Topic Overview

What students will cover

This topic groups the major Year 13 modern physics ideas so you can move from nuclear models into quantum evidence without losing the overall thread.

You begin with radioactive decay and half-life, then use mass-energy equivalence to explain nuclear binding energy and energy release. The quantum lessons use the photoelectric effect, atomic spectra, and electron diffraction to build the evidence for photons, discrete energy levels, and matter waves before you consolidate the topic through revision and review.

Revision

Topic revision route

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Recall vocabulary

  • Activity

    the rate of decay of nuclei in a radioactive sample.

  • Decay constant

    the probability per unit time that an individual nucleus will decay.

  • Half-life

    the time taken for the number of undecayed nuclei, or the activity, to fall to half its initial value.

  • Mass defect

    the difference between the mass of a nucleus and the total mass of its separate nucleons.

  • Binding energy

    the energy required to separate a nucleus into its individual nucleons.

  • work function

    A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.

  • threshold frequency

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  • photoelectron

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  • energy level

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  • line spectrum

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  • electron diffraction

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  • de Broglie wavelength

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  • radioactive decay

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  • exponential decay

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  • binding energy per nucleon

    A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.

  • Nuclear fission

    the splitting of a heavy nucleus into two or more smaller nuclei.

  • Nuclear fusion

    the joining of light nuclei to form a heavier nucleus.

  • photoelectric effect

    A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.

Resource bank

Lesson resources
6
Topic resources
0

Open the relevant lesson first, then use its linked slides, worksheets, simulations, or practice tasks.

Syllabus

CIE 9702 coverage in this topic

30 points across 8 lessons

Show details
22.1.1

understand that electromagnetic radiation has a particulate nature

22.1.2

understand that a photon is a quantum of electromagnetic energy

22.1.4

use the electronvolt (eV) as a unit of energy

22.1.5

understand that a photon has momentum and that the momentum is given by p = E / c

22.2.1

understand that photoelectrons may be emitted from a metal surface when it is illuminated by electromagnetic radiation

22.2.2

understand and use the terms threshold frequency and threshold wavelength

22.2.3

explain photoelectric emission in terms of photon energy and work function energy 1

22.2.4

recall and use hf = Φ + 2 mvmax2

22.2.5

explain why the maximum kinetic energy of photoelectrons is independent of intensity, whereas the photoelectric current is proportional to intensity

22.3.1

understand that the photoelectric effect provides evidence for a particulate nature of electromagnetic radiation while phenomena such as interference and diffraction provide evidence for a wave nature

22.3.2

describe and interpret qualitatively the evidence provided by electron diffraction for the wave nature of particles

22.3.3

understand the de Broglie wavelength as the wavelength associated with a moving particle

22.4.1

understand that there are discrete electron energy levels in isolated atoms (e.g. atomic hydrogen)

22.4.2

understand the appearance and formation of emission and absorption line spectra

23.1.1

understand the equivalence between energy and mass as represented by E = mc2 and recall and use this equation

23.1.2

represent simple nuclear reactions by nuclear equations of the form 147 N + 24 He " 178 O + 11 H

23.1.3

define and use the terms mass defect and binding energy

23.1.4

sketch the variation of binding energy per nucleon with nucleon number

23.1.5

explain what is meant by nuclear fusion and nuclear fission

23.1.6

explain the relevance of binding energy per nucleon to nuclear reactions, including nuclear fusion and nuclear fission

23.1.7

calculate the energy released in nuclear reactions using E = c2∆ m

23.2.1

understand that fluctuations in count rate provide evidence for the random nature of radioactive decay

23.2.2

understand that radioactive decay is both spontaneous and random

23.2.3

define activity and decay constant, and recall and use A = λN

23.2.6

understand the exponential nature of radioactive decay, and sketch and use the relationship x = x0e –λt, where x could represent activity, number of undecayed nuclei or received count rate

Lessons

Lesson sequence

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