Preprint Article Version 2 Preserved in Portico This version is not peer-reviewed

Exact Solution of Decaying Turbulence

Version 1 : Received: 29 August 2023 / Approved: 29 August 2023 / Online: 30 August 2023 (09:01:51 CEST)
Version 2 : Received: 31 August 2023 / Approved: 4 September 2023 / Online: 4 September 2023 (12:00:54 CEST)
Version 3 : Received: 6 September 2023 / Approved: 7 September 2023 / Online: 7 September 2023 (09:28:55 CEST)
Version 4 : Received: 15 September 2023 / Approved: 18 September 2023 / Online: 18 September 2023 (13:56:35 CEST)

A peer-reviewed article of this Preprint also exists.

Migdal, A. To the Theory of Decaying Turbulence. Fractal Fract. 2023, 7, 754. Migdal, A. To the Theory of Decaying Turbulence. Fractal Fract. 2023, 7, 754.

Abstract

We have found an infinite dimensional manifold of exact solutions of the Navier-Stokes loop equation for the Wilson loop in decaying Turbulence in arbitrary dimension $d >2$. This solution family is equivalent to a fractal curve in complex space $\mathbb C^d$ with random steps parametrized by $N$ Ising variables $\sigma_i=\pm 1$, in addition to a rational number $\frac{p}{q}$ and an integer winding number $r$, related by $\sum \sigma_i = q r$. This equivalence provides a \textbf{dual} theory describing a strong turbulent phase of the Navier-Stokes flow in $\mathbb R_d$ space as a random geometry in a different space, like ADS/CFT correspondence in gauge theory. This is a \textbf{quantum} statistical system with integer-valued parameters, satisfying some number theory constraints. Its long-range interaction leads to critical phenomena when its size $N \rightarrow \infty$ or its chemical potential $\mu \rightarrow 0$. The system with fixed $N$ has different asymptotics at odd and even $N\rightarrow \infty$, but the limit $\mu \rightarrow 0$ is well defined. The energy dissipation rate is analytically calculated as a function of $\mu$ using methods of number theory. It grows as $\nu/\mu^2$ in the continuum limit $\mu \rightarrow 0$, leading to anomalous dissipation at $\mu \propto \sqrt{\nu} \rightarrow 0$. The same method applies to other observables. The small perturbation of the fixed manifold satisfies the linear equation we solved in a general form. This perturbation decays as $t^{-\lambda}$, where the anomalous dimensions $\lambda$ satisfy the spectral equation \eqref{spectralEq}. The spectrum becomes a continuum in the statistical limit $N \ra \infty$, leading to multifractal phenomena.

Keywords

Turbulence, Fractal, Anomalous dissipation, Fixed point, Velocity circulation, Loop Equations, Euler Phi, Prime numbers

Subject

Physical Sciences, Theoretical Physics

Comments (1)

Comment 1
Received: 4 September 2023
Commenter: Alexander Migdal
Commenter's Conflict of Interests: Author
Comment: Added new important results: the equation for the spectrum of time decay indexes, $t^{-\lambda}$. This spectrum becomes continuous in the local limit of our system, suggesting multifractal phenomena.
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