A-Level Revision Aid: This resource is designed to support your revision. Content may contain errors. If you find a discrepancy with your class teaching, your teacher is correct — please let us know at alevelrevise@scott.scottrix.co.uk.
A-Level Physics revision: photoelectric effect with Einstein's equation, energy levels and line spectra, wave-particle duality, de Broglie wavelength and particle physics basics (standard model, conservation laws) - AQA 7408 3.2, OCR A H556 4.4/6.4-6.5, Edexcel 9PH0 Topics 5/8.
🎯 Learning Objectives
Explain the photoelectric effect with Einstein's equation hf = φ + KE_max, threshold frequency and stopping potential (AO1/AO2) - AQA 7408 3.2.2.1, OCR A H556 4.4
Use the photon model E = hf = hc/λ and calculate photon energies and momenta (AO2) - AQA 7408 3.2.2.1
Describe atomic line spectra and discrete energy levels; calculate photon wavelength from transitions ΔE = hf (AO2) - AQA 7408 3.2.2.2
Explain wave-particle duality and use the de Broglie relation λ = h/p (AO1/AO2) - AQA 7408 3.2.2.2, OCR A H556 4.4.2
Describe the standard model: quarks, leptons, hadrons (baryons and mesons), and apply conservation laws (charge, baryon number, lepton number, strangeness) (AO1/AO2) - AQA 7408 3.2.1, Edexcel 9PH0 Topic 8
Describe particle interactions (strong, weak, electromagnetic) and beta decay at quark level (AO2) - AQA 7408 3.2.1
📋 Key Definitions and Core Concepts
Photon: A quantum of electromagnetic energy: E = hf = hc/λ; photons transfer energy in discrete packets.
Work function (φ): The minimum energy needed to remove an electron from a metal surface; φ = hf_0 where f_0 is the threshold frequency.
Threshold frequency (f_0): The minimum frequency of light that ejects photoelectrons; below it, no electrons are emitted however intense the light.
Stopping potential (V_s): The pd that just stops the fastest photoelectrons: eV_s = KE_max.
Energy level: A discrete allowed electron energy in an atom; electrons absorb or emit photons only when moving between levels, ΔE = hf.
Ionisation: Removal of an electron from an atom; the ionisation energy of hydrogen is 13.6 eV (from the ground level E = -13.6 eV to zero).
de Broglie wavelength: λ = h/p - every moving particle has an associated wavelength; electron diffraction demonstrates it.
Hadron: A particle made of quarks that feels the strong interaction: baryons (3 quarks, e.g. proton, neutron) and mesons (quark-antiquark pair, e.g. pion).
Lepton: A fundamental particle that does not feel the strong interaction: electron, muon, tau and their neutrinos.
Strangeness: A quantum number conserved in strong interactions but allowed to change by ±1 in weak interactions.
📌 Key Points
Photon: E = hf = hc/λ; 1 eV = 1.60 × 10^-19 J.
Photoelectric: hf = φ + KE_max; threshold f_0 = φ/h; one photon interacts with one electron - no time lag, intensity only changes the rate.
Stopping potential: eV_s = KE_max.
Energy levels: E_n = -13.6/n^2 eV (hydrogen); transitions give ΔE = hf; emission (excited → lower) and absorption (lower → higher).
de Broglie: λ = h/p = h/√(2mE_k) for non-relativistic particles; electron diffraction proves wave nature.
Quarks (u, d, s, c, b, t) in baryons (3 quarks) and mesons (q q̄); leptons (e, μ, τ and neutrinos); interactions: strong, weak, EM, gravity (negligible).
Conservation: charge, baryon number, lepton number always; strangeness in strong interactions only (weak can change it by ±1).
The photoelectric effect
Shine light on a metal and electrons can be ejected - the photoelectric effect (AQA 7408 3.2.2.1; OCR A H556 4.4.1; Edexcel 9PH0 Topic 5). Three observations killed the wave theory: (1) there is a threshold frequency f_0 below which no electrons are emitted, however intense the light (wave theory: any frequency should work given enough intensity); (2) emission is instantaneous even for dim light (wave theory: energy should take time to accumulate); (3) the maximum kinetic energy of photoelectrons depends only on frequency, not intensity (wave theory: brighter light should mean faster electrons).
