Unit 2 in two days
What 20 WPH12 Waves and Electricity papers, from October 2019 to June 2026, say you should learn, in the order that earns marks fastest.
- It’s the same 17 question types every time. Each Section B uses 9 to 15 of them (usually 11 to 13), and the multiple-choice questions pick up most of the rest. Learn the standard answer to each and most of the paper will look familiar.
- Electricity and waves split most of the marks: about 30 each on average in the last four papers (electricity 25 to 40, waves 22 to 35), with photons and quantum taking 18 to 25.
- Four topics were in Section B of nearly every paper: circuit calculations (20 of 20), refraction and total internal reflection (19), the photoelectric effect (18) and resistivity (17).
- Most formulas are printed at the back of the paper. What you need is the few that aren’t, plus the explanation chains examiners mark. Both are below.
- Lenses and the Doppler effect never came up in any of the 20 papers and aren’t on the formula sheet. Skip them.
Your two days
Tick things off as you go; ticks are saved in this browser.
Day 1: learn (about 6 hours)
Day 2: practise (about 4½ hours)
Only have 3 hours? Electricity (60 min), then photoelectric effect, refraction and TIR, gratings and stationary waves (60 min), then 6-mark skeletons A, B, D and G (20 min), then Section B of January 2026 with the mark scheme open (40 min).
What’s likely in October 2026
This comes from how often each topic appeared and what June 2026 left out. Pearson doesn’t work to a fixed rota, so use it to decide what to learn first, not what to skip. The unit is small enough to cover all of it.
Almost certain in Section B
- Circuit calculations: series and parallel, power, energy (20 of 20 papers)
- Refraction, critical angle and TIR (19 of 20). The one paper without it was June 2026, so expect it back.
- Photoelectric effect (18 of 20)
- Resistivity, R = ρl/A (17 of 20, and every paper since October 2023)
- Stationary waves on a string or in a tube (16 of 20)
Very likely
- Diffraction grating calculation plus “explain the bright maxima”. Diffraction was in every paper from January 2024 to January 2026, then only an MCQ in June 2026.
- Thermistor or LDR potential divider (15 of 20)
- e.m.f. and internal resistance (15 of 20)
- de Broglie wavelength, usually of an accelerated electron (6 of the last 8)
- Intensity, efficiency and photons per second (6 of the last 8)
Skipped by June 2026’s Section B, so good odds of a comeback
- Superposition, path difference and coherence
- Polarisation
- Pulse-echo (ultrasound, sonar)
- Drift velocity, I = nqvA (an MCQ almost every time anyway)
Might shrink to an MCQ
Energy levels were a full question in June 2026. The calculation takes ten minutes to learn, so learn it anyway.
The 6-mark question
The last six were: TIR at a water surface (Oct 2024), an LDR with internal resistance (Jan 2025), a stationary wave in a tube (Jun 2025), a thermistor potential divider (Oct 2025), ultrasound finding a crack (Jan 2026) and cells in series vs parallel (Jun 2026).
Overdue: the photoelectric effect (last a 6-marker in October 2023), two-source interference (January 2024), line spectra (June 2024) and filament vs thermistor graphs (January 2021). My two picks are the photoelectric effect and two-source interference. All ten skeletons are in the 6-mark bank and they’re short, so learn every one.
Where the marks came from
One column per paper. Red means the topic had at least one part-question in Section B. The shaded column is June 2026, the paper just before yours. Tap a topic to jump to its notes. On a phone, swipe the table sideways.
| Topic |
|---|
Electricity
Usually 25 to 40 of the 80 marks, and its topics are the most predictable, so it comes first. Plain formulas are printed on the formula sheet; highlighted ones aren’t, so learn those.
Series, parallel, power and energy
- V = W/Q
- I = ΔQ/Δt
- R = V/I
- P = VI = I2R = V2/R
- W = VIt
- R = R1 + R2 + …
- 1/R = 1/R1 + 1/R2 + …
- N = It/e
- 1 kWh = 3.6 × 106 J
Know cold
- Series: the same current everywhere, and the p.d.s add up to the supply.
- Parallel: the same p.d. across every branch, and the branch currents add up. Two in parallel give R1R2/(R1 + R2), always less than the smallest one.
- For “the power in one resistor”, first find the current through that resistor only (or the p.d. across it).
- Number of electrons = charge ÷ 1.60 × 10−19 C.
