understand the concept of work, and recall and use work done = force × displacement in the direction of the force

Work, Energy and Power – Cambridge IGCSE / A‑Level Physics (9702)

Learning Objectives

  • Define work and explain its role as an energy‑transfer process.
  • Apply the work‑formula W = F s cosθ for constant forces and for forces that vary with displacement.
  • State and use the work‑energy theorem in its most general form.
  • Derive and use the expressions for kinetic energy, gravitational potential energy (near‑Earth and in a field), elastic (spring) potential energy, electric potential energy and magnetic energy.
  • Calculate power and efficiency for a range of mechanical, electrical and thermal processes.
  • Relate work to the first law of thermodynamics and to energy changes in simple harmonic motion.
  • Identify and evaluate work in deformation of solids, electrical circuits, magnetic systems and nuclear reactions.
  • Plan, carry out and evaluate simple experiments that measure work, energy or power (AO2/AO3).

1. Work – Definition and General Formula

Work is the transfer of energy that occurs when a force (or a set of forces) acts through a displacement.

\(W = \int \vec F \cdot d\vec s = F s \cos\theta\) (for a constant force)

  • Scalar quantity – only its sign (positive, negative or zero) indicates the direction of energy transfer.
  • SI unit: 1 J = 1 N·m = kg·m²·s⁻².

1.1 Sign of Work

Angle θ (between F and s)WorkPhysical meaning
0° ≤ θ < 90°PositiveForce component aids the motion (e.g. pushing a sled forward).
θ = 90°ZeroForce perpendicular to displacement (e.g. centripetal force, normal reaction on a frictionless incline).
90° < θ ≤ 180°NegativeForce opposes the motion (e.g. friction, braking, gravity when an object descends).

2. Work‑Energy Theorem (most general form)

The net work done on a system equals the total change in its mechanical energy, plus any change in internal energy caused by non‑conservative forces.

\(W{\text{net}} = \Delta K + \Delta U{\text{nc}} = \Delta E{\text{mech}} + \Delta U{\text{int}}\)

For a particle acted on only by conservative forces, \(W_{\text{net}} = \Delta K\) and the mechanical energy \(K+U\) is conserved.

3. Forms of Energy and Associated Work

3.1 Kinetic Energy (KE)

\(K = \tfrac12 m v^{2}\)

  • Derived directly from the work‑energy theorem for a constant net force.
  • Always positive; zero only when the object is at rest.

3.2 Gravitational Potential Energy (GPE)

  • Near‑Earth approximation (uniform field):
    \(U_{g}=m g h\)
  • General field (point mass M):
    \(U = -\dfrac{G M m}{r}\)
  • Zero of potential may be chosen arbitrarily; the change in U is what matters.

3.3 Elastic (Spring) Potential Energy

\(U_{s}= \tfrac12 k x^{2}\quad\text{(Hooke’s‑law spring)}\)

  • Valid only while the spring obeys \(F = kx\).
  • Energy is released when the spring returns to its natural length.

3.4 Work in Deformation of Solids (Stress ↔ Strain)

For a material that obeys Hooke’s law in tension or compression, the work done in producing a strain ε is stored as elastic energy.

\(W = \int \sigma \, d\varepsilon \; V = \tfrac12 \sigma \varepsilon V\)

  • \(\sigma\) = stress (N m⁻²), \(\varepsilon\) = strain (dimensionless), \(V\) = volume of the element.
  • Useful for questions on stretching a wire, compressing a column or energy stored in a rubber band.

3.5 Electrical Work and Potential Energy

  • Work done by an electrostatic force moving a charge q through a potential difference V:

    \(W = q V\)

  • Electric potential energy of a system of point charges:

    \(U = \dfrac{1}{4\pi\varepsilon{0}} \dfrac{q{1}q_{2}}{r}\)

  • In circuits, the energy supplied by a source of emf E over a time t at current I:

    \(W = E I t\)

3.6 Magnetic Work and Energy

  • Force on a moving charge in a magnetic field: \(\vec F = q\vec v \times \vec B\).

    Work is zero because \(\vec F\) is always perpendicular to \(\vec v\) (\(\theta = 90^{\circ}\)).

  • Energy stored in an inductor (magnetic field):

    \(U_{L}= \tfrac12 L I^{2}\)

  • Work required to move a magnetic dipole \(\vec \mu\) through a change in magnetic field:

    \(W = -\int \vec \mu \cdot d\vec B\)

3.7 Nuclear Energy (mass–energy equivalence)

Energy released in a nuclear reaction is given by Einstein’s relation:

\(E = \Delta m\,c^{2}\)

  • \(\Delta m\) = loss of mass, \(c = 3.00\times10^{8}\,\text{m s}^{-1}\).
  • Often presented as a real‑world application of the work‑energy idea (energy released = work done by the strong nuclear force).

4. Power and Efficiency

  • Power – rate of doing work or transferring energy:

    \(P = \dfrac{W}{t}=Fv = \dfrac{\Delta E}{\Delta t}\)

    Units: 1 W = 1 J s⁻¹.