Einstein's photon model: light arrives in discrete packets of energy E = hf. One photon is absorbed by one electron in a one-to-one interaction: the electron gains hf, spends the work function φ (minimum energy to escape the surface) and leaves with the remainder: hf = φ + KE_max. Instantaneous, because the energy arrives in one packet. Intensity changes the number of photons per second, so it changes the rate of emission, not the energy per electron. Threshold: KE_max = 0 gives f_0 = φ/h. Electrons deeper in the metal need more than φ, so they leave with less than KE_max - hence a range of energies up to the maximum.
Stopping potential derivation: apply a reverse pd V_s that just stops the fastest electrons. The electrons do work eV_s against the field, losing all their KE: eV_s = KE_max = hf - φ. Plotting V_s against f gives a straight line of gradient h/e and intercept -φ/h - one experimental route to Planck's constant. The gold-leaf electroscope demonstration: a negatively charged zinc plate loses its charge instantly under UV light (electrons ejected) but not under visible light even at high intensity - below threshold for zinc (φ ≈ 4.3 eV, UV ≈ 5+ eV).
Worked example: photoelectric equation
Light of wavelength 420 nm is incident on a metal with work function 1.9 eV. Find the maximum kinetic energy of the photoelectrons. (h = 6.63 × 10^-34 J s, c = 3.00 × 10^8 m/s)
Line 1: Photon energy E = hc/λ = (6.63 × 10^-34 × 3.00 × 10^8)/(420 × 10^-9) = 4.74 × 10^-19 J (M1 A1).
Line 2: φ = 1.9 × 1.60 × 10^-19 = 3.04 × 10^-19 J (M1: eV to J conversion).
Electrons in atoms occupy discrete energy levels - negative values because the electron is bound (zero is free, at infinity) (AQA 7408 3.2.2.2). An electron can move between levels only by absorbing or emitting exactly the energy gap as a photon: ΔE = hf = hc/λ. Emission spectra (bright lines on dark) come from excited electrons falling to lower levels; absorption spectra (dark lines on continuous) from cool gas absorbing exactly those photons out of white light passing through. Each element has a unique set of levels, hence unique spectral lines - the fingerprint used to identify elements in stars.
Hydrogen: E_n = -13.6/n^2 eV (n = 1 ground: -13.6 eV; n = 2: -3.40 eV; n = 3: -1.51 eV; n = ∞: 0, ionisation). Series names: transitions ending on n = 1 (Lyman, UV), n = 2 (Balmer, visible), n = 3 (Paschen, IR). Fluorescence: absorb UV, electrons excited, then cascade down emitting visible photons of lower energy each - energy is conserved overall. Excitation by collision: electrons in a fluorescent tube collide with gas atoms, transferring exactly the excitation energies; the fluorescent coating converts UV to visible. Line spectra evidence: discrete lines prove discrete levels - a continuum of possible energies would give a continuous spectrum.
Worked example: hydrogen transition
A hydrogen electron falls from n = 3 (E_3 = -1.51 eV) to n = 2 (E_2 = -3.40 eV). Find the photon energy and wavelength.
Line 3: λ = 6.6 × 10^-7 m = 660 nm - red light, a Balmer line (A1).
Wave-particle duality
Light behaves as a wave (interference, diffraction) and as particles (photoelectric effect, photon momentum) - the photon model with E = hf and p = h/λ (AQA 7408 3.2.2.2). de Broglie's hypothesis extends duality to matter: every moving particle has an associated wavelength λ = h/p. For a non-relativistic particle with kinetic energy E_k, p = √(2mE_k) (from E_k = p^2/2m), so λ = h/√(2mE_k); for an electron accelerated through pd V: E_k = eV, so λ = h/√(2meV).
Evidence: electron diffraction. Accelerate electrons through a pd and fire them at a thin polycrystalline graphite film: the screen shows concentric diffraction rings - the spacing matches the predicted λ = h/p. Faster electrons (higher accelerating voltage) give smaller λ and closer rings - the quantitative test. Neutron diffraction similarly probes crystal structure. Why don't we see cricket-ball diffraction? λ = h/p with a macroscopic p is ~10^-34 m - unobservably small; duality only shows when λ is comparable to the spacing of the obstacles (atomic spacings ~10^-10 m for electrons through ~100 V).
Electron microscopes exploit the small λ: resolving power improves as wavelength shrinks, so electrons at ~100 kV (λ ~ 4 pm) resolve far finer detail than visible light (λ ~ 500 nm).
Worked example: de Broglie wavelength
An electron (m = 9.11 × 10^-31 kg) is accelerated through 150 V. Find its de Broglie wavelength.
Line 1: E_k = eV = 1.60 × 10^-19 × 150 = 2.4 × 10^-17 J (M1 A1).
