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) | Work | Physical meaning |
|---|
| 0° ≤ θ < 90° | Positive | Force component aids the motion (e.g. pushing a sled forward). |
| θ = 90° | Zero | Force perpendicular to displacement (e.g. centripetal force, normal reaction on a frictionless incline). |
| 90° < θ ≤ 180° | Negative | Force 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)
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
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)
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.
- Identify: \(F = 20\text{ N},\; s = 3\text{ m},\; \theta = 0^{\circ}\).
- Calculate: \(W = Fs\cos\theta = (20)(3)(1) = 60\text{ J}\).
- 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.
- Work by the pulling force: \(W_{\text{pull}} = Fs = (15)(4) = 60\text{ J}\).
- Vertical rise: \(h = 4\sin30^{\circ}=2\text{ m}\).
- Work done by gravity (negative): \(W_{g}= -mgh = -(2)(9.81)(2) = -39.2\text{ J}\).
- 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
- Calculate the work done by a 10 N force acting at 60° to the horizontal when an object moves 5 m horizontally.
- 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.
- Explain why the work done by the normal reaction force on a block sliding down a frictionless incline is zero.
- 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.
- 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.
- Determine the electrical work required to move a charge of 5 µC through a potential difference of 250 V.
- 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.
- 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.
- 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
| Concept | Formula | Key Points | Typical 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.