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    Nuclear decay — Eduqas A-Level Physics

    Test yourself on Nuclear decay with EDUQAS A-Level practice questions.

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    Nuclear decay explained

    This topic covers the physical and mathematical treatment of undamped simple harmonic motion (SHM).

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    It investigates the energy interchanges during SHM, the effects of damping, and the phenomena of forced oscillations and resonance in real systems.

    What to demonstrate

    1. Definition of simple harmonic motion as a statement in words
    2. Mathematical defining equation a = -ω²x
    3. Graphical representation of acceleration vs displacement
    Show all 15 objectives
    1. Solution x = A cos(ωt + φ)
    2. Definitions of frequency, period, amplitude, and phase
    3. Period T = 1/f or T = 2π/ω
    4. Velocity v = -Aω sin(ωt + φ)
    5. Period of a system with stiffness k and mass m: T = 2π√(m/k)
    6. Period of a simple pendulum: T = 2π√(l/g)
    7. Energy interchange between kinetic and potential energy
    8. Free oscillations and the effect of damping
    9. Importance of critical damping in systems like vehicle suspensions
    10. Forced oscillations and resonance
    11. Variation of amplitude with driving frequency and the effect of damping on resonance curves
    12. Practical examples of useful resonance (e.g., circuit tuning) and avoidable resonance (e.g., bridge design)

    Nuclear decay exam tips

    Topic Overview

    Nuclear decay is the process by which unstable atomic nuclei lose energy by emitting radiation. This topic is central to nuclear physics and covers the three main types of decay: alpha, beta, and gamma. Each type involves different particles and has distinct properties, such as ionising power and penetration depth. Understanding nuclear decay is essential for explaining natural radioactivity, nuclear reactions, and applications like medical imaging and carbon dating.

    In the WJEC A-Level Physics syllabus, nuclear decay builds on atomic structure and introduces key concepts such as decay equations, half-life, and the random nature of decay. You will learn to write balanced nuclear equations, calculate decay constants, and use exponential decay models. This topic also links to energy-mass equivalence (E=mc²) and the stability of nuclei, providing a foundation for more advanced topics like nuclear fission and fusion.

    Mastering nuclear decay is not just about memorising facts; it requires applying mathematical models to real-world scenarios. For example, you might calculate the age of an archaeological sample using carbon-14 dating or determine the activity of a radioactive source. These skills are highly valued in exams and demonstrate a deep understanding of how the physical world operates at the nuclear level.