  • Efficiency – useful output as a percentage of input:

    \(\eta = \dfrac{W{\text{useful}}}{W{\text{input}}}\times100\%\)

    Accounts for non‑conservative losses (friction, heat, electrical resistance, radiation).

5. First Law of Thermodynamics

\(\Delta U = Q + W\)

  • \(Q\) = net heat added to the system (positive if added).
  • \(W\) = net work done *on* the system (positive if done on the system, negative if done by the system).
  • When only work is involved (e.g. adiabatic compression of an insulated gas), \(\Delta U = W\).
  • In isothermal processes for an ideal gas, \(\Delta U = 0\) so \(Q = -W\).

6. Connections to Other Syllabus Areas

6.1 Ideal Gases (Topic 15)

\(W = -\int{Vi}^{V_f} P\,dV\)

  • Isothermal expansion: \(W = nRT\ln\left(\dfrac{Vf}{Vi}\right)\).
  • Adiabatic expansion: \(W = \dfrac{PiVi-PfVf}{\gamma-1}\) where \(\gamma = Cp/Cv\).

6.2 Thermodynamics (Topic 16)

  • Specific heat: \(Q = mc\Delta T\).
  • Latent heat: \(Q = mL\).
  • These expressions are frequently combined with the first law when analysing engines, refrigerators or calorimetry experiments.

6.3 Oscillations and Waves (Topics 17‑18)

  • For a simple harmonic oscillator:

    \(E{\text{total}} = \tfrac12 kA^{2}=K{\max}=U_{\max}\)

  • Energy in a standing wave is distributed between kinetic energy of the medium and potential energy of the deformation; the total energy is constant (ignoring damping).

6.4 Electricity and Magnetism (Topics 19‑21)

  • Electrical work in moving charges, energy stored in capacitors (\(U{C}= \tfrac12 C V^{2}\)) and inductors (\(U{L}= \tfrac12 L I^{2}\)).
  • Magnetic work is zero for a charge moving in a uniform \(\vec B\) field, but energy is stored in magnetic fields of coils and solenoids.

6.5 Nuclear and Medical Physics (Topics 23‑24)

  • Energy released in fission or fusion reactions calculated via \(E=\Delta m c^{2}\).
  • Applications: PET scanners, radiotherapy – illustrate the link between mass loss and usable work/energy.

7. Practical / Experimental Skills (AO2/AO3)

  • Measuring mechanical work: Use a dynamometer to record force and a metre rule or motion sensor for displacement; calculate \(W = Fs\) (θ = 0°).
  • Elastic energy experiment: Stretch a spring, plot force versus extension, determine \(k\) from the slope, then compute \(U_{s}=½kx^{2}\).
  • Electrical work: Connect a resistor to a known voltage source, measure current with an ammeter and time with a stopwatch; compute \(W = V I t\).
  • Power of a lifting machine: Use a pulley system, measure effort force and distance, compare with load weight × height; calculate efficiency \(\eta\).
  • Thermodynamic work: Perform an isothermal expansion of a gas in a piston with a pressure sensor; integrate \(P\,dV\) numerically to obtain work.

8. Worked Examples

Example 1 – Horizontal Push (Mechanical Work)

A 5 kg crate is pushed across a frictionless floor by a constant horizontal force of 20 N over 3 m.

  1. Identify: \(F = 20\text{ N},\; s = 3\text{ m},\; \theta = 0^{\circ}\).
  2. Calculate: \(W = Fs\cos\theta = (20)(3)(1) = 60\text{ J}\).
  3. Result: 60 J of positive work is done on the crate.

Example 2 – Inclined Plane (Work against Gravity)

A 2 kg block is pulled up a smooth 30° incline by a 15 N force parallel to the plane. The block moves 4 m along the plane.

  1. Work by the pulling force: \(W_{\text{pull}} = Fs = (15)(4) = 60\text{ J}\).
  2. Vertical rise: \(h = 4\sin30^{\circ}=2\text{ m}\).
  3. Work done by gravity (negative): \(W_{g}= -mgh = -(2)(9.81)(2) = -39.2\text{ J}\).
  4. Net work: \(W_{\text{net}} = 60 - 39.2 = 20.8\text{ J}\) → increase in kinetic energy.

Example 3 – Spring Compression (Elastic PE)

A spring with \(k = 250\;\text{N m}^{-1}\) is compressed 0.12 m from its natural length.

\(U_{s}= \tfrac12 kx^{2}= \tfrac12 (250)(0.12)^{2}=1.8\text{ J}\)

Example 4 – Electrical Work (Charging a Capacitor)

A 10 µF capacitor is charged from 0 V to 12 V by a constant 12 V source.

\(W = \tfrac12 C V^{2}= \tfrac12 (10\times10^{-6})(12)^{2}=7.2\times10^{-4}\text{ J}\)

Example 5 – Magnetic Energy in an Inductor

An inductor of inductance \(L = 0.25\;\text{H}\) carries a current that rises uniformly to 3 A.

