Standard k-epsilon model
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</math> | </math> | ||
+ | == Effect of Bouyancy == | ||
+ | |||
+ | <math> | ||
+ | P_b = \beta g_i \frac{\mu_t}{{\rm Pr}_t} \frac{\partial T}{\partial x_i} | ||
+ | </math> | ||
+ | |||
+ | |||
+ | <br> | ||
+ | where Pr<sub>t</sub> is the turbulent Prandtl number for energy and g<sub>i</sub> is the component of the gravitational vector in the ith direction. For the standard and realizable - models, the default value of Pr<sub>t</sub> is 0.85. | ||
+ | |||
+ | The coefficient of thermal expansion, <math> \beta </math> , is defined as <br> | ||
+ | <math> | ||
+ | \beta = - \frac{1}{\rho} \left(\frac{\partial \rho}{\partial T}\right)_p | ||
+ | </math> | ||
== Model Constants == | == Model Constants == |
Revision as of 00:32, 14 September 2005
Contents |
Transport Equation for standard k-epsilon model
For k
For dissipation
Modeling turbulent viscosity
Turbulent viscosity is modelled as:
Production of k
Where is the modulus of the mean rate-of-strain tensor, defined as :
Effect of Bouyancy
where Prt is the turbulent Prandtl number for energy and gi is the component of the gravitational vector in the ith direction. For the standard and realizable - models, the default value of Prt is 0.85.
The coefficient of thermal expansion, , is defined as
Model Constants