Revision Notes
AQA A-Level Physics: Particles and radiation (7408) – Revision Notes
Condensed revision notes for AQA A-level Physics 7408 Particles and radiation: tables, conservation checks, photon equations and a quick self-test.
- Subject
- Physics
- Level
- A LEVELS
- Topic
- Particles and radiation
- Author
- Marlbridge Academic Team
- Updated
Aligned to AQA A Level Physics (7408), For first teaching 2015. Official specification .
Syllabus page (what it covers and how it is assessed): AQA A Level Physics.
Syllabus points this page covers
7408
- 2 Particles and radiation (whole topic)
- 3.2.1 Particles
- 3.2.2 Electromagnetic radiation and quantum phenomena
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These notes condense section 3.2 Particles and radiation of the AQA AS and A-level Physics (7407/7408) specification, version 1.4 (AS and A-level exams June 2016 onwards): 3.2.1 Particles and 3.2.2 Electromagnetic radiation and quantum phenomena. It is AS and A-level content, examined in A-level Paper 1 and assumed in Paper 2. Sections 3.9-3.13 are options (you study one, assessed in Paper 3 Section B); this topic is compulsory. For full explanations and worked examples, use the Particles and radiation study guide.
Also see: practice questions, the AQA A-level Physics hub, the printable checklist and the free diagnostics.
Key equations
| Equation | Use | Units |
|---|---|---|
| specific charge = Q/m | nuclei, ions, particles | C kg⁻¹ |
| E = hf = hc/λ | photon energy | J |
| hf = ϕ + Ek(max) | photoelectric effect | J (or eV on both sides) |
| eVs = Ek(max) | stopping potential | Vs in V |
| hf = E1 − E2 | photon emitted between levels | J |
| λ = h/mv | de Broglie wavelength | m |
| 1 eV = 1.60 × 10⁻¹⁹ J | energy conversion | – |
Constants used here: h = 6.63 × 10⁻³⁴ J s, c = 3.00 × 10⁸ m s⁻¹, e = 1.60 × 10⁻¹⁹ C, mₑ = 9.11 × 10⁻³¹ kg.
3.2.1.1 The atom in numbers
| Charge / C | Rel. charge | Mass / kg | Rel. mass | |
|---|---|---|---|---|
| p | +1.60 × 10⁻¹⁹ | +1 | 1.67 × 10⁻²⁷ | 1 |
| n | 0 | 0 | 1.67 × 10⁻²⁷ | 1 |
| e⁻ | −1.60 × 10⁻¹⁹ | −1 | 9.11 × 10⁻³¹ | ≈ 0.0005 |
- Z = protons; A = nucleons; neutrons = A − Z. Nuclide notation: ᴬ_Z X.
- Isotopes: same Z, different number of neutrons.
- Specific charge = charge/mass (C kg⁻¹). For an ion use the net charge (number of electrons gained or lost × e) and mass ≈ A × 1.67 × 10⁻²⁷ kg.
3.2.1.2 Nuclear stability
- Strong nuclear force: attractive to about 3 fm, repulsive below about 0.5 fm, acts between nucleons.
- Alpha: ᴬ_Z X → ᴬ⁻⁴_(Z−2) Y + ⁴₂α.
- β⁻: ᴬ_Z X → ᴬ_(Z+1) Y + ⁰₋₁β + ν̄ₑ.
- Neutrino proposed because beta particles have a range of energies: energy conservation needed another particle.
3.2.1.3 Antiparticles and photons
| Particle | Antiparticle | Rest energy / MeV |
|---|---|---|
| electron | positron | 0.511 |
| proton | antiproton | 938.3 |
| neutron | antineutron | 939.6 |
| neutrino | antineutrino | – |
Same mass and rest energy; opposite charge.
- E = hf = hc/λ.
- Annihilation: particle + antiparticle → two photons (momentum). E_photon(min) = rest energy of one particle.
- Pair production: one photon → particle + antiparticle. E_photon(min) = 2 × rest energy.
Worked reminder. Minimum photon energy to make a neutron-antineutron pair = 2 × 939.6 = 1879.2 MeV. Any extra energy becomes kinetic energy of the pair.