- Derivations they’ve asked for: the parallel formula (same V, currents add, so V/R = V/R1 + V/R2) and P = V2/R (put I = V/R into P = VI).
- “Assess whether both lamps work normally”: work out the actual p.d. or current for each lamp and compare it with its rating.
Try: June 2025 Q16, January 2026 Q15 and Q16, June 2026 Q11 and Q12.
Resistivity
- R = ρl/A
- A = πd2/4
Know cold
- Resistivity is RA/l: the resistance of a piece of the material 1 m long with a 1 m2 cross-section. Unit Ω m. It depends on the material (and temperature), not the shape.
- Practical: measure the diameter with a micrometer at several points, rotating it, and average. Length with a metre rule. Ammeter in series, voltmeter across the wire (or an ohmmeter). Change the length with a crocodile clip and plot R against l: the gradient is ρ/A, so ρ = gradient × A. Keep the current small and switch off between readings so the wire doesn’t heat up.
- Same material: R ∝ l/d2. Stretch a wire to twice the length at constant volume and its area halves, so R goes up four times.
- Traps: convert mm to m before squaring (mm2 × 10−6 = m2), and don’t use the diameter as the radius.
Try: June 2026 Q17, October 2025 Q13 (the practical), October 2024 Q15.
Potential dividers with thermistors and LDRs
- Vout = Vin × R/Rtotal
- V1/V2 = R1/R2
Know cold
- Parts in series carry the same current, so they share the supply p.d. in the ratio of their resistances.
- Bigger resistance, bigger share. When a thermistor warms (or an LDR gets more light) its resistance falls, so the p.d. across it falls and the fixed resistor’s p.d. rises by the same amount.
- “Deduce whether the heater switches on”: read R off the graph, work out the p.d. across whichever component the output is taken from, compare it with the switching value, conclude.
- A voltmeter that isn’t very high-resistance lowers the resistance of the part it’s connected across, so it reads low.
- Along a uniform wire the p.d. is proportional to the length: V = Vtotal × x/l.
Try: October 2025 Q17, June 2026 Q14, October 2023 Q14.
e.m.f. and internal resistance
- ε = I(R + r)
- V = ε − Ir
Know cold
- e.m.f. is the energy transferred to each unit of charge by the source (chemical to electrical). “An e.m.f. of 6.0 V” means 6.0 J for every coulomb.
- p.d. is the energy transferred from each unit of charge by a component.
- When current flows, the terminal p.d. is less than ε because some energy per coulomb is transferred in the internal resistance. Those “lost volts” are Ir.
- A high-resistance voltmeter across a cell with nothing else connected reads ε: the current is almost zero, so Ir is almost zero.
- Bigger external R, smaller current, fewer lost volts, so the terminal p.d. gets closer to ε. Maximum current is ε/r.
- A battery heats up under heavy load because a large current dissipates I2r inside it. An old battery has a bigger r, so more lost volts and too little p.d. for a high-current motor.
- Cells in series: ε and r both add. Identical cells in parallel: the same ε, with r divided by the number of cells.
- Practical: cell, ammeter and variable resistor in series, voltmeter across the cell. Vary R, record V and I, plot V against I: the y-intercept is ε and the gradient is −r. If they make you plot R against 1/I, the gradient is ε and the intercept is −r. A straight line means r is constant.
Try: January 2026 Q13, June 2026 Q15, January 2024 Q14.
Charge, current and drift velocity
- I = nqvA
- I = ΔQ/Δt
Know cold
- n is the number of charge carriers per m3, q = 1.60 × 10−19 C, v is the drift velocity and A the cross-sectional area.
- Drift velocity in a metal is tiny because n is enormous (about 1028 to 1029 per m3).
- Same current through two wires in series: v ∝ 1/(nA). Double the diameter, four times the area, a quarter of the drift velocity.
- Copper vs nichrome of the same size carrying the same current: nichrome has fewer conduction electrons per m3, so its electrons drift faster.
- Semiconductors have far smaller n than metals, which is why their resistivity is so much higher.
Try: January 2026 Q11, October 2025 Q11, January 2023 Q13.
Why resistance changes, and I–V graphs
The chains examiners mark
- Metal or filament getting hotter: the ions vibrate more, conduction electrons collide with them more often, the current (drift velocity) falls for the same p.d., so R = V/I rises. The number of conduction electrons stays about the same.
