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Physics (AS & A Level) 9702 · Chapter 23

Nuclear physics

Mass-energy equivalence, nuclear equations, mass defect and binding energy, binding energy per nucleon, fusion and fission, the random nature of decay, activity and the decay constant, half-life, and exponential decay.

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23.1 Mass defect and nuclear binding energy

Mass and energy

Mass and energy are equivalent:

E=mc2E = mc^2

So a change in energy means a change in mass: ΔE=c2Δm\Delta E = c^2\Delta m. A nuclear reaction that releases energy leaves the products with less total mass.

Nuclear equations

Nucleon number and proton number balance on both sides:

714N+24He→ 817O+11H^{14}_{7}\text{N} + ^{4}_{2}\text{He} \rightarrow\, ^{17}_{8}\text{O} + ^{1}_{1}\text{H}

Mass defect and binding energy

  • Mass defect: the difference between the total mass of the separate nucleons and the mass of the nucleus. The nucleus is always lighter.
  • Binding energy: the energy needed to separate a nucleus completely into its individual nucleons. It equals c2c^2 × the mass defect.

Binding energy per nucleon

A graph of binding energy per nucleon against nucleon number, rising steeply to a peak at iron and falling slowly

A graph of binding energy per nucleon against nucleon number, rising steeply to a peak at iron and falling slowly

A higher binding energy per nucleon means a more stable nucleus. The peak is near iron-56.

Fusion and fission

FusionFission
What happenstwo light nuclei joina heavy nucleus splits into two lighter ones and some neutrons
Where on the curveleft of the peakright of the peak
Examplehydrogen to helium in starsuranium-235 in a reactor

Fusion needs very high temperatures, so that the positive nuclei are moving fast enough to overcome their electrostatic repulsion.

23.2 Radioactive decay

Spontaneous and random

  • Random: you cannot predict which nucleus will decay next or when, though each one has a constant probability per unit time.
  • Spontaneous: decay is not affected by external factors such as temperature or pressure.

The fluctuations in the count rate from a radioactive source are evidence for its randomness.

Activity and the decay constant

Activity AA is the number of decays per unit time, measured in becquerels (1 Bq = 1 decay per second).

The decay constant λ\lambda is the probability per unit time that a nucleus will decay.

A=λNA = \lambda N

Half-life

Half-life t1/2t_{1/2} is the time taken for the number of undecayed nuclei of a nuclide (or the activity) to fall to half.

λ=ln⁡2t1/2=0.693t1/2\lambda = \frac{\ln 2}{t_{1/2}} = \frac{0.693}{t_{1/2}}

Exponential decay

x=x0e−λtx = x_0 e^{-\lambda t}

where xx can be the activity, the number of undecayed nuclei, or the received count rate.

An exponential decay curve of the number of undecayed nuclei against time, halving every half-life

An exponential decay curve of the number of undecayed nuclei against time, halving every half-life

Taking logs gives ln⁡A=ln⁡A0−λt\ln A = \ln A_0 - \lambda t. So a plot of ln⁡A\ln A against tt is a straight line with gradient −λ-\lambda.

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