been proposed in order to realign the theoretical physical predictions with the empirical experiments. They indicate that energy dissipation, and thus singularities, are not space filling for high Reynolds numbers. This note aims to give a precise mathematical statement on the energy conservation of such fractal models of Turbulence. We prove that for H\"older continuous weak solutions of the incompressible Euler equations energy conservation holds if the upper Minkowski dimension of the spatial singular set (possibly also time-dependent) is small, or more precisely if In particular, the…
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Taxonomy
TopicsStochastic processes and financial applications · Fluid Dynamics and Turbulent Flows · Complex Systems and Time Series Analysis
