Paper 4, Section II, C

Classical Dynamics
Part II, 2015

Consider a rigid body with angular velocity ω\boldsymbol{\omega}, angular momentum L\mathbf{L} and position vector r\mathbf{r}, in its body frame.

(a) Use the expression for the kinetic energy of the body,

12d3rρ(r)r˙2,\frac{1}{2} \int d^{3} \mathbf{r} \rho(\mathbf{r}) \dot{\mathbf{r}}^{2},

to derive an expression for the tensor of inertia of the body, I. Write down the relationship between L,I\mathbf{L}, \mathbf{I} and ω\boldsymbol{\omega}.

(b) Euler's equations of torque-free motion of a rigid body are

I1ω˙1=(I2I3)ω2ω3I2ω˙2=(I3I1)ω3ω1I3ω˙3=(I1I2)ω1ω2\begin{aligned} &I_{1} \dot{\omega}_{1}=\left(I_{2}-I_{3}\right) \omega_{2} \omega_{3} \\ &I_{2} \dot{\omega}_{2}=\left(I_{3}-I_{1}\right) \omega_{3} \omega_{1} \\ &I_{3} \dot{\omega}_{3}=\left(I_{1}-I_{2}\right) \omega_{1} \omega_{2} \end{aligned}

Working in the frame of the principal axes of inertia, use Euler's equations to show that the energy EE and the squared angular momentum L2\mathbf{L}^{2} are conserved.

(c) Consider a cuboid with sides a,ba, b and cc, and with mass MM distributed uniformly.

(i) Use the expression for the tensor of inertia derived in (a) to calculate the principal moments of inertia of the body.

(ii) Assume b=2ab=2 a and c=4ac=4 a, and suppose that the initial conditions are such that

L2=2I2E\mathbf{L}^{2}=2 I_{2} E

with the initial angular velocity ω\omega perpendicular to the intermediate principal axis e2\mathbf{e}_{2}. Derive the first order differential equation for ω2\omega_{2} in terms of E,ME, M and aa and hence determine the long-term behaviour of ω\boldsymbol{\omega}.