OCR A Physics Paper 3 Prep

A focused guide to the big gaps from Papers 1 and 2. Use this to decide what to revise before Unified Physics.

Read this first: this is not a guaranteed prediction list. Paper 3 can assess anything from the whole A Level course. The best use of this guide is to prioritise topics that were missing or light in Papers 1 and 2, then practise mixed questions.

Highest priority revision areas

Start here if you are short on time. These are the areas that feel most likely to be useful for Paper 3 because they were absent, light, or easy to combine with other topics.

Module 5

Simple harmonic motion

Know the definitions, the graphs and the energy changes. Be ready for displacement, velocity and acceleration graphs, plus damping and resonance.

Module 6

Capacitors and exponential decay

Practise charging and discharging graphs, time constant, and using natural logs to turn an exponential graph into a straight line.

Module 6

Electromagnetic induction

Faraday's law, Lenz's law, flux linkage, generators and transformers are all strong candidates for structured calculation questions.

Module 4

Quantum physics

Revise photons, photoelectric effect, stopping potentials, work function, threshold frequency, electron diffraction and de Broglie wavelength.

Module 5

Thermal physics

Brownian motion, specific heat capacity, specific latent heat, ideal gases and Maxwell-Boltzmann distributions are all worth a careful look.

Module 6

Nuclear and medical physics

Half-life, carbon dating, binding energy, fission, fusion, X-ray attenuation, CAT scans and PET scans could easily appear in Paper 3.

Paper 1 gaps to revise

These are mainly from forces, materials, momentum, thermal physics, circular motion and oscillations.

Motion

SUVAT and projectiles

  • Constant acceleration equations.
  • Horizontal and vertical motion treated separately.
  • Projectile questions where one direction has constant velocity and the other has acceleration.
  • Graph skills: gradient and area under velocity-time graphs.
Forces

Drag and terminal velocity

  • Why drag increases with speed.
  • Falling objects with weight, drag and resultant force.
  • Terminal velocity when resultant force is zero.
  • Fluid contexts such as a ball bearing falling through oil.
Materials

Material properties

  • Hooke's law and force-extension graphs.
  • Area under force-extension graphs as work done.
  • Stress, strain, Young modulus and ultimate tensile strength.
  • Ductile, brittle and polymeric materials.
  • Elastic and plastic deformation.
Momentum

Impulse and collisions

  • Momentum as a vector quantity.
  • Force as rate of change of momentum.
  • Impulse as FΔt.
  • Area under a force-time graph.
  • Conservation of momentum in one and two dimensions.
  • Elastic and inelastic collisions.
Thermal

Brownian motion and kinetic theory

  • Brownian motion as evidence for particles moving randomly.
  • Smoke particles being hit by air molecules.
  • Gas pressure explained by molecular collisions with container walls.
  • Links between temperature and molecular kinetic energy.
Thermal

Specific heat and latent heat

  • E = mcΔθ for specific heat capacity.
  • E = mL for specific latent heat.
  • Electrical practical methods.
  • Why temperature stays constant during a change of state.
  • Uncertainty, insulation and energy loss evaluation points.
Gases

Ideal gases and distributions

  • Assumptions of the kinetic model.
  • pV = nRT and pV = NkT.
  • Maxwell-Boltzmann distribution shape.
  • Root mean square speed.
  • How temperature changes the distribution.
Circular

Circular motion

  • Radians, angular velocity and period.
  • v = rω.
  • a = v²/r = rω².
  • F = mv²/r = mrω².
  • Banked turns, aircraft in horizontal circles, vertical loops and where the force is greatest.
SHM

Simple harmonic motion

  • SHM condition: acceleration is proportional to displacement and in the opposite direction.
  • a = -ω²x.
  • x = A cos(ωt) or x = A sin(ωt).
  • vmax = ωA.
  • Displacement, velocity and acceleration graphs.
  • Energy graphs and exchange between kinetic and potential energy.
SHM

Damping and resonance

  • Free oscillations compared with forced oscillations.
  • Natural frequency.
  • Resonance when driving frequency equals natural frequency.
  • Amplitude-frequency graphs.
  • Effect of damping on the resonance peak.

Paper 2 gaps to revise

These are mainly from electricity, waves, quantum physics, capacitors, electromagnetism, nuclear physics and medical imaging.

Electricity

Mean drift velocity

  • Current as moving charge.
  • I = Anev.
  • What each symbol means.
  • Why drift velocity is usually small even when the circuit responds quickly.
  • Conductors, semiconductors and insulators in terms of charge carrier density.
Electricity

Resistivity and power

  • R = ρL/A.
  • Resistivity practical for a metal wire.
  • Temperature effects in metals and semiconductors.
  • Electrical power: P = IV, P = I²R, P = V²/R.
  • Energy transfer: W = VIt.
Waves

Intensity and interference

  • Intensity as power per unit area.
  • Intensity is proportional to amplitude squared.
  • Inverse square behaviour when radiation spreads out from a point source.
  • Superposition, coherence and phase difference.
  • Constructive and destructive interference.
Waves

Young double slit

  • Use λ = ax/D.
  • Know what fringe spacing, slit separation and screen distance mean.
  • Be ready to explain why the pattern is evidence for the wave nature of light.
  • Compare double slit with diffraction grating style questions.
Quantum

