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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

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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.

ParticleRelative chargeRelative massLocation
Proton+11nucleus
Neutron01nucleus
Electron−11/1840 (about 0.0005)around the nucleus
NuclideZANStable?
Hydrogen-1110yes
Deuterium121yes
Tritium132no (beta emitter)
Carbon-126126yes
Carbon-146148no (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

TypeCompositionChargeStopped by
Alphahelium-4 nucleus+2paper
Betaelectron−1aluminium
Gammaphoton0thick 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.

GroupMembers
Quarksup, down, charm, strange, top, bottom
Leptonselectron, muon, tau and their neutrinos
Force carriersphoton, gluon, W and Z bosons
Higgs bosongives particles mass (discovered 2012 at CERN)

Quark charges

  • up, charm, top +2/3 e;
    • down, strange, bottom −1/3 e.

The Standard Model and accelerators
Protons are uud and neutrons udd.
Meson
A meson is a hadron of one quark and one antiquark, such as the pion.
Every particle has an antiparticle; they annihilate into gamma photons.
Pair production: a gamma photon of at least 1.02 MeV near a nucleus can create an electron-positron pair, any extra energy becoming kinetic energy; in a magnetic field the two tracks curve in opposite directions.
The four fundamental forces are strong, electromagnetic, weak and gravitational, carried by gluons, photons and W and Z bosons respectively (strong, electromagnetic, weak).
Linear accelerators send particles in a straight line through tubes with alternating p.d.; synchrotrons use a ring of magnets and accelerating cavities, reusing the path.
The Large Hadron Collider is a 27 km ring.
Higher collision energies create heavier particles and probe smaller distances, because higher momentum means shorter de Broglie wavelength.
Conservation laws (charge, energy, momentum, baryon number, lepton number) show whether a reaction can happen.

Section 4 of 6Worked examples

  1. Radium-226 (Z = 88) decays by alpha emission to radon. Write the equation. [2]2 marks

  2. A sample has activity 3200 Bq and half-life 6.0 hours. Find its activity after 24 hours. [2]2 marks

  3. A wooden artefact has 25% of the carbon-14 of living wood (half-life 5730 years). How old is it? [2]2 marks

  4. Complete: 23892U → 23490Th + ?. [1]1 mark

  5. Explain why the nucleus holds together despite proton repulsion. [3]3 marks

Section 5 of 6Key terms

TermMeaning
Proton number (Z)Number of protons in the nucleus; identifies the element.
Strong nuclear forceShort-range attractive force holding nucleons together, range about 3 × 10−15 m.
Ionising radiationRadiation with enough energy to remove electrons from atoms and form ions.
Elementary particleA particle not made of any smaller particles.
MesonA hadron made of one quark and one antiquark.
Standard ModelTheory of 6 quarks, 6 leptons, exchange bosons and the Higgs boson.
Mass defectDifference between the mass of separate nucleons and the nucleus; gives binding energy via E = Δmc2.

Section 6 of 6Exam technique

1
Forgetting to balance both A and Z in decay equations.
2
Thinking half-life is half the total decay time — activity halves every half-life.
3
Saying alpha is the most dangerous source outside the body — it is most dangerous inside.
4
Confusing binding energy with energy to build the nucleus — it is the energy needed to separate it.
5
Treating quarks as having whole-number charges.

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