Duality of Navier-Stokes to a one-dimensional system
Alexander Migdal
TL;DR
The paper reframes Navier–Stokes turbulence as a linear quantum-like problem in loop space, introducing a momentum-loop equation whose exact, universal decaying-turbulence solution is the Euler ensemble. This ensemble admits a dual description as a string theory on a discrete target space of regular star polygons, with a random-walk dynamics over polygon vertices and an associated dual Wilson-loop amplitude; a No Explosion Theorem removes finite-time singularities under stochastic initial data. The work yields precise predictions for the decay of turbulence, vorticity statistics, and energy spectra, matching numerical and experimental data, and provides a rigorous link between fluid dynamics, number theory, and discrete string theories. It also clarifies how large Reynolds limits can differ from vanishing viscosity limits and discusses rich avenues for physical generalizations and mathematical directions. Overall, it offers a mathematically tractable, testable framework for turbulent NS dynamics with deep connections to geometry and quantum-like loop space methods.
Abstract
The Navier--Stokes (NS) equations describe fluid dynamics through a high-dimensional, nonlinear system of partial differential equations (PDEs). Despite their fundamental importance, their behavior in turbulent regimes remains incompletely understood, and their global regularity is still an open problem. Here, we reformulate the NS equations as a nonlinear equation for the momentum loop $\vec{P}(θ, t)$, effectively reducing the original three-dimensional PDE to a one-dimensional problem. We present an explicit analytical solution -- the Euler ensemble -- which describes the universal asymptotic state of decaying turbulence and is supported by numerical simulations and experimental validation. This Euler ensemble is equivalent to a string theory with discrete target space given by a set of regular star polygons, with additional Ising (Fermi) degrees of freedom at the vertices. This string theory can also be interpreted as a random walk on regular star polygons. The Wilson loop for turbulence, \[ \left\langle \exp\left( \imath \oint dθ\, \vec{C}'(θ) \cdot \vec{v}(\vec{C}(θ, t)) \right) \right\rangle, \] reduces to a dual amplitude of this string theory with distributed external momentum proportional to $\vec{C}'(θ)/\sqrt{t}$.