- NTC thermistor getting hotter: electrons gain energy and more conduction electrons are released (n rises). This outweighs the extra vibration, so the current rises for the same p.d. (I = nqvA) and R falls.
- LDR in brighter light: absorbed photons release more conduction electrons, n rises, R falls.
- I–V shapes: a resistor is a straight line through the origin. A filament lamp is an S-curve bending towards the V-axis. A thermistor curves towards the I-axis as it heats. A diode passes almost no current until about 0.6–0.7 V forward, and none in reverse.
Try: January 2026 Q12, October 2025 Q12(b), January 2021 Q16.
Photons and quantum
About 18 to 25 marks, and the most formulaic part of the paper.
Photoelectric effect
- E = hf
- v = fλ (c = fλ)
- hf = φ + ½mv2max
- 1 eV = 1.60 × 10−19 J
- f0 = φ/h
Know cold
- Work function φ: the minimum energy needed to release an electron from the surface of the metal. Threshold frequency f0: the lowest frequency that releases electrons, f0 = φ/h.
- The calculation chain: λ, then f = c/λ, then E = hf, then Ek(max) = hf − φ, then v = √(2Ek/m). Keep everything in joules, or everything in eV.
- Brighter light at the same frequency (above f0): more photons per second, more electrons per second, a bigger current. Ek(max) doesn’t change.
- Longer wavelength: lower frequency, less energy per photon, lower Ek(max). Below f0 nothing comes out, however bright.
- Why the electrons have a range of kinetic energies: φ is only the minimum. Electrons from deeper in the metal lose energy in collisions on the way out.
- Graph of Ek(max) against f: the gradient is h, the x-intercept is f0 and the y-intercept is −φ.
- “Why this proves light is photons” is skeleton A in the 6-mark bank.
Try: October 2025 Q15, January 2026 Q21, June 2026 Q19.
Intensity, efficiency and photons per second
- I = P/A
- efficiency = useful power out ÷ total power in
- A = 4πr2 (point source)
- photons per second = P/(hf)
Know cold
- Intensity is power per unit area (W m−2). From a point source it follows the inverse square law: twice the distance, a quarter of the intensity.
- Solar panel: power in = intensity × area, and efficiency = electrical power out ÷ power in.
- Photons per second = power ÷ energy of one photon = Pλ/(hc). Electrons per second = current ÷ e. Percentage of photons that release electrons = electrons per second ÷ photons per second × 100.
Try: June 2025 Q18, June 2026 Q18(a), January 2021 Q20.
de Broglie and electron diffraction
- λ = h/p
- p = mv
- Ek = ½mv2
- Ek = eV (electron accelerated through V volts)
Know cold
- Electron diffraction, a ring pattern from graphite or a thin metal foil, is the evidence that electrons behave as waves, because diffraction is a wave property. It shows up because the electrons’ wavelength is similar to the spacing between atoms (about 10−10 m).
- Raise the accelerating p.d. and the electrons go faster, with more momentum, so a shorter wavelength, less diffraction and smaller rings.
- Accelerated electron: Ek = eV in joules, then v = √(2Ek/m), then λ = h/(mv).
- Everyday objects like a car have a wavelength far too small to ever diffract.
Try: January 2026 Q14, June 2025 Q15, October 2023 Q15.
Energy levels and line spectra
- E = hf
- hf = E1 − E2
- λ = hc/ΔE
Know cold
- Levels are negative. 0 eV means the electron has left the atom (ionised), and the most negative level is the ground state.
- Calculation: the gap in eV × 1.60 × 10−19 gives joules, then f = ΔE/h, then λ = c/f.
- A photon is absorbed only if its energy exactly matches a gap: all or nothing, otherwise the atom stays as it was. A colliding electron can hand over part of its energy and keep the rest.
- Discrete levels mean only certain gaps, so only certain frequencies: a line spectrum. Different elements have different levels, so different spectra.
- Number of possible lines from level n down to the ground state: n(n − 1)/2. Also an MCQ in almost every paper where it isn’t in Section B.
Try: June 2026 Q13, June 2024 Q17, October 2021 Q16.
Waves
About 22 to 35 marks. June 2026 went light on these, so they’re the likeliest to be heavy in October.
Refraction, critical angle and TIR
- n = c/v
- n1 sin θ1 = n2 sin θ2
- sin C = 1/n
- sin C = n2/n1 (between two materials)
Know cold
- Refraction is a change in direction when a wave crosses into a medium where its speed is different. The frequency stays the same; speed and wavelength change.
