The math optional, made finite. Daily Practice

Work-energy theorem

At a Glance

Why This Chapter Matters

Both UPSC questions on this atom are compulsory 10-mark items from Section B — fast, reliable marks. The 2019 question is a straightforward work-as-integral problem that takes under six minutes. The 2017 question uses energy conservation to derive a motion equation on a cardioid, testing whether you can correctly identify gravitational depth and elastic potential energy. Together they form two reusable templates that cover every work-energy question the examiner has written.

Minimum Theory

Work-energy theorem. The work done by a force F\mathbf{F} as a particle moves from AA to BB along a path equals the change in kinetic energy:

WAB=TBTA=ABFdr.W_{A\to B} = T_B - T_A = \int_A^B \mathbf{F}\cdot d\mathbf{r}.

For a conservative force with potential VV (where F=V\mathbf{F} = -\nabla V), this is simply W=VAVBW = V_A - V_B.

Conservation of energy. If all forces are conservative (gravity, elastic string, etc.), the total mechanical energy is constant: T+V=ET + V = E. Set EE using the initial conditions at the release point; then write T+Vgrav+Velastic=ET + V_\text{grav} + V_\text{elastic} = E at a general position to get the equation of motion.

Inverse-square gravity. At distance rr from the centre of the earth, the attractive force per unit mass is μ/r2\mu/r^2 (or, for a particle of weight WW on the surface of a body of radius hh: calibrate k=Wh2k = Wh^2 so the force at distance rr is k/r2k/r^2). The work done in falling from r=r1r = r_1 to r=r2<r1r = r_2 < r_1 is

W=k ⁣(1r21r1).W = k\!\left(\frac{1}{r_2} - \frac{1}{r_1}\right).

Elastic potential energy. For a string of natural length aa and modulus of elasticity λ\lambda, the elastic PE of extension ee is λe2/(2a)\lambda e^2/(2a).

Question Archetypes

ArchetypeRecognition cue
energy-conservationBead/ring on a wire with elastic string released from rest; “show by energy conservation that…“
work-done-integralParticle falls under inverse-square (or variable) force; “show the work done is…“

energy-conservation (1 question(s); 2017)

Recognition Cues

Solution Template

  1. Write the speed v2=r˙2+r2θ˙2v^2 = \dot r^2 + r^2\dot\theta^2 in terms of θ˙\dot\theta using the curve equation r=r(θ)r = r(\theta).
  2. Identify the gravitational PE using the depth below a fixed datum (downward vertical = direction of positive depth).
  3. Compute the elastic PE: extension e=ra0e = r - a_0 (natural length a0a_0); PE =λe2/(2a0)= \lambda e^2/(2a_0).
  4. Write T+Vgrav+Velastic=0T + V_\text{grav} + V_\text{elastic} = 0 (since total energy is zero: released from rest at a configuration with zero PE).
  5. Divide by common factors to obtain the stated equation.

Worked Example

2017 Paper 1, 2017-P1-Q5c (10 marks)

A fixed wire is in the shape of the cardioid r=a(1+cosθ)r=a(1+\cos\theta), the initial line being the downward vertical. A small ring of mass mm slides on the wire and is attached to the point r=0r=0 of the cardioid by an elastic string of natural length aa and modulus of elasticity 4mg4mg. The string is released from rest when the string is horizontal. Show by energy conservation that aθ˙2(1+cosθ)gcosθ(1cosθ)=0a\dot\theta^2(1+\cos\theta)-g\cos\theta(1-\cos\theta)=0.

Step 1 — Speed. With r=a(1+cosθ)r = a(1+\cos\theta), r˙=asinθθ˙\dot r = -a\sin\theta\,\dot\theta:

v2=r˙2+r2θ˙2=a2sin2θθ˙2+a2(1+cosθ)2θ˙2=2a2θ˙2(1+cosθ).v^2 = \dot r^2 + r^2\dot\theta^2 = a^2\sin^2\theta\,\dot\theta^2 + a^2(1+\cos\theta)^2\dot\theta^2 = 2a^2\dot\theta^2(1+\cos\theta).

T=12mv2=ma2θ˙2(1+cosθ).T = \tfrac12 m v^2 = ma^2\dot\theta^2(1+\cos\theta).

