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Realizable k-ε

Properties

Model equations

The turbulence kinetic energy equation is given by:

DDt(ρk)=(ρDkk)+ρG23ρ(u)kρϵ+Sk \Ddt{\rho k} = \div \left(\rho D_k \grad k\right) + \rho G - \frac{2}{3}\rho \left(\div \u\right) k - \rho \epsilon + S_k

and the dissipation rate by:

DDt(ρϵ)=(ρDϵϵ)+C1ρSϵC2ρϵ2k+(νϵ)0.5+Sϵ \Ddt{\rho \epsilon} = \div \left(\rho D_\epsilon \grad \epsilon \right) + C_1 \rho \mag{\tensor{S}} \epsilon - C_2 \rho \frac{\epsilon^2}{k + \left(\nu \epsilon\right)^{0.5}} + S_\epsilon

The turbulence viscosity is calculated using:

νt=Cμk2ϵ \nu_t = C_{\mu} \frac{k^2}{\epsilon}

where the CμC_{\mu} is given by:

Cμ=1A0+AsUkϵ C_{\mu} = \frac{1}{A_0 + A_s U^{*} \frac{k}{\epsilon}}

Default model coefficients

Initialisation

Usage

The model is specified using:

RAS
{
turbulence on;
RASModel realizableKE;
}

Boundary conditions

Walls

Further information

Source code:

References:

  • Shih et al. 62