- Slowing down bends the ray towards the normal, speeding up bends it away. Along the normal there’s no change in direction, because the whole wavefront slows at the same moment.
- TIR needs both: travelling from higher n to lower n, and an angle of incidence bigger than C. At exactly C the refracted ray runs along the boundary. Below C, part reflects and part refracts.
- “Deduce whether TIR happens”: work out C, get the angle of incidence from the geometry (angles in a triangle add to 180°), compare, conclude.
- Useful values: glass (n = 1.5) has C ≈ 42°, water (n = 1.33) has C ≈ 49°.
- Optical fibre: the cladding has a lower n than the core. It makes C bigger than a core-to-air boundary would, but protects the core. A lower-n cladding gives a smaller C, so more light is trapped. Pulses spread out because rays take paths of different lengths.
- Measuring n: ray box and glass block, measure i and r at several angles, plot sin i against sin r, and the gradient is n.
- Two materials with similar n (a bead in water, skin on glass) barely refract or reflect at the boundary, so the edge “disappears” and TIR stops where they touch.
Try: January 2026 Q20, October 2025 Q14, October 2024 Q17.
Stationary waves: strings and tubes
- v = √(T/μ)
- v = fλ
- W = mg
- node to node = λ/2
- string: λ = 2L
- closed tube: L = λ/4
Know cold
- How it forms (the 3-mark version): the wave reflects at the end, the incident and reflected waves (same frequency and amplitude) travel in opposite directions and superpose, giving nodes where they always cancel and antinodes where they reinforce. The 6-mark version is skeleton D.
- String fixed at both ends: fundamental λ = 2L. Tube closed at one end: a node at the closed end and an antinode at the open end, fundamental L = λ/4. Tube open at both ends: L = λ/2.
- Combine the formulas: f = (1/2L)√(T/μ), so f ∝ √T, f ∝ 1/L and f ∝ 1/√μ. A graph of f2 against T is a straight line through the origin with gradient 1/(4L2μ). A graph of node spacing against 1/f has gradient v/2.
- μ is mass per unit length (kg m−1). Tension from a hanging mass is mg, with g = 9.81.
- Points between two neighbouring nodes are in phase; points in neighbouring loops are in antiphase. Amplitude varies with position.
- Stationary vs progressive: stationary has no net energy transfer, has nodes and antinodes, and the same phase within a loop. Progressive transfers energy, has the same amplitude everywhere, and its phase changes along the wave.
- Practical: vibration generator, string over a pulley with hanging masses. Change f until the pattern is clear. Node positions are hard to judge, so measure across several loops.
Try: June 2026 Q16, June 2025 Q17, October 2024 Q18.
Diffraction and gratings
- nλ = d sin θ
- d = 1/N (N = lines per metre)
- tan θ = x/D
Know cold
- Diffraction is waves spreading out as they pass through a gap or around an obstacle. It’s biggest when the gap is about one wavelength wide.
- Huygens’ construction: every point on a wavefront acts as a source of secondary wavelets, and the new wavefront is the line touching all of them.
- Lines per mm × 1000 = lines per m, and d = 1 ÷ that. x is the distance from the central maximum to the maximum, D the grating-to-screen distance.
- Highest possible order: n ≤ d/λ, rounded down, because sin θ can’t be more than 1. That’s also why a third order can be impossible.
- Why there’s a bright maximum: light diffracts at each slit, waves from neighbouring slits superpose, and at the maximum the path difference is a whole number of wavelengths, so they arrive in phase and interfere constructively.
- White light: a white central maximum (every colour has zero path difference there), then spectra with violet nearest the centre and red furthest out, because shorter λ gives smaller θ.
- Practical: don’t look into the laser and avoid reflections. Measure between the first orders on both sides and halve it, and use a large grating-to-screen distance to cut the percentage uncertainty.
Try: January 2026 Q17, October 2025 Q16, October 2024 Q16.
Superposition, interference and coherence
- phase difference = (path difference ÷ λ) × 360°
Know cold
- Superposition: where waves meet, the resultant displacement is the sum of their individual displacements.
- Coherent: the same frequency and a constant phase difference. Two separate lamps aren’t coherent, so they can’t give a steady pattern.
- Constructive: in phase, path difference nλ, maximum amplitude (loud, bright).