Line 2: p = √(2mE_k) = √(2 × 9.11 × 10^-31 × 2.4 × 10^-17) = 6.61 × 10^-24 kg m/s (M1 A1).
Line 3: λ = h/p = 6.63 × 10^-34/6.61 × 10^-24 = 1.0 × 10^-10 m = 0.10 nm (A1) - comparable to atomic spacing, hence electron diffraction works.
Particle physics basics: the standard model
Quarks (u, d, s, c, b, t) and antiquarks build hadrons - particles feeling the strong interaction (AQA 7408 3.2.1; Edexcel 9PH0 Topic 8; OCR A H556 6.5). Baryons are three quarks (proton uud, neutron udd); mesons are quark-antiquark pairs (pions, kaons). Leptons are fundamental, non-strong: electron, muon, tau and their neutrinos (ν_e, ν_μ, ν_τ). Quark charges: u = +2/3e, d = -1/3e - add them for hadron charges (proton: 2/3 + 2/3 - 1/3 = +1e).
Interactions: the strong force binds quarks (gluons) and holds nuclei together - very short range (~10^-15 m); the weak force mediates beta decay (W±, Z^0 bosons) and can change quark flavour; the electromagnetic force acts on charged particles (photons); gravity is negligible at particle scales. Conservation laws for deciding if a reaction happens: charge, baryon number B (baryon +1, antiquark -1/3 per quark... in practice: baryon +1, meson 0, lepton 0), lepton number L (electron family: electron +1, electron neutrino +1, their antiparticles -1), and strangeness - conserved in strong interactions, changed by ±1 in weak interactions (kaons are strange particles, created in pairs by the strong force).
Beta-minus decay at quark level: n → p + e^- + ν̄_e. At quark level, one d quark changes to a u quark via the weak interaction, emitting a W^- boson which decays into an electron and an antineutrino: d → u + W^-, then W^- → e^- + ν̄_e (Feynman diagram in words: incoming d line bends to u, W^- zigzag leaves the vertex and splits into the electron-antineutrino pair). Check conservation: charge 0 → (+1) + (-1) + 0 ✓; baryon number 1 → 1 ✓; lepton number 0 → 0 + (+1) + (-1) ✓. Pair production (photon → particle-antiparticle pair, needs E ≥ 2mc^2) and annihilation (particle-antiparticle → two photons) are the standard energy-bookkeeping examples - PET scanners use positron-electron annihilation.
Worked example: conservation check
Is p + π^- → K^+ + K^0 possible in a strong interaction? (π^-, K^+ and K^0 contain strange/anti-strange quarks; K^0 has strangeness +1.)
Line 2: Charge conservation fails, so the reaction is impossible however the other numbers work (A1). (Check the others for practice: B = 1 + 0 → 0 + 0 fails too.)
Practical work: estimating Planck's constant with LEDs
The standard practical for quantum phenomena is estimating h from LEDs (OCR PAG5; Edexcel practical work on quantum; AQA covers it under 3.2.2). Each LED emits photons of a known colour/wavelength λ when the pd across it reaches the activation voltage V_0: the electrical energy per electron eV_0 equals the photon energy hf = hc/λ. So eV_0 = hc/λ, giving h = eV_0 λ/c.
Method: connect an LED in series with a resistor and a variable supply; increase the pd slowly in the dark until the LED just begins to emit - record that activation voltage (take several readings, average). Repeat for LEDs of several wavelengths (red, yellow, green, blue). Plot V_0 against 1/λ: a straight line through the origin of gradient hc/e, so h = gradient × e/c. Using the gradient across all LEDs averages random error and tests the model (a straight line confirms eV_0 ∝ 1/λ).
Evaluation points: judging the exact activation point is subjective (the LED glows dimly before it is obvious) - use a consistent, dim criterion in darkness; the pd measured is across the LED plus any voltmeter loading - use a high-resistance voltmeter; some energy is lost as heat in the LED (non-radiative recombination), so the measured h tends to be high; wavelength spreads (LEDs are not perfectly monochromatic) add uncertainty. Quote h with its uncertainty and compare with 6.63 × 10^-34 J s using the percentage difference.
Worked example: h from an LED
A blue LED (λ = 470 nm) just lights at V_0 = 2.62 V.
Line 1: eV_0 = hc/λ, so h = eV_0 λ/c (M1: energy balance).
Line 2: h = (1.60 × 10^-19 × 2.62 × 470 × 10^-9)/(3.00 × 10^8) (M1: substitution).