    Key Concepts
    • →Alpha decay: emission of an alpha particle (helium nucleus, 2 protons + 2 neutrons), resulting in a daughter nucleus with atomic number decreased by 2 and mass number decreased by 4.
    • →Beta-minus decay: a neutron converts into a proton, emitting an electron and an antineutrino; atomic number increases by 1, mass number unchanged.
    • →Gamma decay: emission of high-energy photons from an excited nucleus, often following alpha or beta decay; no change in atomic or mass number.
    • →Half-life: the time taken for half the radioactive nuclei in a sample to decay; it is constant for a given isotope and independent of initial quantity.
    • →Exponential decay law: N = N₀ e^(-λt), where N is the number of undecayed nuclei, λ is the decay constant, and t is time.
    Marking Points
    • Definition of simple harmonic motion as a statement in words
    • Mathematical defining equation a = -ω²x
    • Graphical representation of acceleration vs displacement
    • Solution x = A cos(ωt + φ)
    • Definitions of frequency, period, amplitude, and phase
    • Period T = 1/f or T = 2π/ω
    • Velocity v = -Aω sin(ωt + φ)
    • Period of a system with stiffness k and mass m: T = 2π√(m/k)
    • Period of a simple pendulum: T = 2π√(l/g)
    • Energy interchange between kinetic and potential energy
    • Free oscillations and the effect of damping
    • Importance of critical damping in systems like vehicle suspensions
    • Forced oscillations and resonance
    • Variation of amplitude with driving frequency and the effect of damping on resonance curves
    • Practical examples of useful resonance (e.g., circuit tuning) and avoidable resonance (e.g., bridge design)
    Examiner Tips
    • 💡Always ensure your calculator is in the correct mode (radians or degrees) when using trigonometric functions for SHM equations
    • 💡When drawing graphs of displacement, velocity, or acceleration against time, ensure the phase relationships are correct
    • 💡Use fiducial markers when timing oscillations to improve accuracy
    • 💡Remember that the area under a force-extension graph represents energy stored
    • 💡Be prepared to explain the importance of critical damping in real-world applications like car suspensions
    • 💡Always write balanced nuclear equations with correct notation: superscript for mass number, subscript for atomic number. For example, ²³⁸₉₂U → ²³⁴₉₀Th + ⁴₂He. Check that mass and atomic numbers balance on both sides.
    • 💡When calculating half-life from a graph, use the exponential decay curve. Pick a point where the activity or count rate is exactly half of an earlier value, and read the time difference. Avoid using the initial point if the graph is noisy.
    • 💡For questions involving decay constant λ, remember the relationship λ = ln2 / t₁/₂. Ensure units are consistent (e.g., λ in s⁻¹ if half-life is in seconds). Show all working, including the substitution into the exponential decay formula.
    Common Mistakes
    • Confusing the period of a simple pendulum with that of a mass-spring system
    • Incorrectly applying the small angle approximation for pendulums
    • Failing to account for the phase difference between displacement and velocity graphs
    • Misinterpreting the effect of damping on the sharpness of resonance curves
    • Confusing free oscillations with forced oscillations
    • Misconception: Alpha particles are the most dangerous because they have the most mass. Correction: While alpha particles are highly ionising, they are easily stopped by a sheet of paper or skin. They are only dangerous if ingested or inhaled, as they can cause significant internal damage.
    • Misconception: Half-life means the time for all nuclei to decay. Correction: Half-life is the time for half the nuclei to decay, not all. After two half-lives, one quarter remains, and so on. The decay continues indefinitely, though the number becomes negligible.
    • Misconception: Beta particles are electrons from the electron cloud. Correction: Beta particles are electrons emitted from the nucleus during beta decay, not from the electron cloud. They are produced when a neutron transforms into a proton.
    Frequently Asked Questions
    What is the difference between alpha, beta, and gamma radiation?
    Alpha radiation consists of helium nuclei (2 protons, 2 neutrons) and is highly ionising but weakly penetrating (stopped by paper). Beta radiation consists of fast-moving electrons (or positrons) and is moderately ionising and penetrating (stopped by a few mm of aluminium). Gamma radiation is electromagnetic waves (photons) with high energy, low ionising power, and high penetration (requires thick lead or concrete to stop).
    How do you calculate the half-life from experimental data?
    Plot a graph of activity (or count rate) against time. The half-life is the time taken for the activity to fall to half its initial value. Alternatively, use the exponential decay equation: N = N₀ e^(-λt). Take natural logs: ln(N) = ln(N₀) - λt. The gradient of a ln(N) vs t graph gives -λ, and half-life t₁/₂ = ln2 / λ.
    Why is nuclear decay random?
    Nuclear decay is random because it is impossible to predict when a particular nucleus will decay. The decay process is governed by quantum mechanics, and each unstable nucleus has a constant probability of decaying per unit time, independent of its history or external conditions. This randomness leads to the exponential decay law.
    What is the decay constant and how is it related to half-life?
    The decay constant (λ) is the probability per unit time that a given nucleus will decay. It is related to half-life (t₁/₂) by the equation λ = ln2 / t₁/₂. A larger decay constant means a shorter half-life, so the substance decays more quickly.
    How does carbon-14 dating work?
    Carbon-14 is a radioactive isotope with a half-life of 5730 years. It is produced in the atmosphere and taken up by living organisms. When an organism dies, it stops absorbing carbon-14, and the existing carbon-14 decays. By measuring the remaining carbon-14 in a sample and comparing it to the initial amount (assumed constant in the atmosphere), the time since death can be calculated using the exponential decay formula.
    What is the difference between activity and count rate?
    Activity is the number of decays per second in a radioactive source, measured in becquerels (Bq). Count rate is the number of decays detected per second by a detector, which is usually less than the activity due to detector efficiency and geometry. In calculations, count rate is often proportional to activity, so the same exponential decay laws apply.