[ANSYS, Inc. Logo] return to home search
next up previous contents index

4.9.6 Modeling the Turbulence Kinetic Energy

In general, when the turbulence kinetic energy is needed for modeling a specific term, it is obtained by taking the trace of the Reynolds stress tensor:


 k = \frac{1}{2}\overline{u'_i u'_i} (4.9-27)

As described in Section  4.9.9, an option is available in ANSYS FLUENT to solve a transport equation for the turbulence kinetic energy in order to obtain boundary conditions for the Reynolds stresses. In this case, the following model equation is used:


 \frac{\partial}{\partial t} (\rho k) + \frac{\partial}{\part... ...{ii} + G_{ii}\right) - \rho \epsilon (1 + 2 {\rm M}_t^2) + S_k (4.9-28)

where $\sigma_k = 0.82$ and $S_k$ is a user-defined source term. Equation  4.9-28 is obtainable by contracting the modeled equation for the Reynolds stresses (Equation  4.9-1). As one might expect, it is essentially identical to Equation  4.4-1 used in the standard $k$- $\epsilon$ model.

Although Equation  4.9-28 is solved globally throughout the flow domain, the values of $k$ obtained are used only for boundary conditions. In every other case, $k$ is obtained from Equation  4.9-27. This is a minor point, however, since the values of $k$ obtained with either method should be very similar.


next up previous contents index Previous: 4.9.5 Effects of Buoyancy
Up: 4.9 Reynolds Stress Model
Next: 4.9.7 Modeling the Dissipation
Release 12.0 © ANSYS, Inc. 2009-01-23