On URANS Congruity with Time Averaging: Analytical laws suggest improved models
Abstract
The standard 1-equation model \ of turbulence was first derived by Prandtl and has evolved to be a common method for practical flow simulations. Five fundamental laws that any URANS model should satisfy are \[ array [c]ccc 1. & Time window: & array [c]c τ 0 implies v URANS→ u NSE \&\\ τ T array \\ 2. & l(x)=0\ at walls: & l(x)→ 0 as x→ walls,\\ 3. & Bounded energy: & t∫1 2|v(x,t)|2+k(x,t)dx<∞\\ 4. & array [c]c Statistical \\ equilibrium: array & T→∞1T∫0T model(t)dt=O( U3L) \\ 5. & array [c]c Backscatter\\ possible: array & (without negative viscosities) array \] This report proves that a kinematic specification of the model's turbulence lengthscale by \[ l(x,t)=2k1/2(x,t)τ , \] where τ\ is the time filter window, results in a 1-equation model satisfying Conditions 1,2,3,4 without model tweaks, adjustments or wall damping multipliers.
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