- Destructive: antiphase (180°, π rad), path difference (n + ½)λ, minimum amplitude (quiet, dark).
- Quiet spots aren’t totally silent because the two waves arrive with different amplitudes.
- Beats: two slightly different frequencies aren’t coherent, so the phase difference keeps changing and the loudness rises and falls.
- Noise-cancelling: send out sound in antiphase so it interferes destructively.
Try: January 2023 Q15, January 2024 Q17, October 2022 Q15.
Wave basics and graphs
- v = fλ
- f = 1/T
Know cold
- Transverse: oscillations perpendicular to the direction the wave travels (light, waves on a string). Longitudinal: oscillations parallel to it (sound). Compressions have high pressure and density, rarefactions low. The displacement is zero at the centre of each.
- A displacement–distance graph gives λ and amplitude. A displacement–time graph gives the period and amplitude, never λ.
- Oscilloscope: period = number of divisions × time-base. Measure across several cycles.
- Speed of sound practical: the signal generator drives the loudspeaker and one oscilloscope trace, the microphone gives the other trace. Move the microphone until the traces are back in phase: that distance is one λ (measure across several). Then v = fλ, or plot λ against 1/f and the gradient is v.
Try: June 2021 Q17 (the speed of sound practical), June 2024 Q15, October 2025 Q2 to Q5.
Polarisation
Know cold
- Unpolarised: oscillations in all planes (every direction perpendicular to the direction of travel). Plane polarised: oscillations in one plane only. That’s the 3-mark “explain the difference” answer.
- Only transverse waves can be polarised, which is how we know light is transverse and why sound can’t be polarised.
- Test: look through one filter and rotate it. Unpolarised light: no change in brightness. Plane-polarised light: brightness goes from maximum to zero every 90°.
- Two filters: bright when lined up, dark at 90°. Three filters with the outer two crossed: turning the middle one to 45° lets some light through.
- Reflected glare is partly polarised, so polarising sunglasses cut it. Phone and LCD screens give out polarised light, so they look black through sunglasses turned 90°. A receiving aerial has to line up with the transmitter’s polarisation.
- Stress: between crossed filters, stressed plastic shows coloured fringes; closely packed fringes mean high stress.
Try: October 2025 Q18, June 2025 Q12(b), January 2026 Q18(c).
Pulse-echo
- distance = speed × time ÷ 2
Know cold
- A transducer sends short pulses. Part of each pulse reflects at a boundary between materials of different density (a crack, an air gap), the echo time is measured, the speed is known, and distance = vt/2 because the pulse goes there and back. Full version: skeleton E.
- Shorter pulses give better resolution: with a long pulse, echoes from boundaries close together overlap.
- Higher frequency means shorter λ, so smaller detail shows up. That’s why cracks are scanned with MHz, not kHz.
- The gap between pulses has to be longer than the echo time from the furthest target.
Try: January 2026 Q19, June 2025 Q13, June 2024 Q13.
6-mark bank
One Section B question carries an asterisk and 6 marks. Examiners give up to 4 marks for separate correct points and up to 2 for how well they link. Six points in a logical order gets 6; five points caps you at 5. Each skeleton is six points in the order you’d write them, one sentence each.
A. Why the photoelectric effect shows light is made of photonsJanuary 2022 Q13, October 2023 Q17, June 2021 Q15
- Light arrives as photons, each with energy E = hf, so the energy depends on frequency.
- Each photon interacts with one electron and gives it all its energy.
- An electron is released only if the photon energy is at least the work function, so there’s a threshold frequency. Below it nothing is emitted, however bright the light.
- Emission is instant, because the energy arrives in one packet rather than building up.
- Leftover energy becomes kinetic energy, Ek(max) = hf − φ, so it depends on frequency, not intensity.
- Brighter light means more photons per second, so more electrons per second (a bigger current), but not faster ones.
If the question mentions the wave model: it predicts that any frequency would work if the light were bright enough, that brighter light would give faster electrons, and that there’d be a delay.
B. Two-source interference (loudspeakers, harbour gaps, noise-cancelling)January 2023 Q15, January 2024 Q17, October 2020 Q13, October 2022 Q15
- Waves spread out (diffract) from each source or gap, so they overlap.
- Where they meet, they superpose.
- Where the path difference is a whole number of wavelengths they arrive in phase: constructive interference, loud or large amplitude.