\(U_{L}= \tfrac12 L I^{2}= \tfrac12 (0.25)(3)^{2}=1.125\text{ J}\)

Example 6 – Nuclear Energy Release

In a fission reaction 1.0 g of \(\,^{235}\)U undergoes complete fission. Mass defect \(\Delta m = 0.001\text{ g}\).

\(E = \Delta m c^{2}= (1.0\times10^{-6}\text{ kg})(3.00\times10^{8}\text{ m s}^{-1})^{2}=9.0\times10^{10}\text{ J}\)

9. Practice Questions

  1. Calculate the work done by a 10 N force acting at 60° to the horizontal when an object moves 5 m horizontally.
  2. A 0.5 kg ball is thrown vertically upward with an initial speed of 8 m s⁻¹. Determine the work done by gravity when the ball reaches its highest point.
  3. Explain why the work done by the normal reaction force on a block sliding down a frictionless incline is zero.
  4. For an ideal gas expanding isothermally from 1.0 L to 3.0 L at 300 K, calculate the work done if the external pressure remains constant at \(1.0\times10^{5}\) Pa.
  5. A mass‑spring system oscillates with amplitude 0.10 m and spring constant 80 N m⁻¹. Find the maximum kinetic energy and the total mechanical energy.
  6. Determine the electrical work required to move a charge of 5 µC through a potential difference of 250 V.
  7. A steel wire of length 2 m, cross‑section 1 mm² and Young’s modulus \(2.0\times10^{11}\) N m⁻² is stretched by 1 mm. Calculate the work stored as elastic energy.
  8. Calculate the efficiency of a motor that lifts a 50 kg load through 5 m in 4 s while drawing 0.8 A from a 240 V supply.
  9. Using \(E=\Delta mc^{2}\), compute the energy released when 0.2 g of mass is converted entirely into energy.

10. Summary Table – Key Energy Concepts

ConceptFormulaKey PointsTypical Application
Work\(W = \vec F\!\cdot\!\vec s = Fs\cos\theta\)Only the component of F parallel to s does work; sign indicates energy transfer direction.Pushing a crate, lifting a weight, electrical work \(qV\).
Kinetic Energy\(K = \tfrac12 mv^{2}\)Derived from work‑energy theorem; always non‑negative.Finding speed after a force acts.
Gravitational PE (near‑Earth)\(U_{g}=mgh\)Reference level arbitrary; linear with height.Energy change of a lifted or falling object.
Gravitational PE (field)\(U = -\dfrac{GMm}{r}\)Applicable for satellites, planetary motion.Orbital energy calculations.
Elastic PE (spring)\(U_{s}= \tfrac12 kx^{2}\)Only for ideal Hooke’s‑law springs.Energy stored in a compressed/extended spring.
Elastic PE (solid deformation)\(W = \tfrac12 \sigma \varepsilon V\)Stress–strain work; useful for wires, bars.Stretching a metal wire, compressing a column.
Electric PE (point charges)\(U = \dfrac{1}{4\pi\varepsilon{0}}\dfrac{q{1}q_{2}}{r}\)Energy of a charge configuration.Capacitor energy, electrostatic problems.
Electrical Work\(W = qV = V I t\)Positive when charge moves with the field.Charging a capacitor, powering a motor.
Magnetic Energy (inductor)\(U_{L}= \tfrac12 L I^{2}\)Energy stored in a magnetic field.Coils in transformers, solenoids.
Power\(P = \dfrac{W}{t}=Fv=\dfrac{\Delta E}{\Delta t}\)Rate of energy transfer.Motor rating, athlete performance.
Efficiency\(\eta = \dfrac{W{\text{useful}}}{W{\text{input}}}\times100\%\)Accounts for losses (friction, heat, resistance).Evaluating engines, lifts, electrical devices.
First Law (Thermodynamics)\(\Delta U = Q + W\)Work and heat are interchangeable forms of energy.Gas compression, heating, cooling cycles.
Energy in SHM\(E{\text{total}} = \tfrac12 kA^{2}=K{\max}=U_{\max}\)Total mechanical energy constant (no damping).Mass‑spring oscillator, pendulum (small angles).
Nuclear Energy\(E = \Delta m\,c^{2}\)Mass defect converted to energy.Fission reactors, fusion, medical isotopes.

11. Key Take‑aways

  • Work quantifies energy transfer: W = F s cosθ. Only the component of force parallel to the displacement does work.
  • The most general work‑energy theorem is Wₙₑₜ = ΔK + ΔUₙ𝚌; for conservative forces it reduces to Δ(K+U)=0.
  • Kinetic, gravitational (both near‑Earth and field), elastic, electrical and magnetic energies are the main forms needed for the syllabus.
  • When only conservative forces act, total mechanical energy is conserved; otherwise include the work of non‑conservative forces or use the first law.
  • Power is the rate of doing work; efficiency measures how much of the input energy appears as useful output.
  • Work, heat and internal energy are unified by the first law of thermodynamics.
  • In simple harmonic motion, kinetic and elastic energies continuously interchange while the total remains constant.
  • Practical skills—measuring forces, distances, voltages, currents and times—are essential for experimental verification of the concepts.