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Nuclear Reactions: Fission, Fusion, and Binding Energy

Properties of the Nucleus
4 · From the Universe to the Atom

What this note covers

  1. Mass Defect and the Origin of Nuclear Binding Energy
  2. Worked Example 1 — Mass Defect and Binding Energy of Helium-4
  3. Binding Energy Per Nucleon Curve and Nuclear Stability
  4. Balancing Nuclear Equations — Conservation Laws
  5. Worked Example 2 — Deuterium–Tritium Fusion Energy Calculation
  6. Fission vs Fusion: Energy Comparison and Physical Context
  7. Conservation of Mass-Energy in Nuclear Reactions: The Complete Picture

7 sections · 14 key terms & formulas · 6 common mistakes

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HSC Physics · revision note 11 of 20