- Moving to a new position changes the path difference.
- Where the path difference is an odd number of half-wavelengths they arrive in antiphase: destructive interference, quiet or small amplitude.
- This needs coherent sources (same frequency, constant phase difference). It’s never totally silent because the two waves arrive with different amplitudes.
Beats version: the two frequencies differ, so the sources aren’t coherent, the phase difference keeps changing, and the sound alternates between loud and quiet.
C. Line spectra and discharge tubesOctober 2021 Q16, June 2024 Q17
- Electrons in atoms can only have certain discrete energy levels.
- The atom gains energy: by absorbing a photon of exactly the right energy, or in a discharge tube by colliding with an electron accelerated by the p.d.
- An electron moves up to a higher level (the atom is excited).
- It drops back to a lower level and emits a photon.
- The photon’s energy equals the difference between the two levels, hf = E1 − E2.
- Only certain differences exist, so only certain frequencies and wavelengths appear: a line spectrum. Each element has its own levels, so its own spectrum.
D. How a stationary wave formsJune 2025 Q17 (a 3-mark version is in most papers)
- The source sends a wave along the string or down the tube.
- The wave reflects at the end (the fixed end, pulley or closed end).
- The incident and reflected waves have the same frequency and amplitude and travel in opposite directions, so they superpose.
- Where they’re always in antiphase, destructive interference gives a node (zero amplitude).
- Where they’re in phase, constructive interference gives an antinode (maximum amplitude).
- The ends fix the pattern: a fixed or closed end is a node and an open end of a tube is an antinode, so only certain frequencies fit.
E. Pulse-echo: finding a depth or a crackJanuary 2026 Q19, January 2020 Q13
- A transducer sends out short pulses of ultrasound.
- Part of each pulse reflects at the boundary between different materials (the crack), where the density changes.
- The transducer detects the echo and the time between sending and receiving is measured.
- The speed of ultrasound in the material is known.
- Distance = speed × time.
- Halve it, because the pulse travelled there and back.
F. Refraction and TIR at a surfaceOctober 2024 Q17
- Light is slower in water than in air (water has the higher refractive index).
- A ray leaving the water speeds up and bends away from the normal; a ray entering bends towards it.
- Work out the critical angle: sin C = 1/1.33, so C ≈ 49°.
- A ray hitting the surface from below at more than C is totally internally reflected.
- A ray at less than C refracts out, with some partial reflection.
- Say where each ray ends up, for example which ones reach the eye.
G. Thermistor or LDR potential dividerOctober 2025 Q17, October 2019 Q14, October 2023 Q14
- Temperature (or light level) goes up, so electrons gain energy.
- More conduction electrons are released.
- So the thermistor’s (or LDR’s) resistance falls.
- It’s in series with the fixed resistor: same current, and the supply p.d. is shared in proportion to resistance.
- It’s now a smaller share of the total resistance, so the p.d. across it falls and the p.d. across the fixed resistor rises.
- Link it to the output: the device switches when that p.d. crosses the set value. Add the calculation if the question asks for one.
H. LDR with internal resistance, or power in the whole circuitJanuary 2025 Q16, June 2023 Q14
- More light releases more conduction electrons in the LDR.
- So the LDR’s resistance falls.
- The circuit’s total resistance falls, so the current rises (the e.m.f. doesn’t change).
- The lost volts, Ir, rise because the current is bigger.
- So the terminal p.d., ε − Ir, falls. That’s what a voltmeter across the cell shows.
- Power version: the whole circuit’s power is P = εI, and I went up with ε unchanged, so the total power rises.
I. Filament lamp vs thermistor I–V graphsJanuary 2021 Q16
- Filament: as the p.d. rises, the current rises and the filament heats up.
- Its ions vibrate more, so electrons collide with them more often.
- So its resistance rises: the current increases more slowly than the p.d. and the graph curves over.
- Thermistor: it also heats up as the current rises.
- But more conduction electrons are released (n rises in I = nqvA).
- So its resistance falls: the current increases faster than the p.d. and the graph curves upward.
J. Current and p.d. rules, and cells in series vs parallelJune 2022 Q15, June 2026 Q18
- Current is the rate of flow of charge, and charge is conserved.
- So the current is the same everywhere in a series circuit, and at a junction the current in equals the current out.
- P.d. is the energy transferred per unit charge, and energy is conserved.
