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Class 11 · Physics · Part 1

Chapter 5: Work, Energy and Power

Revision notes, practice numericals, a question bank, assertion and reason questions and answers to the NCERT questions. Tap a group to open it; opening one closes the others.

5.1Introduction and the scalar productWork, energy and power in physics; A · B

Precise meanings

  • In everyday speech 'work', 'energy' and 'power' are used loosely. In physics each has a precise meaning. Energy is the capacity to do work. Power is how fast work is done.
  • A farmer ploughing or a student studying are 'working' in daily life, but in physics work needs a force and a displacement.

The scalar (dot) product

  • A · B = A B cos θ, where θ is the angle between the vectors. The result is a scalar: A (B cos θ) = magnitude of A times the component of B along A.
  • It is commutative, A · B = B · A, and distributive, A · (B + C) = A · B + A · C. Also A · (λB) = λ (A · B).
  • Unit vectors: î · î = ĵ · ĵ = k̂ · k̂ = 1 and î · ĵ = ĵ · k̂ = k̂ · î = 0. In components A · B = Aₓ Bₓ + Ay By + Az Bz and A · A = A².
  • A · B = 0 if A and B are perpendicular (and non-zero).
  • Example 5.1: for F = (3 î + 4 ĵ − 5 k̂) and d = (5 î + 4 ĵ + 3 k̂): F · d = 15 + 16 − 15 = 16, F = d = √50, cos θ = 16/50 = 0.32 so θ = cos⁻¹ 0.32.
θFF cos θF sin θdisplacement dW = F d cos θ = F · donly F cos θ does work
Work done by a constant force: only the component of the force along the displacement contributes.
5.2–5.4Work, kinetic energy and the work-energy theoremW = F · d, K = ½mv², Kf − Ki = W

From kinematics to work and energy

  • For constant acceleration v² − u² = 2 a·d. Multiplying by m/2: ½mv² − ½mu² = m a · d = F · d.
  • Call K = ½ m v² the kinetic energy and W = F · d the work. Then Kf − Ki = W: the work-energy theorem. The change in kinetic energy equals the work done by the net force.

Work

  • Work of a constant force: W = F d cos θ = F · d. It is done by a force on a body over a displacement. 'Calculate the work done' is incomplete unless we say by which force (or group of forces) and over what displacement.
  • Work and energy have dimensions [M L² T⁻²]; the SI unit is the joule (1 J = 1 N m). Other units: erg (10⁻⁷ J), kWh (3.6 × 10⁶ J), eV (1.6 × 10⁻¹⁹ J).
  • Work is a scalar but can be positive (0° ≤ θ < 90°), negative (90° < θ ≤ 180°, e.g. friction) or zero.
  • No work is done if (i) the displacement is zero (pushing a rigid wall; holding a weight steadily), (ii) the force is zero (a block gliding on a smooth table), or (iii) the force is perpendicular to the displacement (gravity on a block on a smooth table; the earth's gravity on a satellite in a circular orbit).

Example highlights

  • Example 5.2: a raindrop of 1.00 g falls 1.00 km and reaches 50.0 m s⁻¹. ΔK = ½ × 10⁻³ × 50² = 1.25 J; work by gravity Wg = m g h = 10 J; work by the unknown resistive force Wr = ΔK − Wg = −8.75 J (negative).
  • Example 5.3: a cyclist skids to a stop in 10 m under a 200 N road force opposite to the motion: work done by the road = 200 × 10 × cos 180° = −2000 J. The work by the cycle on the road is zero because the road does not move. So the work done by the two forces of a third-law pair need not be equal and opposite.
  • Example 5.4: a 50 g bullet at 200 m s⁻¹ has K = 1000 J. It emerges with 10% of this energy: vf = √(2 × 100/0.05) = 63.2 m s⁻¹, a drop of only 68% in speed.

Kinetic energy

  • K is a scalar, always positive (or zero). It measures the work a moving body can do because of its motion (a mill grinding corn with a flowing stream, a sailing ship using the wind).
  • K and momentum: K = p²/2m. Doubling the speed makes K four times as large.
5.5–5.6Work done by a variable forceArea under the F–x graph, W = ∫ F dx

Area under the curve

  • For a small displacement Δx, ΔW = F(x) Δx (the area of a thin rectangle). Adding the rectangles and letting Δx → 0: W = ∫ F(x) dx from xᵢ to xf, the area under the F–x curve.
  • Areas below the axis count as negative work.
xF(x)xᵢxfshaded area = Σ F Δx → work W = ∫ F dxF(x)
Work done by a variable force: the area under the F–x curve between xᵢ and xf.

Example 5.5: pushing a trunk

  • A woman pushes a trunk with 100 N for 10 m, then her force falls linearly to 50 N at 20 m. Friction is 50 N (opposing). Work by the woman = rectangle + trapezium = 100 × 10 + ½ (100 + 50) × 10 = 1750 J. Work by friction = −50 × 20 = −1000 J.

