β Unit 1: What ideas explain the physical world?
What holds atomic nuclei together and why do some decay?
Describe the structure of atomic nuclei, the strong nuclear force, and the modes of radioactive decay (alpha, beta-minus, beta-plus, gamma), and write balanced nuclear equations
A focused answer to the VCE Physics Unit 1 dot point on nuclear structure and decay. Describes the strong nuclear force, the neutron-proton ratio for stability, and the four classical decay modes ($\alpha$, $\beta^-$, $\beta^+$, $\gamma$). Works the VCAA SAC-style balanced-equation problem.
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What this dot point is asking
VCAA wants you to describe the nucleus (protons, neutrons, the strong force, stability), identify the four classical decay modes, and write balanced nuclear equations that conserve mass number and atomic number.
The nucleus
Atomic nuclei contain protons () and neutrons (), together called nucleons. The mass number . Notation: where is the chemical symbol.
The strong nuclear force binds nucleons. It is short-range (about fm), attractive, and stronger than the electromagnetic repulsion between protons over very short distances.
Stability
Stable nuclei occupy a narrow "valley of stability" on a vs chart. For light nuclei (), stable isotopes have . For heavier nuclei, more neutrons are needed to dilute the proton-proton repulsion: stable isotopes have near uranium.
Unstable nuclei decay toward the valley of stability through one or more decay events.
Alpha decay
The nucleus emits an alpha particle (He). Common for heavy nuclei ().
Alpha particles are highly ionising but have low penetration (stopped by paper).
Beta-minus decay
A neutron decays into a proton plus an electron plus an electron antineutrino. The electron is emitted as the beta particle.
Common for neutron-rich nuclei. The antineutrino carries away part of the kinetic energy, producing the continuous beta energy spectrum.
Beta-plus decay
A proton decays into a neutron plus a positron plus an electron neutrino. Common for proton-rich nuclei.
The positron annihilates with an electron, producing two MeV gamma photons in opposite directions. This is the basis of PET imaging.
Gamma emission
A nucleus in an excited state drops to a lower state by emitting a gamma photon. and are unchanged.
Often follows alpha or beta decay (the daughter is left in an excited state).
Conservation in nuclear equations
Always conserve:
- Mass number (total nucleons).
- Atomic number (total charge).
- Lepton number (electron + neutrino vs positron + antineutrino).
Energy, momentum and angular momentum are also conserved, but VCE Year 11 questions focus on and .
VCAA exam style
Year 11 SAC tasks include:
- Identifying the decay mode from a parent and daughter pair.
- Writing balanced equations.
- Identifying stable vs unstable isotopes from a chart of nuclides.
Common traps
Wrong direction in beta decay. Beta-minus increases (extra proton). Beta-plus decreases .
Treating gamma emission as changing the element. Gamma keeps both and unchanged.
Forgetting the (anti)neutrino. For full marks, include it. The antineutrino in beta-minus accompanies the electron; the neutrino in beta-plus accompanies the positron.
In one sentence
Atomic nuclei contain protons and neutrons bound by the short-range strong force, with stability determined by the neutron-to-proton ratio; unstable nuclei decay by alpha (, ), beta-minus (, neutron proton plus electron plus antineutrino), beta-plus (, proton neutron plus positron plus neutrino) or gamma (no / change) emission, and every decay equation must conserve mass number and atomic number.
Past exam questions, worked
Real questions from past VCAA papers on this dot point, with our answer explainer.
Year 11 SAC4 marksCarbon-14 ($^{14}_6$C) undergoes beta-minus decay. (a) Write the balanced equation. (b) Identify the daughter nucleus and explain the conservation laws applied.Show worked answer β
(a) Balanced equation.
(b) Daughter and conservation.
Daughter nucleus: nitrogen-14.
Conservation: mass number () and atomic number () are both conserved. Charge is conserved (the antineutrino is neutral). Energy and momentum are conserved (shared between the beta particle and the antineutrino, explaining the continuous beta energy spectrum).
Markers reward conservation of and in the equation, the daughter named explicitly, and inclusion of the antineutrino.
Related dot points
- Solve problems involving exponential decay and half-life ($N = N_0 (\tfrac{1}{2})^{t/T_{1/2}}$), and apply to dating techniques (carbon-14, uranium-lead) and nuclear medicine (technetium-99m, iodine-131)
A focused answer to the VCE Physics Unit 1 dot point on half-life and applications. Applies the integer half-life formula $N = N_0 (1/2)^n$ and the continuous form $N = N_0 e^{-\lambda t}$ with $\lambda = \ln 2 / T_{1/2}$, and works the VCAA SAC-style carbon-14 dating and Tc-99m medical-isotope problems.
- Atomic nucleus structure (protons, neutrons), isotopes, types of radioactive decay (alpha, beta, gamma), nuclear stability, half-life, fission and fusion, and applications including nuclear power
A focused answer to the VCE Physics Unit 1 key knowledge point on nuclear physics. Atomic structure (Z, N, A), alpha, beta and gamma decay, half-life $N = N_0 (1/2)^{t/T_{1/2}}$, nuclear stability, fission, fusion, and applications in nuclear power and medicine.
- Explain temperature in terms of the average translational kinetic energy of particles ($\bar{E}_k = \frac{3}{2} k_B T$), distinguishing absolute (kelvin) and celsius temperature scales
A focused answer to the VCE Physics Unit 1 dot point on the kinetic theory of temperature. Defines temperature as proportional to the average translational kinetic energy of particles, applies $\bar{E}_k = \frac{3}{2}k_B T$ in kelvin, and works the VCAA SAC-style problem on doubling absolute temperature and predicting molecular speeds.