Properties

Model equations

The turbulence kinetic energy equation is given by:

\[\Ddt{\rho k} = \div \left(\rho D_k \grad k\right) + \rho G - \frac{2}{3}\rho \left(\div \u\right) k - \rho \epsilon + S_k\]

and the dissipation rate by:

\[\Ddt{\rho \epsilon} = \div \left(\rho D_\epsilon \grad \epsilon \right) + C_1 \rho \mag{\tensor{S}} \epsilon - C_2 \rho \frac{\epsilon^2}{k + \left(\nu \epsilon\right)^{0.5}} + S_\epsilon\]

The turbulence viscosity is calculated using:

\[\nu_t = C_{\mu} \frac{k^2}{\epsilon}\]

where the \(C_{\mu}\) is given by:

\[C_{\mu} = \frac{1}{A_0 + A_s U^{*} \frac{k}{\epsilon}}\]

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]