Step 2 — Gravitational PE. The initial line is the downward vertical, so the depth below OO is rcosθ=a(1+cosθ)cosθr\cos\theta = a(1+\cos\theta)\cos\theta. Taking OO as datum:

Vg=mga(1+cosθ)cosθ.V_g = -mg\cdot a(1+\cos\theta)\cos\theta.

Step 3 — Elastic PE. Natural length aa, modulus λ=4mg\lambda=4mg, current length r=a(1+cosθ)r=a(1+\cos\theta), extension e=acosθe = a\cos\theta:

Ve=4mg2a(acosθ)2=2mgacos2θ.V_e = \frac{4mg}{2a}(a\cos\theta)^2 = 2mga\cos^2\theta.

Step 4 — Zero initial energy. At release, the string is horizontal, so the radius vector is horizontal. Since the initial line is the downward vertical, horizontal means θ=π/2\theta = \pi/2. There r=ar = a, e=0e = 0, T=0T = 0, Vg=0V_g = 0, Ve=0V_e = 0, hence E0=0E_0 = 0.

Step 5 — Conservation. T+Vg+Ve=0T + V_g + V_e = 0:

ma2θ˙2(1+cosθ)mga(1+cosθ)cosθ+2mgacos2θ=0.ma^2\dot\theta^2(1+\cos\theta) - mga(1+\cos\theta)\cos\theta + 2mga\cos^2\theta = 0.

Divide by mama:

aθ˙2(1+cosθ)gcosθ(1+cosθ2cosθ)=0.a\dot\theta^2(1+\cos\theta) - g\cos\theta(1+\cos\theta - 2\cos\theta) = 0.

aθ˙2(1+cosθ)gcosθ(1cosθ)=0.\boxed{a\dot\theta^2(1+\cos\theta) - g\cos\theta(1-\cos\theta) = 0.}

Common Traps


work-done-integral (1 question(s); 2019)

Recognition Cues

Solution Template

  1. Write the force law F(r)=k/r2F(r) = k/r^2.
  2. Calibrate kk from the surface weight: W=k/h2k=Wh2W = k/h^2 \Rightarrow k = Wh^2.
  3. Convert “height above surface” to “distance from centre”: add the earth’s radius.
  4. Integrate W=rendrstartk/r2dr=k[1/r]W = \int_{r_\text{end}}^{r_\text{start}} k/r^2\,dr = k[-1/r].
  5. Substitute limits and simplify.

Worked Example

2019 Paper 1, 2019-P1-Q5d (10 marks)

The force of attraction of a particle by the earth is inversely proportional to the square of its distance from the earth’s centre. A particle, whose weight on the surface of the earth is WW, falls to the surface of the earth from a height 3h3h above it. Show that the magnitude of work done by the earth’s attraction force is 34hW\dfrac{3}{4}hW, where hh is the radius of the earth.

Step 1 — Force law and calibration. Force at distance rr is F(r)=k/r2F(r) = k/r^2. At the surface (r=hr = h), F=WF = W, so k=Wh2k = Wh^2.

Step 2 — Distance from centre. Height 3h3h above the surface means starting distance rstart=h+3h=4hr_\text{start} = h + 3h = 4h from the centre.

Step 3 — Work integral. Force and displacement both point inward (work is positive):

W=h4hWh2r2dr=Wh2 ⁣[1r]h4h=Wh2 ⁣(1h14h)=Wh34.\mathcal{W} = \int_h^{4h} \frac{Wh^2}{r^2}\,dr = Wh^2\!\left[-\frac{1}{r}\right]_h^{4h} = Wh^2\!\left(\frac{1}{h} - \frac{1}{4h}\right) = Wh\cdot\frac{3}{4}.

W=34hW.\boxed{\mathcal{W} = \frac{3}{4}\,hW.}

Common Traps

Marks-Aware Writing

A 10-mark answer must: write the correct energy form or force law; set up the computation cleanly; execute the integration (or energy balance) in full; state the final result. In the work-done question, showing the integral and evaluating both limits earns most marks — the setup and result together are worth about 8 marks. In the energy-conservation question, the kinetic energy calculation (Step 1) typically earns 3–4 marks; potential energy terms another 3–4; the final algebraic simplification 2–3.

Practice Set

We've mapped all 13 years of this exam. Get new chapters, tools, and solutions as we release them — free.