Photons and photoelectric effect

  • Photon energy: E = hf and E = hc/λ.
  • Electronvolt conversions.
  • Work function and threshold frequency.
  • Einstein equation: hf = Φ + KEmax.
  • Stopping potential and maximum kinetic energy.
  • Gold-leaf electroscope and zinc plate explanation.
Quantum

Electron diffraction and de Broglie

  • Electrons showing wave-like behaviour.
  • Diffraction through thin polycrystalline graphite.
  • de Broglie wavelength: λ = h/p.
  • Higher momentum means shorter wavelength.
Capacitors

Capacitor circuits

  • Capacitance: C = Q/V.
  • Capacitors in series and parallel.
  • Charging and discharging through a resistor.
  • Time constant: τ = CR.
  • Energy stored: W = 1/2 QV, W = 1/2 CV².
Capacitors

Exponential graphs

  • Equations like x = x0e-t/CR.
  • Linearise by taking natural logs.
  • For discharge, plot ln V against t.
  • The gradient is negative and linked to 1/CR.
  • This skill also links to radioactive decay and X-ray attenuation.
Fields

Parallel-plate capacitors

  • C = ε0A/d.
  • Increasing area increases capacitance.
  • Increasing plate separation decreases capacitance.
  • Adding a dielectric increases capacitance.
Induction

Faraday, Lenz and generators

  • Magnetic flux: Φ = BA cosθ.
  • Flux linkage: .
  • Induced e.m.f. depends on rate of change of flux linkage.
  • Lenz's law gives the direction of the induced e.m.f.
  • Simple a.c. generators and transformers.
Particles

Particle classification and decay

  • Hadrons, leptons and quarks.
  • Proton and neutron quark composition.
  • Beta minus and beta plus decay.
  • Conservation of charge, baryon number and lepton number.
  • Do not forget the neutrino or antineutrino.
Nuclear

Nuclear radius and density

  • Alpha scattering and the nuclear model.
  • Nuclear notation.
  • Radius equation: R = r0A1/3.
  • Nuclear density calculations using mass divided by volume.
Nuclear

Half-life and carbon dating

  • Decay is spontaneous and random.
  • Activity: A = λN.
  • Half-life and λt1/2 = ln2.
  • Decay equations: A = A0e-λt and N = N0e-λt.
  • Carbon dating could appear as a longer written explanation with calculations.
Nuclear

Binding energy, fission and fusion

  • Mass defect and E = Δmc².
  • Binding energy per nucleon.
  • Energy released from fission and fusion.
  • Balanced nuclear equations.
  • Chain reactions and reactor components.
Medical

X-rays, CAT and PET

  • X-ray tube and production of X-ray photons.
  • Attenuation equation: I = I0e-μx.
  • Contrast media.
  • CAT scanner advantages over a single X-ray image.
  • Medical tracers, gamma camera and PET scans.

Cross-topic combinations to practise

Paper 3 likes to mix ideas. The aim is not just to know topics separately, but to spot links between topics.

Big synoptic focus

Generators and simple harmonic motion

This is a very sensible Paper 3 style combination because both topics involve sinusoidal motion or sinusoidal variation.

  1. Start with rotation. A coil rotates in a magnetic field. The angle between the coil and the field changes continuously.
  2. Flux changes with angle. Magnetic flux can be written as Φ = BA cosθ. For a rotating coil, the angle changes with time, so the flux changes with time.
  3. Induced e.m.f. depends on rate of change. Faraday's law says the induced e.m.f. depends on how quickly the flux linkage changes.
  4. This gives an alternating output. The e.m.f. changes direction every half-turn, so the generator produces an alternating e.m.f.
  5. The maths looks like SHM. In SHM, displacement often varies as x = A cos(ωt) or x = A sin(ωt). In a generator, flux and e.m.f. also vary sinusoidally.
  6. Maximum values happen at different points. Flux is maximum when the coil is aligned so the field passes through the largest effective area. The induced e.m.f. is maximum when the flux is changing fastest.
Likely skill: explain the shape of an e.m.f.-time graph and link it to the rotating coil.
Likely calculation: use angular frequency, period or frequency to connect rotation rate with the output waveform.
Likely trap: saying maximum flux means maximum induced e.m.f. It does not. Maximum induced e.m.f. happens when the rate of change of flux is greatest.
Graphs

Exponential decay everywhere

Capacitor discharge, radioactive decay and X-ray attenuation all use the same mathematical shape. Practise plotting natural log graphs to get a straight line and using the gradient.

Thermal plus mechanics

Brownian motion and collisions

Brownian motion links kinetic theory to momentum ideas. The random motion comes from many uneven molecular collisions with tiny visible particles.

Waves plus quantum

Wave-particle evidence

Young double slit supports the wave model of light. Photoelectric effect supports the photon model. Electron diffraction supports the wave nature of particles.

Nuclear

Binding energy and decay

Be ready to combine nuclear equations, mass defect, binding energy per nucleon, fission, fusion and energy release in one messy question.

How to revise this efficiently

1
Do not just read notes. For each topic, do one calculation question and one written explanation.
2
Practise graphs. Paper 3 often rewards pupils who can explain gradients, areas, intercepts and log-linear graphs.
3
Practise practical evaluation. Know the method, safety, uncertainties, improvements and sources of error for the main practicals.
4
Mix topics. Do not revise each chapter as if it lives alone. Paper 3 is called Unified Physics for a reason.

Best quick plan: 25 minutes on SHM and generators, 25 minutes on capacitor decay, 25 minutes on quantum, then 25 minutes on nuclear or medical exponential decay.