HW 4

Problem 1

Write down the Reynolds Transport Theorem (RTT) from memory (review first if you need to, but don’t just copy it from something written).

Problem 2

Use the RTT to derive the species transport equation.

Problem 3

Use the RTT to derive the momentum transport equation. The Lagrangian conservation law is simply Newton’s second law, that is, the rate of change of momentum is the sum of the external forces. The forces we consider are gravity, pressure, and viscous. We write these net forces as integrals over a generic body. Pressure and viscous forces act on the surface; gravity forces act volumetrically. Let $\vec{M}$ denote momentum. Denote tensors with double overbars. The pressure force, viscous, and gravity (body) forces are

$$d\vec{F}_P=-P\vec{n}dA=-P\bar{\bar{\delta}}\cdot\vec{n}dA,$$$$d\vec{F}_v = -\bar{\bar{\tau}}\cdot\vec{n}dA,$$$$d\vec{F}_g = - \rho\vec{g}dV,$$

where $\bar{\bar{\delta}}$ is the unit tensor.

Problem 4

Use the RTT to derive the total energy transport equation. Total energy is internal plus kinetic: $E=U + \frac{1}{2}m\vec{v}\cdot\vec{v}$. The Lagrangian conservation law is simply the first law of thermodynamics:

$$\frac{dE_{sys}}{dt} = \dot{Q} + \dot{W}.$$

Here, $\dot{Q}$ is the integral of the heat flux vector $\vec{q}$ over the surface, and $\dot{W}$ is the work done on the body, force times distance per time, or, $d\dot{W} = -d\vec{F}\cdot\vec{v}.$