The math optional, made finite. Daily Practice

Work and Potential Energy; Conservation

At a Glance

Why This Chapter Matters

This atom appeared once (2017) as a Section B question worth 16 marks — a full energy-methods derivation. UPSC uses it to test whether you can connect the line-integral definition of work to the potential-energy function, derive the work–energy theorem, and apply conservation of energy to a concrete mechanical system. A structured derivation with a numerical application earns full marks.

Minimum Theory

Work done by a force

For a particle moving along a path CC, the work done by force F\mathbf{F} is:

W=CFdr=C(Fxdx+Fydy+Fzdz)W = \int_C \mathbf{F} \cdot d\mathbf{r} = \int_C (F_x\,dx + F_y\,dy + F_z\,dz)

For a constant force: W=FΔr=FdcosαW = \mathbf{F}\cdot\Delta\mathbf{r} = F\,d\cos\alpha, where α\alpha is the angle between F\mathbf{F} and displacement.

Kinetic energy and work–energy theorem

Kinetic energy: T=12mv2T = \tfrac{1}{2}m|\mathbf{v}|^2.

From Newton’s second law F=mr¨\mathbf{F} = m\ddot{\mathbf{r}}:

WAB=ABFdr=ABmr¨r˙dt=ddt(12mv2)dt=TBTAW_{A\to B} = \int_A^B \mathbf{F}\cdot d\mathbf{r} = \int_A^B m\ddot{\mathbf{r}}\cdot\dot{\mathbf{r}}\,dt = \frac{d}{dt}\left(\tfrac{1}{2}m|\mathbf{v}|^2\right)\,dt = T_B - T_A

This is the work–energy theorem: work done equals change in kinetic energy.

Conservative forces and potential energy

A force F\mathbf{F} is conservative if CFdr=0\oint_C \mathbf{F}\cdot d\mathbf{r} = 0 for every closed path, equivalently ×F=0\nabla\times\mathbf{F} = \mathbf{0}.

For a conservative force, there exists a scalar potential energy V(r)V(\mathbf{r}) such that:

F=V,i.e.,Fx=Vx,  Fy=Vy,  Fz=Vz\mathbf{F} = -\nabla V, \quad \text{i.e.,}\quad F_x = -\frac{\partial V}{\partial x},\; F_y = -\frac{\partial V}{\partial y},\; F_z = -\frac{\partial V}{\partial z}

Work done by a conservative force:

WAB=ABFdr=ABdV=VAVBW_{A\to B} = \int_A^B \mathbf{F}\cdot d\mathbf{r} = -\int_A^B dV = V_A - V_B

Conservation of mechanical energy

Combining the work–energy theorem with the potential energy expression (all forces conservative):

TBTA=VAVB    TA+VA=TB+VBT_B - T_A = V_A - V_B \implies T_A + V_A = T_B + V_B

E=T+V=constant\boxed{E = T + V = \text{constant}}

Common potential energies

Power

P=dWdt=FvP = \frac{dW}{dt} = \mathbf{F}\cdot\mathbf{v}

Units: watts (W) = J/s.

Question Archetypes

ArchetypeRecognition
energy-conservation-derivation”Derive the principle of conservation of energy” or “using energy methods, find the speed/height/extension at a given point”

energy-conservation-derivation (1 question; 2017)

Recognition Cues

Solution Template

  1. Identify all forces; determine which are conservative.
  2. Write T=12mv2T = \tfrac{1}{2}mv^2 and the appropriate VV for each conservative force.
  3. Apply T+V=ET + V = E at two key positions (usually initial state and state of interest).
  4. Solve the resulting algebraic equation for the unknown.
  5. State the answer with correct units; verify dimensions.

Worked Example

2017 Paper 1, 2017-P1-Q8b (16 marks)

A particle of mass mm is attached to one end of a light elastic spring of natural length ll and modulus of elasticity λ\lambda. The other end of the spring is fixed to a point AA on a smooth horizontal table. The particle is held at rest at a distance l+al + a from AA and released. Derive the equation of motion from energy principles and find the speed of the particle when it returns to the natural length position.

Step 1. Set up coordinates and forces.

Let xx denote the extension of the spring beyond natural length ll. At initial release, x=ax = a; at natural length, x=0x = 0.

The elastic restoring force is F=λlxF = -\dfrac{\lambda}{l}\,x (Hooke’s law, tension positive towards AA).

This is conservative with potential energy:

V=λx22lV = \frac{\lambda x^2}{2l}

(since F=dV/dxF = -dV/dx). Kinetic energy: T=12mx˙2T = \tfrac{1}{2}m\dot{x}^2.

Step 2. State total energy at initial position.

At x=ax = a, x˙=0\dot{x} = 0:

E=T+V=0+λa22l=λa22lE = T + V = 0 + \frac{\lambda a^2}{2l} = \frac{\lambda a^2}{2l}

Step 3. Apply conservation of energy.

At general extension xx:

12mx˙2+λx22l=λa22l\frac{1}{2}m\dot{x}^2 + \frac{\lambda x^2}{2l} = \frac{\lambda a^2}{2l}

Differentiating with respect to tt gives the equation of motion:

mx¨+λlx=0    x¨+ω2x=0,ω2=λmlm\ddot{x} + \frac{\lambda}{l}x = 0 \implies \ddot{x} + \omega^2 x = 0, \quad \omega^2 = \frac{\lambda}{ml}

This is simple harmonic motion.

Step 4. Speed at natural length (x=0x = 0).

Setting x=0x = 0 in the energy equation:

12mv2+0=λa22l    v2=λa2ml\frac{1}{2}mv^2 + 0 = \frac{\lambda a^2}{2l} \implies v^2 = \frac{\lambda a^2}{ml}

v=aλml\boxed{v = a\sqrt{\frac{\lambda}{ml}}}

Common Traps

Marks-Aware Writing

This is a 16-mark Section B derivation. Examiners expect:

  1. Definition of TT and VV with correct formulas for the specific system (3 marks).
  2. Calculation of total energy EE from initial conditions (2 marks).
  3. Conservation equation written in full at general position (3 marks).
  4. Equation of motion derived by differentiation (3 marks).
  5. Application — substituting the specific position and solving for the unknown (3 marks).
  6. Correct final answer with units (2 marks).

Show every algebraic step; do not jump from the energy equation to the answer without showing the substitution.

Practice Set

Only one historical question on this atom (shown above).

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