Nonlinear eddy viscosity and algebraic stress models for solving complex turbulent flows

By T. Gatski, T. Jongen. 2000

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Computational study of flow around a simplified car body (2008, methodology): “All of them base on the same pressure-strain correlation model, namely the quasi-linear SSG model [15].”
Role of solar wind turbulence in the coupling of the solar wind to the Earth's magnetosphere (2003, methodology): “When a turbulence model is used in a simulation to represent the affects of turbulence with transport coefficients, the most important coefficient is eddy viscosity, which is an approximation to the Reynolds stress [e.g., Okamoto, 1994; Gatski and Jongen, 2000].”
Turbulence Modeling in the Age of Data (2018, methodology): “For instance, with the assumption that the Reynolds stress tensor is only a function of the local, averaged velocity gradient tensor, the Cayley-Hamilton theorem can be applied to derive an exact expansion basis (Gatski and Jongen 2000).”
Dynamics of attached turbulent cavitating flows (2001, background): “In addition to the above-mentioned approaches, there are also proposals based on nonlinear eddy viscosity and algebraic stress models [90], very large eddy simulation [91], and large eddy simulation [92].”