Year 13
Side A3: Nuclear & Quantum
Develop modern physics through radioactivity, binding energy, photons, and wave-particle ideas.
Part of Year 13 CIE Physics 9702.
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.
Topic revision route
Use the generated links below to move from lesson review to retrieval practice, syllabus checks, and useful resources.
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
A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.
de Broglie wavelength
A definition has not been added for this term yet. Use the lesson sequence below to review where it appears.
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
CIE 9702 coverage in this topic
30 points across 8 lessons
understand that electromagnetic radiation has a particulate nature
understand that a photon is a quantum of electromagnetic energy
recall and use E = hf
use the electronvolt (eV) as a unit of energy
understand that a photon has momentum and that the momentum is given by p = E / c
understand that photoelectrons may be emitted from a metal surface when it is illuminated by electromagnetic radiation
understand and use the terms threshold frequency and threshold wavelength
explain photoelectric emission in terms of photon energy and work function energy 1
recall and use hf = Φ + 2 mvmax2
explain why the maximum kinetic energy of photoelectrons is independent of intensity, whereas the photoelectric current is proportional to intensity
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
describe and interpret qualitatively the evidence provided by electron diffraction for the wave nature of particles
understand the de Broglie wavelength as the wavelength associated with a moving particle
recall and use λ = h / p
understand that there are discrete electron energy levels in isolated atoms (e.g. atomic hydrogen)
understand the appearance and formation of emission and absorption line spectra
recall and use hf = E1 – E2
understand the equivalence between energy and mass as represented by E = mc2 and recall and use this equation
represent simple nuclear reactions by nuclear equations of the form 147 N + 24 He " 178 O + 11 H
define and use the terms mass defect and binding energy
sketch the variation of binding energy per nucleon with nucleon number
explain what is meant by nuclear fusion and nuclear fission
explain the relevance of binding energy per nucleon to nuclear reactions, including nuclear fusion and nuclear fission
calculate the energy released in nuclear reactions using E = c2∆ m
understand that fluctuations in count rate provide evidence for the random nature of radioactive decay
understand that radioactive decay is both spontaneous and random
define activity and decay constant, and recall and use A = λN
define half-life
use λ = 0.693 / t 1 2
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
Lesson sequence
Open lesson pages for summaries, objectives, notes, and linked resources. Test lessons stay locked for now.
Lesson
01Radioactivity and Half Life
Introduce radioactive decay patterns and half-life calculations.
Lesson
02Nuclear Physics, Binding Energy
Develop nuclear models and binding energy calculations.
Lesson
03Photoelectric Effect
Use the photoelectric effect as evidence for quantum behaviour.
Lesson
04Energy Levels in Atoms and Line Spectra
Link atomic energy levels to emission and absorption spectra.
Lesson
05Wave Particle Duality
Develop the wave-particle model for matter and radiation.
Lesson
06Revision
Consolidate nuclear and quantum physics before assessment.
Lesson
07Test
Assess the nuclear and quantum physics topic.
Lesson
08Review
Review errors and strengthen understanding after the topic test.