← 2025 Paper 2
UPSC Maths 2025 Paper 2 Q8c-i — Solution
10 marks · Section B
Question
A particle of mass m moves in a force field of potential V(r)=−r2kcosθ, k is constant. Find the Hamiltonian and the Hamilton’s equations in spherical polar coordinates (r,θ,ϕ).
Technique
Work in spherical polar coordinates: write the kinetic energy, form the canonical momenta pq=∂L/∂q˙, invert to express q˙ in momenta, build H=T+V (natural, time-independent system), and write Hamilton’s equations q˙=∂H/∂pq, p˙q=−∂H/∂q.
Solution
Kinetic energy and Lagrangian
In spherical coordinates (r,θ,ϕ) the speed-squared is
v2=r˙2+r2θ˙2+r2sin2θϕ˙2.
So
T=21m(r˙2+r2θ˙2+r2sin2θϕ˙2),L=T−V=T+r2kcosθ.
Canonical momenta
p_\theta = \frac{\partial L}{\partial\dot\theta} = m r^2\dot\theta,\quad
p_\phi = \frac{\partial L}{\partial\dot\phi} = m r^2\sin^2\theta\,\dot\phi.$$
Invert:
$$\dot r = \frac{p_r}{m},\qquad \dot\theta = \frac{p_\theta}{m r^2},\qquad \dot\phi = \frac{p_\phi}{m r^2\sin^2\theta}.$$
### Hamiltonian
Since the coordinate transformation is time-independent and $V$ has no velocity dependence, $H = T + V$ expressed in momenta:
$$\boxed{H = \frac{p_r^2}{2m} + \frac{p_\theta^2}{2m r^2} + \frac{p_\phi^2}{2m r^2\sin^2\theta} - \frac{k\cos\theta}{r^2}.}$$
### Hamilton's equations
Coordinate equations $\dot q = \partial H/\partial p_q$:
$$\dot r = \frac{p_r}{m},\qquad \dot\theta = \frac{p_\theta}{m r^2},\qquad \dot\phi = \frac{p_\phi}{m r^2\sin^2\theta}.$$
Momentum equations $\dot p_q = -\partial H/\partial q$:
$$\dot p_r = -\frac{\partial H}{\partial r} = \frac{p_\theta^2}{m r^3} + \frac{p_\phi^2}{m r^3\sin^2\theta} - \frac{2k\cos\theta}{r^3},$$
$$\dot p_\theta = -\frac{\partial H}{\partial\theta} = \frac{p_\phi^2\cos\theta}{m r^2\sin^3\theta} - \frac{k\sin\theta}{r^2},$$
$$\dot p_\phi = -\frac{\partial H}{\partial\phi} = 0.$$
The last equation shows $\phi$ is cyclic (ignorable): $p_\phi = m r^2\sin^2\theta\,\dot\phi$ is conserved (azimuthal angular momentum). The energy $H$ is conserved since $\partial H/\partial t = 0$.
## Answer
$$H = \frac{p_r^2}{2m} + \frac{p_\theta^2}{2mr^2} + \frac{p_\phi^2}{2mr^2\sin^2\theta} - \frac{k\cos\theta}{r^2},$$
with Hamilton's equations
$$\dot r = \tfrac{p_r}{m},\quad \dot\theta = \tfrac{p_\theta}{mr^2},\quad \dot\phi = \tfrac{p_\phi}{mr^2\sin^2\theta},$$
$$\dot p_r = \frac{p_\theta^2}{mr^3} + \frac{p_\phi^2}{mr^3\sin^2\theta} - \frac{2k\cos\theta}{r^3},\quad
\dot p_\theta = \frac{p_\phi^2\cos\theta}{mr^2\sin^3\theta} - \frac{k\sin\theta}{r^2},\quad
\dot p_\phi = 0.$$
$\phi$ is cyclic, so $p_\phi$ is conserved.