The effects of turbulence modeling on the prediction of equilibrium states
of turbulent buoyant shear flows were investigated. The velocity field mode
ls used include a two-equation closure, a Reynolds-stress closure assuming
two different pressure-strain models and three different dissipation rate t
ensor models. As for the thermal field closure models, two different pressu
re-scrambling models and nine different temperature variance dissipation ra
te (epsilon (theta)) equations were considered. The emphasis of this paper
is focused on the effects of the epsilon (theta)-equation, of the dissipati
on rate models, of the pressure-strain models and of the pressure-scramblin
g models on the prediction of the approach to equilibrium turbulence. Equil
ibrium turbulence is defined by the time rate of change of the scaled Reyno
lds stress anisotropic tensor and heat flux vector becoming zero. These con
ditions lead to the equilibrium state parameters, given by (P) over tilde/e
psilon, (P) over tilde (theta)/epsilon (theta), R = (<(<theta>(2))over bar>
/2 epsilon (theta))/(k/epsilon), Sk/epsilon and G/epsilon, becoming constan
t. Here, (P) over tilde and (P) over tilde (theta) are the production of tu
rbulent kinetic energy k and temperature variance <(<theta>(2))over bar>, r
espectively, epsilon and epsilon (theta) are their respective dissipation r
ates, R is the mixed time scale ratio, G is the buoyant production of k and
S is the mean shear gradient. Calculations show that the epsilon (theta)-e
quation has a significant effect on the prediction of the approach to equil
ibrium turbulence. For a particular epsilon (theta)-equation, all velocity
closure models considered give an equilibrium state if anisotropic dissipat
ion is accounted for in one form or another in the dissipation rate tensor
or in the epsilon -equation. It is further found that the models considered
for the pressure-strain tensor and the pressure-scrambling vector have lit
tle or no effect on the prediction of the approach to equilibrium turbulenc
e.