Line 3: h = 1.969 × 10^-25/3.00 × 10^8 = 6.6 × 10^-34 J s (A1) - within a few percent of the accepted 6.63 × 10^-34 J s.
💡 Worked Example
Exam-style: Light of wavelength 420 nm is incident on a metal with work function 1.9 eV. (a) Calculate the maximum kinetic energy of the emitted photoelectrons in joules. (b) Explain why no photoelectrons are emitted when the wavelength is increased to 700 nm. (h = 6.63 × 10^-34 J s, c = 3.00 × 10^8 m/s) (AQA 7408-style, 6 marks)
Mark-scheme logic: (a) Photon energy E = hc/λ = (6.63 × 10^-34 × 3.00 × 10^8)/(420 × 10^-9) = 4.74 × 10^-19 J (M1 A1: photon energy with unit conversion). Work function φ = 1.9 × 1.60 × 10^-19 = 3.04 × 10^-19 J (M1: eV to J). KE_max = hf - φ = 4.74 × 10^-19 - 3.04 × 10^-19 = 1.7 × 10^-19 J (A1). (b) At 700 nm: photon energy = (6.63 × 10^-34 × 3.00 × 10^8)/(700 × 10^-9) = 2.84 × 10^-19 J = 1.78 eV (M1: new photon energy). This is less than the work function 1.9 eV, so the photon cannot supply the minimum energy to free an electron from the surface (A1: threshold condition). One photon interacts with one electron, so intensity cannot compensate - below threshold frequency no emission occurs whatever the brightness (A1: photon model explanation).
❓ Practice Questions & Mark Schemes
Calculate the energy of a photon of wavelength 400 nm in joules and eV. (h = 6.63 × 10^-34 J s, c = 3.00 × 10^8 m/s)
Answer: E = hc/λ = (6.63 × 10^-34 × 3.00 × 10^8)/(400 × 10^-9) (M1) = 4.97 × 10^-19 J (A1). In eV: 4.97 × 10^-19/1.60 × 10^-19 = 3.1 eV (A1: 1 eV = 1.60 × 10^-19 J).
Calculate the de Broglie wavelength of an electron accelerated through 100 V. (m = 9.11 × 10^-31 kg, h = 6.63 × 10^-34 J s)
Answer: E_k = eV = 1.60 × 10^-19 × 100 = 1.60 × 10^-17 J (M1 A1). p = √(2mE_k) = √(2 × 9.11 × 10^-31 × 1.60 × 10^-17) = 5.40 × 10^-24 kg m/s (M1 A1). λ = h/p = 1.2 × 10^-10 m = 0.12 nm (A1) - atomic scale, hence electron diffraction.
A hydrogen electron falls from n = 3 (E_3 = -1.51 eV) to n = 2 (E_2 = -3.40 eV). Calculate the wavelength of the emitted photon and state its colour.
Answer: ΔE = -1.51 - (-3.40) = 1.89 eV = 3.02 × 10^-19 J (M1 A1: energy difference sign handled). λ = hc/ΔE = 6.6 × 10^-7 m = 660 nm (M1 A1) - red light, a Balmer-series line.
State the quark transformation in beta-minus decay and show that the process conserves charge, baryon number and lepton number.
Answer: A down quark changes to an up quark via the weak interaction: d → u + e^- + ν̄_e (M1 A1: weak interaction, W^- intermediate). Charge: 0 = +2/3 - 1/3... at particle level 0 → (+1) + (-1) + 0 ✓ (A1). Baryon number: 1/3 (quark) conserved in the d → u change ✓. Lepton number: 0 → 0 + (+1) + (-1) = 0 ✓ (A1).
Electrons accelerated through 200 V show diffraction rings with a thin graphite film. Explain why the rings get closer together if the accelerating voltage is increased.
Answer: Higher V → higher E_k = eV (M1). p = √(2mE_k) increases, so λ = h/p decreases (M1 A1: de Broglie relation). Smaller λ → smaller diffraction angles (sin θ ∝ λ for fixed grating spacing), so the rings move closer to the centre (A1).
In an LED experiment, a red LED (λ = 640 nm) just lights at 1.90 V. Estimate Planck's constant.
Answer: eV_0 = hc/λ (M1: energy balance at activation). h = eV_0 λ/c = (1.60 × 10^-19 × 1.90 × 640 × 10^-9)/(3.00 × 10^8) (M1) = 6.5 × 10^-34 J s (A1) - close to 6.63 × 10^-34 J s.