3.II.15C

Classical Dynamics | Part II, 2006

A particle of mass mm is constrained to move on the surface of a sphere of radius \ell.

The Lagrangian is given in spherical polar coordinates by

L=12m2(θ˙2+ϕ˙2sin2θ)+mgcosθ,L=\frac{1}{2} m \ell^{2}\left(\dot{\theta}^{2}+\dot{\phi}^{2} \sin ^{2} \theta\right)+m g \ell \cos \theta,

where gravity gg is constant. Find the two constants of the motion.

The particle is projected horizontally with velocity vv from a point whose depth below the centre is cosθ=D\ell \cos \theta=D. Find vv such that the particle trajectory

(i) just grazes the horizontal equatorial plane θ=π/2\theta=\pi / 2;

(ii) remains at depth DD for all time tt.

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