- So the p.d.s round a series loop add up to the e.m.f.
- Components in parallel have the same p.d. across them.
- Cells: in series the current is the same and the p.d.s add (higher voltage); in parallel the p.d. is the same and the currents add (higher current). P = VI, so the power can be equal either way. Series suits devices needing a high voltage; in parallel, one failed cell doesn’t stop the rest.
How to score
- “Show that”: write every step and give your answer to one more significant figure than the value in the question.
- “Deduce”, “assess” or “evaluate whether”: calculate the value, compare it in writing (“0.72 V is less than 1.0 V”), then state the conclusion. Skipping the comparison loses the last mark.
- “Explain”: one physics step per sentence, cause before effect, using the key words (conduction electrons, lattice vibrations, in phase, path difference, critical angle).
- Units on every final answer.
- Convert before you substitute: mm to m, mm2 to m2 (× 10−6), nm to m (× 10−9), kΩ, mA, minutes to seconds, kWh to J, eV to J.
- g = 9.81 N kg−1, never 10. Calculator in degrees.
- Timing: roughly a mark a minute, with 10 minutes spare. Don’t spend more than 10 minutes on the ten MCQs.
MCQ traps that keep coming back
- The SI base unit for charge is the ampere second (A s); the coulomb is a derived unit. Watt = kg m2 s−3, volt = J C−1, ohm = J s C−2.
- A displacement–time graph gives the period and frequency, never the wavelength.
- Frequency never changes when a wave refracts.
- Rotating a single polarising filter in unpolarised light doesn’t change the brightness.
- Phase difference is the fraction of a wavelength × 360°: λ/8 is 45°, 3λ/8 is 135°, λ/2 is 180°.
- In a stationary wave, points in one loop are in phase and neighbouring loops are in antiphase.
- A hotter thermistor has more conduction electrons and a lower R. A hotter metal has more vibration and a higher R.
- A photon is absorbed only if its energy exactly matches a gap; an electron can give up part of its energy.
- Brighter light gives more photoelectrons per second, not faster ones.
- Same current, double the diameter: a quarter of the drift velocity.
- Identical cells in parallel: the same e.m.f., internal resistance divided by the number of cells.
- Echo distance = speed × time ÷ 2.
- Grating: convert lines per mm to lines per m (× 1000) before d = 1/N.
- TIR needs higher n to lower n and an angle bigger than C.
- V against I for a cell: gradient −r, y-intercept ε.
- An electron accelerated through V volts gains eV joules (1 eV = 1.60 × 10−19 J).
Formula sheet: what’s printed and what isn’t
The last pages of the paper list the formulas and constants below. Don’t memorise them; practise using them.
Printed for you
- v = fλ
- v = √(T/μ)
- I = P/A
- n1 sin θ1 = n2 sin θ2
- n = c/v
- sin C = 1/n
- nλ = d sin θ
- V = W/Q
- R = V/I
- P = VI
- P = I2R
- P = V2/R
- W = VIt
- R = ρl/A
- I = ΔQ/Δt
- I = nqvA
- series and parallel R
- E = hf
- hf = φ + ½mv2max
- λ = h/p
- e, me, h, c, 1 eV, g
- from Unit 1: Ek = ½mv2, p = mv, P = E/t, W = mg, efficiency
Not printed, so learn these
- ε = I(R + r) and V = ε − Ir
- Vout = Vin × R/Rtotal potential divider
- phase difference = (path difference/λ) × 360°
- node to node = λ/2 string λ = 2L, closed tube L = λ/4
- A = 4πr2 point source
- distance = vt/2 echo
- E = hc/λ
- N = It/e number of electrons
- sin C = n2/n1 between two materials
- d = 1/N and tan θ = x/D grating
- A = πd2/4
- Ek = eV accelerated electron
- 1 kWh = 3.6 × 106 J
Papers to do
- October 2025: end of Day 1, open book, after the notes.
- January 2026: Day 2, timed.
- June 2026: Day 2, timed. It’s the newest paper and the closest to what you’ll sit.
If you finish early: June 2025, then October 2024 and June 2024.
Notes on the papers
- The January 2025 mark scheme wasn’t available for this analysis, so download it from Pearson before you use that paper.
- 2019 June is the old WPH02 specification. Skip it: it tests things like the Doppler effect that aren’t on your paper.
- 2020 June was actually sat in October 2020, because the June 2020 exams were cancelled.