3.2.1.4 Exchange particles
| Force | Exchange particle | Acts on |
|---|---|---|
| Electromagnetic | virtual photon | charged particles |
| Weak | W⁺, W⁻ | all particles |
| Strong (between nucleons) | pion | hadrons |
Method: drawing a weak-interaction diagram
- Write the equation. Put the incoming particles at the bottom.
- Find which particle changes identity (for example p → n).
- Choose W⁺ or W⁻ so charge balances at that vertex.
- At the other vertex, the W turns into (or meets) the leptons; check charge again.
Covered: β⁻, β⁺, electron capture (p + e⁻ → n + νₑ), electron-proton collision (e⁻ + p → n + νₑ). Gluon, Z⁰ and graviton are not tested.
3.2.1.5–3.2.1.6 Classification and quarks
| Quark | Q | B | S |
|---|---|---|---|
| u | +⅔ | +⅓ | 0 |
| d | −⅓ | +⅓ | 0 |
| s | −⅓ | +⅓ | −1 |
Antiquarks: reverse every sign.
| Family | Members | B | Quarks |
|---|---|---|---|
| Baryons | p (uud), n (udd) | +1 | qqq |
| Antibaryons | p̄ (ūūd̄), n̄ (ūd̄d̄) | −1 | q̄q̄q̄ |
| Mesons | π⁺ ud̄, π⁻ dū, π⁰ uū/dd̄, K⁺ us̄, K⁻ sū, K⁰ ds̄, K̄⁰ sd̄ | 0 | qq̄ |
| Leptons | e⁻, μ⁻, νₑ, ν_μ (+ antiparticles) | 0 | none |
- Proton: the only stable baryon. Kaon: decays into pions. Muon: decays into an electron.
- Lepton numbers: Lₑ = +1 for e⁻ and νₑ, −1 for e⁺ and ν̄ₑ; L_μ = +1 for μ⁻ and ν_μ, −1 for μ⁺ and ν̄_μ.
- Strange particles: made in pairs by the strong interaction, decay by the weak interaction.
- Large international teams validate new particle results.
3.2.1.7 Conservation checklist
| Quantity | Strong | Weak |
|---|---|---|
| Charge Q | conserved | conserved |
| Baryon number B | conserved | conserved |
| Lₑ and L_μ (separately) | conserved | conserved |
| Strangeness S | conserved | can change by 0, ±1 |
| Energy, momentum | conserved | conserved |
- β⁻: d → u. β⁺: u → d. Neutron decay: n → p + e⁻ + ν̄ₑ.
- Data will be given for particles outside the specified list.
Method: is this interaction possible?
- Write Q, B, Lₑ, L_μ and S under every particle, on both sides.
- Add each row. Any mismatch in Q, B, Lₑ or L_μ: impossible.
- If only S changes, by 1: possible by the weak interaction only.
- If S changes by 2 or more: impossible.
Worked reminder. K⁺ → π⁺ + π⁰. Q: +1 → +1 + 0. B: 0 → 0. S: +1 → 0 + 0, a change of 1. Allowed, weak decay – as expected, since strange particles decay by the weak interaction.
3.2.2.1 Photoelectric effect
- hf = ϕ + Ek(max); threshold f₀ = ϕ/h; stopping potential eVs = Ek(max).
- One photon frees at most one electron. Below f₀: no emission at any intensity.
- More intensity → more photoelectrons per second; same Ek(max).
- Higher frequency → larger Ek(max).
Worked reminder. Radiation of 1.5 × 10¹⁵ Hz on a metal with ϕ = 3.6 eV: hf = 9.95 × 10⁻¹⁹ J = 6.22 eV, so Ek(max) = 6.22 − 3.6 = 2.62 eV and Vs = 2.62 V. Working in eV throughout avoids converting back and forth.
3.2.2.2 Collisions of electrons with atoms
- 1 eV = 1.60 × 10⁻¹⁹ J. eV → J: multiply. J → eV: divide.
- Excitation: electron moves up a level. Ionisation: electron removed.
