I'm working through Acheson's 'Elementary Fluid Dynamics' and i'm having trouble deriving the conservation of energy equation (exercise 1.4)
$\frac{d}{dt} \int_V \frac{\rho \vert u\vert^2}{2} dV = -\int_{\partial V}(p +\rho \phi + \frac{\rho \vert u\vert^2}{2})\mathbf{u} \cdot \mathbf{n}dS$
where $\mathbf{u}$ is the velocity of the fluid, $\rho$ is the density of the fluid, $\phi$ is the gravitational potential and $p$ is the atmospheric pressure.
No matter what I do I can't get the factor of $\frac{1}{2}$ on the left hand side. Here's my attempt:
Start from Eulers equation, $\frac{\partial \mathbf{u}}{\partial t} + \mathbf{\omega} \times \mathbf{u} = - \nabla (\frac{p}{\rho} +\phi + \frac{1}{2}\vert u\vert ^2)$, and multiply by $\rho$ and dot both sides with $\mathbf{u}$ to get
$\frac{\partial \rho \vert u\vert^2}{\partial t} = - \nabla \tau \cdot \mathbf{u}$, where $\tau = \frac{p}{\rho} +\phi + \frac{1}{2}\vert u\vert ^2$.
Now, using the identity $\nabla \cdot (\tau \mathbf{u}) = \nabla \tau \cdot \mathbf{u} + \tau \nabla \cdot \mathbf{u}$ and the incompresibility condition, this becomes $\frac{\partial \rho \vert u\vert ^2}{\partial t} = - \nabla \cdot (\tau \mathbf{u})$. Integrating over a closed volume $V$ and using the divergence theorem gives
$\frac{d}{dt} \int_V \rho \vert u\vert^2 dV = -\int_{\partial V}(p +\rho \phi + \frac{\rho \vert u\vert^2}{2})\mathbf{u} \cdot \mathbf{n}dS$.
Can anyone see where the missing 2 went? Sorry about the poor latex, i'm learning that too!
