Exact expressions for the unresolved stress in a finite-volume based large-eddy simulation
Syver Døving Agdestein, Roel Verstappen, Benjamin Sanderse
TL;DR
The work develops a discretization-aware framework that unifies large-eddy simulation with finite-volume methods to derive an exact residual-stress tensor (RST) for LES-FVM. For incompressible flows, the resulting LES-FVM RST is non-local and non-symmetric due to discretization and pressure projection, and it provides zero a-posteriori error in DNS-aided tests when used as a closure target. The approach demonstrates that discretization effects are central to accurate closure modeling and shows that Smagorinsky coefficients fitted to the discretization-informed RST improve performance. The results, validated in Burgers’ equation and 3D Navier–Stokes turbulence, offer a principled path to discretization-consistent closures and potential data-driven enhancements. Overall, this work bridges implicit and explicit LES closures by making discretization a first-class component of the residual and its closure.
Abstract
In this article we propose new discretization-informed expressions for the residual stress tensor (RST) in a finite-volume based large-eddy simulation (LES-FVM). In addition to the classical RST $\overline{u u} - \bar{u} \bar{u}$ resulting from the non-commutation between filtering and the nonlinear stress, our RST also contains contributions from the numerical flux, discrete divergence, and pressure terms. Unlike the classical RST, our proposed RST is non-symmetric and non-local. The proposed form of the RST is important for generating appropriate reference data for LES closure modeling. Based on DNS results of the 1D Burgers and 3D incompressible Navier-Stokes equations, we show that the discretization-induced parts of the RST play an important role in the LES-FVM equation for common LES filter widths. When the discrete contribution is included, our RST expression gives zero a-posteriori error in LES, while existing RST expressions give errors that increase over time. For a Smagorinsky model, we show that the Smagorinsky coefficient is higher when fitted to our new RST than when fitted to the classical RST and gives improved results.