- An incoming electron can give part of its energy; a photon is absorbed only if its energy exactly matches a gap (or exceeds the ionisation energy).
- Fluorescent tube: electrons excite mercury atoms → UV photons → phosphor absorbs UV → emits visible light.
3.2.2.3 Energy levels
- Line spectra → discrete energy levels.
- hf = E1 − E2 (levels in J or eV; convert to J before using h).
- n levels give at most n(n − 1)/2 different emission lines.
3.2.2.4 Wave-particle duality
- Photoelectric effect → light behaves as particles. Electron diffraction → particles behave as waves.
- λ = h/mv. Greater momentum → shorter λ → less diffraction (smaller rings).
Must-know distinctions
- Hadron vs lepton: hadrons feel the strong interaction; leptons do not.
- Baryon vs meson: three quarks (B = ±1) vs quark-antiquark (B = 0).
- Annihilation vs pair production: two photons out, minimum energy each = one rest energy; versus one photon in, minimum energy = two rest energies.
- Excitation vs ionisation: moving up a level vs leaving the atom.
- Intensity vs frequency: intensity sets the number of photoelectrons; frequency sets Ek(max).
Quick self-test
- Find the energy of a photon of frequency 5.0 × 10¹⁴ Hz, in J and in eV.
- Convert 2.4 eV to joules.
- A metal has work function 2.3 eV. Find its threshold frequency.
- State the minimum photon energy, in MeV, to produce an electron-positron pair.
- Find the de Broglie wavelength of a 0.20 kg ball moving at 30 m s⁻¹.
- Calculate the specific charge of an alpha particle.
- Find the wavelength emitted when hydrogen falls from −1.51 eV to −13.6 eV.
- Find the de Broglie wavelength of an electron moving at 2.0 × 10⁶ m s⁻¹.
- Give the quark make-up and strangeness of a K⁻.
- Is p → n + e⁺ + ν̄ₑ allowed? Give a reason.
- Which exchange particle is involved in electron capture?
Answers
- E = hf = 6.63 × 10⁻³⁴ × 5.0 × 10¹⁴ = 3.3 × 10⁻¹⁹ J, which is 2.1 eV.
- 2.4 × 1.60 × 10⁻¹⁹ = 3.84 × 10⁻¹⁹ J.
- f₀ = (2.3 × 1.60 × 10⁻¹⁹)/6.63 × 10⁻³⁴ = 5.6 × 10¹⁴ Hz.
- 2 × 0.511 = 1.022 MeV.
- λ = 6.63 × 10⁻³⁴/(0.20 × 30) = 1.1 × 10⁻³⁴ m – far too small to diffract.
- (2 × 1.60 × 10⁻¹⁹)/(4 × 1.67 × 10⁻²⁷) = 4.79 × 10⁷ C kg⁻¹.
- ΔE = 12.09 eV = 1.934 × 10⁻¹⁸ J; λ = hc/ΔE = 1.03 × 10⁻⁷ m (ultraviolet).
- λ = 6.63 × 10⁻³⁴/(9.11 × 10⁻³¹ × 2.0 × 10⁶) = 3.6 × 10⁻¹⁰ m.
- sū, S = −1.
- No: Lₑ goes from 0 to −2 (positron −1, antineutrino −1). It should be a neutrino.
- W⁺ (from proton to electron), or equivalently W⁻ from electron to proton.
Where marks are usually lost
- Writing a neutrino in β⁻ decay or an antineutrino in β⁺ decay.
- Saying annihilation makes one photon; momentum needs two.
- Using the pion as the exchange particle for the weak interaction.
- Checking strangeness for a weak decay and calling it forbidden.
- Saying higher intensity gives faster photoelectrons.
- Leaving energy in eV when substituting into λ = hc/E.
- Calling a meson a baryon because it contains quarks; count the quarks.
- Giving the electron capture products as a neutron and an antineutrino.
- Forgetting the strong force is repulsive below about 0.5 fm when explaining why nuclei do not collapse.
Official syllabus
AQA AS and A-level Physics (7407/7408) specification, version 1.4, July 2026, AS and A-level exams June 2016 onwards, published by AQA. Section 3.2 Particles and radiation.
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