In the Navier Stokes' equation:
$\rho_0 \left( \frac{\partial v}{\partial t} + v \cdot \nabla v\right) = -\nabla p + \mu \nabla^2 v + \hat{f}$
I included the temperature variation of density as per the Boussinesq approximation as
$\hat{f} = \rho_0(1-\alpha\Delta T)g\hat{k}$.
Choosing a viscous time scale $t^* = \frac{t}{d^2/\nu}$ where $d$ is a measure of length (in this case, film thickness) and non-dimensionalizing length and velocity with:
$x^*=x/d$ and $v^*=\frac{v}{\nu/d}$, the Navier Stokes' equation is modified to:
$\rho_0\left(\frac{\nu^2}{d^3} \frac{\partial v}{\partial t} + \frac{\nu^2}{d^3} v\cdot\nabla v \right) = -\frac{1}{d}\nabla p + \frac{\mu\nu}{d^3} \nabla^2 v + \rho_0(1 - \alpha \Delta T) g\hat{k}$.
Dividing throughout by $\frac{\rho_0 \nu^2}{d^3}$, while realizing that the non-dimensional pressure falls out as $\frac{\rho_0 \nu^2}{d^2}$, I get:
$\frac{\partial v}{\partial t} + v\cdot\nabla v = -\nabla p + \nabla^2 v + \frac{gd^3}{\nu}(1 - \alpha \Delta T)g\hat{k}$
Further splitting these terms for simplification:
$\frac{\partial v}{\partial t} + v\cdot\nabla v = -\nabla p + \nabla^2 v + \frac{g d^3}{\nu^2}\hat{k} - \frac{gd^3}{\nu^2} \alpha \Delta T \hat{k}$
Recognizing the following non dimensional numbers:
- Galileo number, $Ga = \frac{g d^3}{\nu^2}$
- Grashoff number, $Gr = \frac{gd^3}{\nu^2} \alpha \Delta T = \frac{Ra}{Pr}$
Where $Ra$ is the Rayleigh number and $Pr$ is the Prandtl number.
I rewrite my now non dimensional Navier Stokes' equation as:
$\frac{\partial v}{\partial t} + v \cdot \nabla v = -\nabla (p - Ga z \hat{k} + Gr z \hat{k}) + \nabla^2 v$
Where $z$ is the z coordinate and $\hat{k}$ is the unit normal in the $z$ direction.
Is this approach flawed since when I compare this with page 2 of this, equation 4 in Bestehorn et al. and equations 5 thru 7 in Ybarra et al., they all have a temperature difference multiplied with the Rayleight number which doesn't make sense.
Did I do something wrong?