On the Prandtl-Kolmogorov 1-equation model of turbulence

TL;DR

This paper analyzes the Prandtl-Kolmogorov 1-equation turbulence model, providing estimates for energy dissipation and proposing a simplified near-wall length scale that ensures physically consistent dissipation rates.

Contribution

It introduces a new near-wall length scale for the 1-equation turbulence model, improving its asymptotic behavior and energy dissipation estimates.

Findings

Derived an estimate for total energy dissipation in eddy viscosity models.

Proposed a modified length scale for near-wall turbulence modeling.

Ensured the model's dissipation rate aligns with physical expectations.

Abstract

We prove an estimate of total (viscous plus modelled turbulent) energy dissipation in general eddy viscosity models for shear flows. For general eddy viscosity models, we show that the ratio of the near wall average viscosity to the effective global viscosity is the key parameter. This result is then applied to the 1-equation, URANS model of turbulence for which this ratio depends on the specification of the turbulence length scale. The model, which was derived by Prandtl in 1945, is a component of a 2-equation model derived by Kolmogorov in 1942 and is the core of many unsteady, Reynolds averaged models for prediction of turbulent flows. Away from walls, interpreting an early suggestion of Prandtl, we set \begin{equation*} l=\sqrt{2}k^{+1/2}\tau, \hspace{50mm} \end{equation*} where $\tau =$ selected time scale. In the near wall region analysis suggests replacing the traditional $l=0.41d$ ($d=$ wall normal distance) with $l=0.41d\sqrt{d/L}$ giving, e.g., \begin{equation*} l=\min \left\{ \sqrt{2}k{}^{+1/2}\tau ,\text{ }0.41d\sqrt{\frac{d}{L}} \right\} . \hspace{50mm} \end{equation*} This $l(\cdot )$ results in a simpler model with correct near wall asymptotics. Its energy dissipation rate scales no larger than the physically correct $O(U^{3}/L)$, balancing energy input with energy dissipation.