Intermittency and lower dimensional dissipation in incompressible fluids
Luigi De Rosa, Philip Isett

TL;DR
This paper demonstrates that in inviscid incompressible fluids, lower-dimensional energy dissipation leads to deviations from classical turbulence predictions, providing a rigorous foundation for intermittency and the fractal nature of turbulent dissipation structures.
Contribution
It establishes a rigorous link between dissipation dimensionality and structure function deviations, connecting geometrical dissipation assumptions with turbulence intermittency.
Findings
Lower-dimensional dissipation implies deviations from K41 predictions for p>3.
The upper bound on structure function exponents matches the β-model from 1970s.
A new local variant of Constantin-E-Titi argument is developed for the proof.
Abstract
In the context of incompressible fluids, the observation that turbulent singular structures fail to be space filling is known as ``intermittency'' and it has strong experimental foundations. Consequently, as first pointed out by Landau, real turbulent flows do not satisfy the central assumptions of homogeneity and self-similarity in the K41 theory, and the K41 prediction of structure function exponents might be inaccurate. In this work we prove that, in the inviscid case, energy dissipation that is lower-dimensional in an appropriate sense implies deviations from the K41 prediction in every th order structure function for . By exploiting a Lagrangian-type Minkowski dimension that is very reminiscent of the Taylor's frozen turbulence hypothesis, our strongest upper bound on coincides with the model proposed by Frisch, Sulem and Nelkin in…
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Taxonomy
TopicsCosmology and Gravitation Theories · Fluid Dynamics and Turbulent Flows · Navier-Stokes equation solutions
