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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 rr from centre of force moves under central force F=k/r2F=-k/r^2. Obtain Lagrangian and derive equations of motion.

Technique

Standard Lagrangian for central force; polar coordinates; PE from F=dV/drF=-dV/dr; EL equations for rr and θ\theta.

Solution

Setup. Central force F=k/r2F=-k/r^2 (attractive, like gravity). Use plane polar coordinates (r,θ)(r,\theta) for 2D motion (central force ⇒ angular momentum conservation ⇒ motion confined to a plane).

Step 1 — Kinetic and potential energy

KE: T=12m(r˙2+r2θ˙2)T=\dfrac{1}{2}m(\dot r^2+r^2\dot\theta^2).

PE: VV such that F=dV/drF=-dV/dr. From F=k/r2F=-k/r^2: dV/dr=k/r2dV/dr=k/r^2, so V=k/r+constV=-k/r+\text{const}. Take const = 0:

V=kr.V=-\dfrac{k}{r}.

(Note: V0V\to 0 as rr\to\infty, V<0V<0 for finite rr — attractive potential.)

Step 2 — Lagrangian

L=TV=12m(r˙2+r2θ˙2)+kr.L=T-V=\dfrac{1}{2}m(\dot r^2+r^2\dot\theta^2)+\dfrac{k}{r}.

Step 3 — Equations of motion (Euler-Lagrange)

rr equation: ddt ⁣(Lr˙)Lr=0\dfrac{d}{dt}\!\left(\dfrac{\partial L}{\partial\dot r}\right)-\dfrac{\partial L}{\partial r}=0.

L/r˙=mr˙\partial L/\partial\dot r=m\dot r, d/dtd/dt = mr¨m\ddot r.

L/r=mrθ˙2k/r2\partial L/\partial r=m r\dot\theta^2-k/r^2.

So mr¨mrθ˙2+k/r2=0m\ddot r-mr\dot\theta^2+k/r^2=0, i.e.

mr¨=mrθ˙2kr2.m\ddot r=mr\dot\theta^2-\dfrac{k}{r^2}.

The mrθ˙2mr\dot\theta^2 is the centripetal (outward) effect; k/r2-k/r^2 is the gravity pull inward.

θ\theta equation: ddt ⁣(Lθ˙)Lθ=0\dfrac{d}{dt}\!\left(\dfrac{\partial L}{\partial\dot\theta}\right)-\dfrac{\partial L}{\partial\theta}=0.

L/θ˙=mr2θ˙\partial L/\partial\dot\theta=mr^2\dot\theta. d/dt(mr2θ˙)=d/dt(mr^2\dot\theta)= ?

L/θ=0\partial L/\partial\theta=0.

So ddt(mr2θ˙)=0\dfrac{d}{dt}(mr^2\dot\theta)=0, i.e. mr2θ˙=mr^2\dot\theta= constant =Lz=L_z (angular momentum).

Step 4 — Summary

  L=12m(r˙2+r2θ˙2)+kr.  \boxed{\;L=\dfrac{1}{2}m(\dot r^2+r^2\dot\theta^2)+\dfrac{k}{r}.\;}

Equations of motion:

Answer

  mr¨=mrθ˙2kr2,mr2θ˙=const.  \boxed{\;m\ddot r=mr\dot\theta^2-\dfrac{k}{r^2},\quad mr^2\dot\theta=\text{const}.\;}
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