Abstract
Rigorous estimates for the total – (kinetic) energy plus pressure – flux in \({\mathbb{R}^3}\) are obtained from the three dimensional Navier-Stokes equations. The bounds are used to establish a condition – involving Taylor length scale and the size of the domain – sufficient for existence of the inertial range and the energy cascade in decaying turbulence (zero driving force, non-increasing global energy). Several manifestations of the locality of the flux under this condition are obtained. All the scales involved are actual physical scales in \({\mathbb{R}^3}\) and no regularity or homogeneity/scaling assumptions are made.
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Dascaliuc, R., Grujić, Z. Energy Cascades and Flux Locality in Physical Scales of the 3D Navier-Stokes Equations. Commun. Math. Phys. 305, 199–220 (2011). https://doi.org/10.1007/s00220-011-1219-8
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DOI: https://doi.org/10.1007/s00220-011-1219-8