Turbulence: Why Measuring Energy Isn't So Simple ✎ express

Original: "Relation between the moments of longitudinal velocity derivatives and of dissipation in turbulence"
· Ping-Fan Yang, Haitao Xu, Alain Pumir
arXiv:2601.16436 · 2026-01-23 · arXiv non-exclusive · independent analysis · 1 min
The usual way to estimate how quickly a fluid loses energy in vortices isn't always accurate.

When water churns behind a boat, the energy of motion is converted into heat through a cascade of vortices. Measuring how quickly this happens directly is difficult: you'd need to track all the vortices at once. So scientists use a simplification: they look at only one velocity component at a single point. A classic formula relates the square of this component to the overall energy dissipation rate.

It turns out this simplification doesn't always work. For average values, it's fine, but if you're interested in strong deviations from the mean, and those are what matter for understanding intermittency in turbulence, the simple formula fails. An additional term enters the calculation, one that depends on how exactly the fluid deforms. This term is described by an invariant of the strain-rate tensor — a characteristic that doesn't depend on the choice of coordinate system.

Estimating a car's speed from engine noise works for normal driving, but during hard acceleration, the noise depends not just on RPMs but also on load.

Fortunately, the error isn't catastrophic. If you assume deformations follow a Gaussian distribution (that is, random, like molecules in a gas) then the exact distribution differs from the approximate one by only a few percent. This means the simple formula can still be used in most practical applications, as long as you keep its limitations in mind.

Turbulence is one of the unsolved problems in classical physics: the equations have been known since the 19th century, but an exact solution for strong turbulence remains elusive.

\epsilon_s = 15 \nu (\partial_1 u_1)^2
Estimate of energy dissipation rate from a single velocity component: ν is viscosity, ∂₁u₁ is the derivative of the longitudinal velocity.
Scientists
Ludwig BoltzmannRudolf ClausiusJacob BekensteinStephen HawkingJames Clerk MaxwellEdward Witten
Concepts
dispersion relation reynolds number second derivative velocity dispersion fluctuation-dissipation theorem velocity distribution time derivative gravitational wave strain mass flow rate quadrupole moment proportionality spacetime interval Navier-Stokes equations power law distribution turbulence variance flux constant moment of inertia damping rate derivative