Work-energy theorem for a variable force

  • In one dimension: dK/dt = d(½mv²)/dt = m v (dv/dt) = F v = F (dx/dt), so dK = F dx. Integrating: Kf − Ki = ∫ F dx = W.
  • The theorem is the integral form of Newton's second law, in scalar form. It does not contain the time information or the directional information of the vector second law.
  • Example 5.6: a 1 kg block enters a rough patch (0.1 m to 2.01 m) where Fr = −k/x with k = 0.5 J: Kf = ½mvᵢ² − k ln(2.01/0.1) = 2 − 0.5 ln 20.1 = 0.5 J, so vf = 1 m s⁻¹.
5.7–5.8Potential energy and conservation of mechanical energyConservative forces, F = −dV/dx, K + V = constant

Potential energy

  • Potential energy is 'stored' energy by virtue of position or configuration (a stretched bow, a raised ball, a compressed spring). It is defined only for conservative forces.
  • For gravity near the earth (h ≪ RE): V(h) = m g h, the negative of the work done by gravity in raising the body. F = −dV/dh = −m g.
  • In general F(x) = −dV/dx and ∫ F dx = Vᵢ − Vf. Equivalently ΔV = −F Δx.

Conservative forces

  • Three equivalent definitions: (i) F can be derived from a potential V(x) by F = −dV/dx; (ii) the work done depends only on the end points; (iii) the work done over a closed path is zero.
  • Gravity, the spring force and electrostatic forces are conservative. Friction is not: the work it does depends on the path and no potential energy can be defined for it.
  • The zero of potential energy is arbitrary. Once chosen it must be used consistently.

Conservation of mechanical energy

  • From ΔK = FΔx and −ΔV = FΔx we get Δ(K + V) = 0. So Kᵢ + V(xᵢ) = Kf + V(xf): the total mechanical energy of a system is conserved if the forces doing work are conservative.
  • A ball dropped from a height H: EH = m g H, Eh = m g h + ½ m vh², E₀ = ½ m vf². All are equal, giving vf = √(2 g H) and vh² = 2 g (H − h).
  • With a non-conservative force too, Ef − Eᵢ = Wnc, the work done by non-conservative forces (it depends on the path).

Example 5.7: a bob in a vertical circle

  • A bob of mass m on a string of length L is given a horizontal speed v₀ at the lowest point A so that the string goes slack only at the top C. At C: m g = m vC²/L so vC = √(g L). Energy at A equals that at C: ½ m v₀² = ½ m vC² + 2 m g L so v₀ = √(5 g L).
  • At B (level of the centre): vB = √(3 g L). The ratio of kinetic energies KB : KC = 3 : 1. After C the bob would move as a horizontal projectile if the string were cut.
LABCv₀vCAt A: v₀ = √(5 g L)At B: vB = √(3 g L)At C: vC = √(g L), T = 0KB : KC = 3 : 1
Example 5.7: a bob that just completes the vertical circle (the string goes slack only at the top).
5.9Potential energy of a springHooke's law, V = ½kx², energy exchange

The spring force

  • For an ideal spring Fs = −k x (Hooke's law), where x is the displacement from equilibrium and k the spring constant (N m⁻¹). A stiff spring has large k.
  • Work done by the spring force in stretching by xm: Ws = −½ k xm² (negative); the external force does +½ k xm². In general Ws = ½ k xᵢ² − ½ k xf², which depends on the end points only, and is zero for a cyclic process. The spring force is conservative.

Potential energy and conservation

  • V(x) = ½ k x² (zero at x = 0). Check: −dV/dx = −kx. If the block is released from rest at xm, ½ k xm² = ½ k x² + ½ m v² at any x.
  • The speed is maximum at x = 0: ½ m vm² = ½ k xm² so vm = xm √(k/m). K and V are complementary parabolas; their sum E is constant.
xenergy−xₘ+xₘ0E = K + VV = ½ k x²K = E − V
A block on a spring: V and K are complementary parabolas; E = K + V stays constant.

Examples 5.8 and 5.9

  • A 1000 kg car at 18 km h⁻¹ (5 m s⁻¹) hits a spring of k = 5.25 × 10³ N m⁻¹ on a smooth road: K = 1.25 × 10⁴ J = ½ k xm² gives xm = 2.00 m.
  • With friction (μ = 0.5) use the work-energy theorem: ½ m v² = ½ k xm² + μ m g xm, a quadratic equation; xm = 1.35 m, less than without friction. The time is not given by energy methods.
5.10PowerRate of doing work, P = F · v, watt, horse power

Definitions

  • Average power Pav = W/t. Instantaneous power P = dW/dt = F · v. Power is a scalar with dimensions [M L² T⁻³].
  • SI unit: the watt, 1 W = 1 J s⁻¹. 1 hp = 746 W.
  • kWh is a unit of energy (not power): 1 kWh = 10³ W × 3600 s = 3.6 × 10⁶ J. A 100 W bulb on for 10 hours uses 1 kWh.

