Nuclear and Particle Physics
Nuclear and Particle Physics — American System Physics Revision Notes & Topical Questions
5 min read 6 parts Lesson 1 of 5 1 quiz
Nuclear and Particle Physics — AMERICAN SYSTEM PHYSICS notes: Describe nuclear structure, binding energy, decay, half-life, fission and the Standard Model, using conservation laws.The nucleon number is A = Z + N (proton number plus neutron number).
- strong nuclear force
- Ionising radiation
- elementary particle
- Worked example 1
- Worked example 2
- Worked example 3
Section 1 of 6Nuclear structure and binding energy
The nucleon number is A = Z + N (proton number plus neutron number). Proton number (atomic number Z) identifies the element and equals the electrons in a neutral atom.
| Particle | Relative charge | Relative mass | Location |
|---|---|---|---|
| Proton | +1 | 1 | nucleus |
| Neutron | 0 | 1 | nucleus |
| Electron | −1 | 1/1840 (about 0.0005) | around the nucleus |
| Nuclide | Z | A | N | Stable? |
|---|---|---|---|---|
| Hydrogen-1 | 1 | 1 | 0 | yes |
| Deuterium | 1 | 2 | 1 | yes |
| Tritium | 1 | 3 | 2 | no (beta emitter) |
| Carbon-12 | 6 | 12 | 6 | yes |
| Carbon-14 | 6 | 14 | 8 | no (beta emitter) |
The strong nuclear force is attractive between nucleons, much stronger than electrostatic repulsion but acting only over a very short range (about 3 × 10−15 m). Protons repel electrostatically; all nucleons attract by the strong force; neutrons add attraction without extra repulsion; where attraction outweighs repulsion the nucleus is stable, and energy equal to the binding energy is needed to separate it.
To calculate binding energy
- add the masses of the separate protons (Z × 1.007276 u) and neutrons (N × 1.008665 u);
- subtract the measured nuclear mass to get the mass defect Δm (u);
- binding energy (MeV) = Δm × 931.5 MeV/u, or convert Δm to kg (× 1.66 × 10−27) and use E = Δmc2;
- divide by A for binding energy per nucleon.
- The higher the binding energy per nucleon, the more stable the nucleus.
Section 2 of 6Radiation, decay, half-life and fission
| Type | Composition | Charge | Stopped by |
|---|---|---|---|
| Alpha | helium-4 nucleus | +2 | paper |
| Beta | electron | −1 | aluminium |
| Gamma | photon | 0 | thick lead |
Decay equations balance A and Z: 23892U → 23490Th + 42He. Activity falls by half every half-life. A typical fission is 10n + 23592U → 14156Ba + 9236Kr + 3 10n + energy (about 200 MeV). Fusion is light nuclei combining and releasing energy.
Ionising radiation has enough energy to remove electrons from atoms, making ions. It damages or kills cells and can cause mutations and cancer. Alpha is most dangerous inside the body; beta and gamma are most dangerous outside it. Precautions: keep sources in lead-lined boxes, handle with tongs, keep distance, minimise exposure time and wear dosimeter badges.
Section 3 of 6The Standard Model and accelerators
The Standard Model describes all known matter as made from 6 quarks and 6 leptons, with forces carried by exchange particles (bosons), plus the Higgs boson. An elementary particle is not made of smaller particles.
| Group | Members |
|---|---|
| Quarks | up, down, charm, strange, top, bottom |
| Leptons | electron, muon, tau and their neutrinos |
| Force carriers | photon, gluon, W and Z bosons |
| Higgs boson | gives particles mass (discovered 2012 at CERN) |
Quark charges
- up, charm, top +2/3 e;
- down, strange, bottom −1/3 e.
Section 4 of 6Worked examples
Radium-226 (Z = 88) decays by alpha emission to radon. Write the equation. [2]2 marks
22688Ra → 22286Rn + 42He. Check: 226 = 222 + 4 and 88 = 86 + 2.
A sample has activity 3200 Bq and half-life 6.0 hours. Find its activity after 24 hours. [2]2 marks
n = 24/6.0 = 4 half-lives. Activity = 3200 × (½)4 = 3200/16 = 200 Bq.
A wooden artefact has 25% of the carbon-14 of living wood (half-life 5730 years). How old is it? [2]2 marks
25% = (½)2, so 2 half-lives: 2 × 5730 = 11 460 years (about 1.1 × 104 years).
Complete: 23892U → 23490Th + ?. [1]1 mark
42He, an alpha particle.
Explain why the nucleus holds together despite proton repulsion. [3]3 marks
Protons repel electrostatically but all nucleons attract through the short-range strong nuclear force; neutrons add attraction without repulsion; where attraction outweighs repulsion the nucleus is stable.
Section 5 of 6Key terms
| Term | Meaning |
|---|---|
| Proton number (Z) | Number of protons in the nucleus; identifies the element. |
| Strong nuclear force | Short-range attractive force holding nucleons together, range about 3 × 10−15 m. |
| Ionising radiation | Radiation with enough energy to remove electrons from atoms and form ions. |
| Elementary particle | A particle not made of any smaller particles. |
| Meson | A hadron made of one quark and one antiquark. |
| Standard Model | Theory of 6 quarks, 6 leptons, exchange bosons and the Higgs boson. |
| Mass defect | Difference between the mass of separate nucleons and the nucleus; gives binding energy via E = Δmc2. |
Section 6 of 6Exam technique
Marked practiceQuizzes for this lesson
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