Nuclear Physics & Radioactivity cheat sheet - grade 11-12

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Physics Grade 11-12

Nuclear Physics & Radioactivity Cheat Sheet

A printable reference covering nuclear notation, radioactive decay, half-life, activity, binding energy, mass defect, and nuclear reactions for grades 11-12.

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Nuclear physics studies the structure, stability, and transformations of atomic nuclei. This cheat sheet helps students track nuclear symbols, balance decay equations, and connect radioactive decay to measurable quantities. It is especially useful for solving half-life, activity, binding energy, and reaction energy problems in grade 11 and 12 physics. The most important ideas are conservation of nucleon number, conservation of charge, and exponential decay. Radioactive samples follow N=N0eλtN = N_0 e^{-\lambda t}, with half-life given by T1/2=ln2λT_{1/2} = \frac{\ln 2}{\lambda}. Nuclear energy calculations use mass defect and Einstein’s relation E=Δmc2E = \Delta m c^2, often expressed using 1u=931.5MeV/c21\,\mathrm{u} = 931.5\,\mathrm{MeV}/c^2.

Key Facts

  • A nuclide is written as ZAX^{A}_{Z}\mathrm{X}, where AA is the mass number, ZZ is the atomic number, and the number of neutrons is N=AZN = A - Z.
  • In every nuclear reaction, total mass number and total atomic number are conserved, so Areactants=Aproducts\sum A_{\text{reactants}} = \sum A_{\text{products}} and Zreactants=Zproducts\sum Z_{\text{reactants}} = \sum Z_{\text{products}}.
  • Alpha decay emits 24He^{4}_{2}\mathrm{He}, so a parent nucleus changes according to ZAXZ2A4Y+24He^{A}_{Z}\mathrm{X} \rightarrow ^{A-4}_{Z-2}\mathrm{Y} + ^{4}_{2}\mathrm{He}.
  • Beta-minus decay emits an electron and an antineutrino, so ZAXZ+1AY+10e+νˉ^{A}_{Z}\mathrm{X} \rightarrow ^{A}_{Z+1}\mathrm{Y} + ^{0}_{-1}e + \bar{\nu}.
  • Beta-plus decay emits a positron and a neutrino, so ZAXZ1AY++10e+ν^{A}_{Z}\mathrm{X} \rightarrow ^{A}_{Z-1}\mathrm{Y} + ^{0}_{+1}e + \nu.
  • Radioactive decay follows N=N0eλtN = N_0 e^{-\lambda t}, where NN is the number of undecayed nuclei, N0N_0 is the initial number, and λ\lambda is the decay constant.
  • Half-life and decay constant are related by T1/2=ln2λT_{1/2} = \frac{\ln 2}{\lambda}, and after nn half-lives the remaining amount is N=N0(12)nN = N_0\left(\frac{1}{2}\right)^n.
  • Nuclear binding energy is found from Eb=Δmc2E_b = \Delta m c^2, where the mass defect is Δm=Zmp+Nmnmnucleus\Delta m = Zm_p + Nm_n - m_{\text{nucleus}}.

Vocabulary

Nuclide
A specific nucleus identified by its number of protons ZZ and total nucleons AA.
Isotope
Atoms of the same element with the same ZZ but different neutron numbers NN.
Half-life
The time T1/2T_{1/2} required for half of the radioactive nuclei in a sample to decay.
Activity
The decay rate of a radioactive sample, given by Aact=λNA_{\text{act}} = \lambda N.
Mass defect
The missing mass Δm\Delta m between separate nucleons and the actual nucleus, converted into binding energy.
Binding energy
The energy EbE_b required to completely separate a nucleus into individual protons and neutrons.

Common Mistakes to Avoid

  • Forgetting to conserve both AA and ZZ is wrong because nuclear equations must balance nucleon number and charge separately.
  • Confusing half-life with decay constant is wrong because T1/2T_{1/2} is a time while λ\lambda is a probability per unit time, related by T1/2=ln2λT_{1/2} = \frac{\ln 2}{\lambda}.
  • Using linear subtraction for radioactive decay is wrong because radioactive decay is exponential, so the correct model is N=N0eλtN = N_0 e^{-\lambda t} or N=N0(12)nN = N_0\left(\frac{1}{2}\right)^n.
  • Treating gamma emission as a change in atomic number is wrong because gamma decay releases energy but leaves AA and ZZ unchanged.
  • Using atomic masses without checking electrons is wrong because mass defect calculations require consistent masses, either all nuclear masses or correctly balanced atomic masses.

Practice Questions

  1. 1 Complete the alpha decay equation: 92238U?+24He^{238}_{92}\mathrm{U} \rightarrow ? + ^{4}_{2}\mathrm{He}.
  2. 2 A sample has N0=6.4×1015N_0 = 6.4 \times 10^{15} nuclei and a half-life of 8.0h8.0\,\mathrm{h}. How many nuclei remain after 24.0h24.0\,\mathrm{h}?
  3. 3 A radioactive isotope has λ=2.31×105s1\lambda = 2.31 \times 10^{-5}\,\mathrm{s}^{-1} and N=3.0×1012N = 3.0 \times 10^{12} nuclei. Find its activity using Aact=λNA_{\text{act}} = \lambda N.
  4. 4 Explain why nuclei with higher binding energy per nucleon are generally more stable than nuclei with lower binding energy per nucleon.