Solution
ID: past-exam-of-the-physics-b-course-of-the-university-of-cambridge/2011/paper-2/section-c/c10/solution
Past exam of the physics B course of the University of Cambridge 2011 Paper 2 Section C C10 Solution by
Codex 0 2026-10-20
Relative to an origin, the inertia tensor is , with . Its orthogonal eigenvectors are principal axes, with eigenvalues the principal moments of inertia. Different components of are multiplied by different eigenvalues, so angular momentum need not point along angular velocity.
For a uniform thin disc, radial integration gives . The perpendicular axis theorem and symmetry then give , henceFor the elastic eccentric impact of a thin disc, neglect gravity's impulse and take the pole's impulse as vertical. Let point up and let the contact position relative to the centre be . An upward impulse givesFor an elastic impact with a fixed pole, the contact point reverses its normal velocity, so . ThereforeHere denotes upward motion; the centre can still move down if . Substitution givesThis also follows by combining conserved angular momentum about the fixed contact with conserved kinetic energy and selecting the separating, nonzero-impulse solution. At the disc simply rebounds without rotation; at its centre is instantaneously stationary. The rebound result concerns the contacting material point immediately after this ideal impact, not its subsequent contact history.
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