English

Bounds on Kolmogorov spectra for the Navier - Stokes equations

Mathematical Physics 2009-06-10 v2 math.MP

Abstract

Let u(x,t)u(x,t) be a (possibly weak) solution of the Navier - Stokes equations on all of R3{\mathbb R}^3, or on the torus R3/Z3{\mathbb R}^3/ {\mathbb Z}^3. The {\it energy spectrum} of u(,t)u(\cdot,t) is the spherical integral E(κ,t)=k=κu^(k,t)2dS(k),0κ<, E(\kappa,t) = \int_{|k| = \kappa} |\hat{u}(k,t)|^2 dS(k), \qquad 0 \leq \kappa < \infty, or alternatively, a suitable approximate sum. An argument involking scale invariance and dimensional analysis given by Kolmogorov (1941) and Obukhov (1941) predicts that large Reynolds number solutions of the Navier - Stokes equations in three dimensions should obey E(κ,t)C0ε2/3κ5/3 E(\kappa, t) \sim C_0\varepsilon^{2/3}\kappa^{-5/3} over an inertial range κ1κκ2\kappa_1 \leq \kappa \leq \kappa_2, at least in an average sense. We give a global estimate on weak solutions in the norm Fxu(,t)\|{\mathcal F}\partial_x u(\cdot, t)\|_\infty which gives bounds on a solution's ability to satisfy the Kolmogorov law. A subsequent result is for rigorous upper and lower bounds on the inertial range, and an upper bound on the time of validity of the Kolmogorov spectral regime.

Cite

@article{arxiv.0807.4505,
  title  = {Bounds on Kolmogorov spectra for the Navier - Stokes equations},
  author = {Andrei Biryuk and Walter Craig},
  journal= {arXiv preprint arXiv:0807.4505},
  year   = {2009}
}

Comments

26 pages with one figure

R2 v1 2026-06-21T11:05:09.556Z