Relaxation of Compressible Euler Flow in a Toroidal Domain
Naoki Sato, Robert L. Dewar

TL;DR
This paper demonstrates that steady Euler flows in a toroidal domain satisfy a nonlinear Beltrami equation, representing a relaxed state that extremizes kinetic energy under specific boundary and conservation constraints.
Contribution
It introduces a nonlinear Beltrami equation for steady Euler flows in a toroidal domain and develops an action principle and Hamiltonian formulation for quasi-relaxed fluid dynamics.
Findings
Steady Euler flow fields obey a nonlinear Beltrami equation.
A relaxed velocity field extremizes kinetic energy under boundary and conservation constraints.
An action principle and Hamiltonian form for quasi-relaxed dynamics are formulated.
Abstract
It is shown that the universal steady Euler flow field, independent of boundary shape or symmetry, in a toroidal domain with fixed boundary obeys a nonlinear Beltrami equation, with the nonlinearity arising from a Boltzmann-like, velocity-dependent factor. Moreover, this is a relaxed velocity field, in the sense that it extremizes the total kinetic energy in the domain under free variations of the velocity field, constrained only by tangential velocity and vorticity boundary conditions and conservation of total fluid helicity and entropy. This is analogous to Woltjer-Taylor relaxation of plasma magnetic field to a stationary state. However, unlike the magnetic field case, attempting to derive slow, quasi-relaxed dynamics from Hamilton's action principle, with constant total fluid helicity as a constraint, fails to agree, in the static limit, with the nonlinear Beltrami solution of the…
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Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Solar and Space Plasma Dynamics · Navier-Stokes equation solutions