Examples

  • Example 5.10: an elevator of 1800 kg (with load) rises at 2 m s⁻¹ against a 4000 N friction: F = m g + Ff = 18 000 + 4000 = 22 000 N and P = F v = 44 000 W ≈ 59 hp.
  • Constant acceleration from rest: P = F v = m a² t, so P ∝ t. Constant power: v ∝ t^(1/2) and x ∝ t^(3/2).
5.11CollisionsElastic, inelastic, one and two dimensions

Conservation laws in collisions

  • In all collisions of an isolated system the total linear momentum is conserved (the impulses on the two bodies are equal and opposite at every instant).
  • Elastic collision: the total kinetic energy after the collision equals that before. Completely inelastic: the bodies move together after the collision. Inelastic: some kinetic energy is lost (heat, sound, deformation).
  • Kinetic energy is conserved (in an elastic collision) only between the beginning and the end; during contact the bodies are deformed and part of the energy is momentarily stored (like a compressed spring).

One dimension

  • Completely inelastic (m₂ initially at rest): vf = m₁ v₁ᵢ/(m₁ + m₂) and the loss of kinetic energy is ΔK = ½ [m₁ m₂/(m₁ + m₂)] v₁ᵢ².
  • Elastic (m₂ initially at rest): v₁f = [(m₁ − m₂)/(m₁ + m₂)] v₁ᵢ and v₂f = [2 m₁/(m₁ + m₂)] v₁ᵢ (also v₂f = v₁ᵢ + v₁f).
  • Equal masses: v₁f = 0 and v₂f = v₁ᵢ (they exchange velocities). If m₂ ≫ m₁: v₁f ≈ −v₁ᵢ and v₂f ≈ 0 (the light ball rebounds).
  • Example 5.11 (neutron moderator): fractional KE kept by the neutron f₁ = [(m₁ − m₂)/(m₁ + m₂)]². For deuterium (m₂ = 2m₁) f₁ = 1/9 and the nucleus gets f₂ = 8/9; for carbon f₁ = 71.6%.
Elastic, equal massesm₁, speed vm₂ (at rest)⟹moves with vat restCompletely inelastic⟹vf = m₁ v/(m₁ + m₂), moving together
One-dimensional collisions: elastic (equal masses exchange velocities) and completely inelastic (bodies move together).

Two dimensions

  • Momentum conservation gives two equations: m₁v₁ᵢ = m₁v₁f cos θ₁ + m₂v₂f cos θ₂ and 0 = m₁v₁f sin θ₁ − m₂v₂f sin θ₂. With four unknowns (v₁f, v₂f, θ₁, θ₂) and an elastic energy equation, one more quantity (such as θ₁) must be known.
  • Example 5.12: two equal billiard balls, one at rest, collide elastically and obliquely: after the collision they move at right angles (θ₁ + θ₂ = 90°). For θ₂ = 37°, θ₁ = 53°.
  • Scattering: when the bodies act on each other at a distance (a comet near the sun, an alpha particle near a nucleus), the final velocities also depend on the type of interaction.
PonderPoints to ponderCommon confusions

Remember

  • Work is always done by a specific force (or group of forces) on a body over a displacement.
  • Work can be negative; kinetic energy and mass cannot.
  • The two forces of a third-law pair sum to zero, but the sum of the work they do need not be zero.
  • The work-energy theorem is the scalar form of the second law; it also holds in all inertial frames. Conservation of mechanical energy follows for conservative forces.
  • Potential energy is defined only up to a constant, and only for conservative forces (none for friction).
  • During a collision, momentum is conserved at each instant; kinetic energy (if the collision is elastic) is conserved only before and after contact.
Quick referenceFormulas at a glanceRevise before the exam

Key results

  • W = F · d = F d cos θ; W = ∫ F dx; K = ½mv² = p²/2m; Kf − Ki = W
  • V = mgh; V = ½kx²; F = −dV/dx; K + V = const; Ef − Eᵢ = Wnc
  • P = W/t; P = F · v; 1 kWh = 3.6 × 10⁶ J; 1 hp = 746 W
  • Elastic (m₂ at rest): v₁f = (m₁ − m₂)v₁ᵢ/(m₁ + m₂), v₂f = 2m₁v₁ᵢ/(m₁ + m₂); inelastic: vf = m₁v₁ᵢ/(m₁ + m₂)

Common mistakes

  • Using W = F d when the force is not along the displacement (forgetting cos θ).
  • Treating kWh as a unit of power.
  • Applying conservation of mechanical energy when friction acts.
  • Saying kinetic energy is conserved in every collision.
  • Forgetting the sign of the work done by friction or by a spring.