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UPSC 2022 Maths Optional Paper 2 Q5d — Step-by-Step Solution
10 marks · Section B
Lagrange's equations · Mechanics & Fluid Dynamics · asked 9× in 13 yrs · Read the full method →
Question
A particle at distance r from centre of force moves under central force F=−k/r2. Obtain Lagrangian and derive equations of motion.
Technique
Standard Lagrangian for central force; polar coordinates; PE from F=−dV/dr; EL equations for r and θ.
Solution
Setup. Central force F=−k/r2 (attractive, like gravity). Use plane polar coordinates (r,θ) for 2D motion (central force ⇒ angular momentum conservation ⇒ motion confined to a plane).
Step 1 — Kinetic and potential energy
KE: T=21m(r˙2+r2θ˙2).
PE: V such that F=−dV/dr. From F=−k/r2: dV/dr=k/r2, so V=−k/r+const. Take const = 0:
V=−rk.
(Note: V→0 as r→∞, V<0 for finite r — attractive potential.)
Step 2 — Lagrangian
L=T−V=21m(r˙2+r2θ˙2)+rk.
Step 3 — Equations of motion (Euler-Lagrange)
r equation: dtd(∂r˙∂L)−∂r∂L=0.
∂L/∂r˙=mr˙, d/dt = mr¨.
∂L/∂r=mrθ˙2−k/r2.
So mr¨−mrθ˙2+k/r2=0, i.e.
mr¨=mrθ˙2−r2k.
The mrθ˙2 is the centripetal (outward) effect; −k/r2 is the gravity pull inward.
θ equation: dtd(∂θ˙∂L)−∂θ∂L=0.
∂L/∂θ˙=mr2θ˙. d/dt(mr2θ˙)= ?
∂L/∂θ=0.
So dtd(mr2θ˙)=0, i.e. mr2θ˙= constant =Lz (angular momentum).
Step 4 — Summary
L=21m(r˙2+r2θ˙2)+rk.
Equations of motion:
Answer
mr¨=mrθ˙2−r2k,mr2θ˙=const.