168–170, 172–173Nuclear PhysicsStretch

Radioactive Decay and Half-Life

You cannot predict when a single unstable nucleus will decay. Yet a sample of billions decays with such regularity that its activity can date a 4000-year-old skeleton. Radioactive decay\textbf{Radioactive decay} is random for individual nuclei and exponential for large numbers.

40 min Topic 11 · Nuclear Radiation

What you'll be able to do

  • Describe alpha, beta and gamma radiation, and write balanced decay equations
  • Explain the random and spontaneous nature of radioactive decay
  • Use A=λNA = \lambda N and N=N0e−λtN = N_{0}e^{-\lambda t}
  • Define half-life and use λt1/2=ln⁡2\lambda t_{1/2} = \ln 2
1

Types of radiation

Alpha\textbf{Alpha} (α\alpha) particles are helium nuclei, 24He^{4}_{2}\mathrm{He}. They are strongly ionising, travel a few centimetres in air and are stopped by paper.

Beta-minus\textbf{Beta-minus} (β−\beta^{-}) particles are fast electrons emitted when a neutron becomes a proton. They are moderately ionising, travel about a metre in air and are stopped by a few millimetres of aluminium.

Gamma\textbf{Gamma} (γ\gamma) rays are high-energy electromagnetic radiation emitted when a nucleus drops to a lower energy state. They are weakly ionising and are reduced, not stopped, by thick lead.

In a decay equation, both nucleon number and proton number must balance. Alpha decay reduces AA by 4 and ZZ by 2; β−\beta^{-} decay leaves AA unchanged and increases ZZ by 1.

88226Ra→ 86222Rn+ 24α^{226}_{88}\mathrm{Ra} \rightarrow\ ^{222}_{86}\mathrm{Rn} +\ ^{4}_{2}\alpha
Alpha decay.
614C→ 714N+ −10β+νˉe^{14}_{6}\mathrm{C} \rightarrow\ ^{14}_{7}\mathrm{N} +\ ^{0}_{-1}\beta + \bar{\nu}_{e}
Beta-minus decay.

Tip — Background radiation is always present. Measure it first and subtract it from every count before analysing a source.

2

Random decay and activity

Decay is random\textbf{random} — you cannot predict which nucleus decays next or when — and spontaneous\textbf{spontaneous} — it is unaffected by temperature, pressure or chemical state.

The decay constant\textbf{decay constant} λ\lambda is the probability per unit time that a given nucleus decays, in s−1\mathrm{s^{-1}}.

The activity\textbf{activity} AA is the number of decays per second, in becquerels (Bq). With NN undecayed nuclei, A=λNA = \lambda N.

A=λN=−dNdtA = \lambda N = -\dfrac{\mathrm{d}N}{\mathrm{d}t}
Activity.
Example 1A sample contains 3.0×10153.0\times10^{15} nuclei with decay constant 2.0×10−9 s−12.0\times10^{-9}\ \mathrm{s^{-1}}. Find its activity.
1A=λN=2.0×10−9×3.0×1015A = \lambda N = 2.0\times10^{-9} \times 3.0\times10^{15}.
Answer6.0×106 Bq6.0\times10^{6}\ \mathrm{Bq}
3

The exponential law

Because the decay rate is proportional to NN, the number of undecayed nuclei falls exponentially. Activity, being proportional to NN, follows the same curve.

Taking natural logs, ln⁡N=ln⁡N0−λt\ln N = \ln N_{0} - \lambda t. A graph of ln⁡N\ln N or ln⁡A\ln A against tt is a straight line of gradient −λ-\lambda — the standard way to find the decay constant from experimental data.

N=N0e−λtN = N_{0}e^{-\lambda t}
Number of undecayed nuclei.
A=A0e−λtA = A_{0}e^{-\lambda t}
Activity.
Example 1A source has initial activity 800 Bq and λ=0.050 h−1\lambda = 0.050\ \mathrm{h^{-1}}. Find its activity after 24 hours.
1A=800e−0.050×24=800e−1.2A = 800e^{-0.050 \times 24} = 800e^{-1.2}.
2=800×0.3012= 800 \times 0.3012.
Answer240 Bq240\ \mathrm{Bq}

Tip — Keep λ\lambda and tt in matching units. Per hour with hours is fine; you only need s−1\mathrm{s^{-1}} when finding activity in Bq from λN\lambda N.

4

Half-life

The half-life\textbf{half-life} t1/2t_{1/2} is the time for the number of undecayed nuclei — or the activity — to halve. It is constant for a given isotope, whatever the starting amount.

Setting N=N0/2N = N_{0}/2 in the exponential law gives e−λt1/2=12e^{-\lambda t_{1/2}} = \tfrac12, so λt1/2=ln⁡2\lambda t_{1/2} = \ln 2.

After nn half-lives, the fraction remaining is (12)n(\tfrac12)^{n}. Medical tracers need half-lives of hours so they are detectable but do not linger; dating needs half-lives comparable to the age being measured.

λt1/2=ln⁡2\lambda t_{1/2} = \ln 2
Half-life and decay constant.
Example 1Carbon-14 has a half-life of 5730 years. A bone has 22% of the carbon-14 activity of living tissue. Estimate its age.
1λ=ln⁡2/5730=1.210×10−4 yr−1\lambda = \ln 2/5730 = 1.210\times10^{-4}\ \mathrm{yr^{-1}}.
20.22=e−λt0.22 = e^{-\lambda t}, so t=−ln⁡0.22λ=1.5141.210×10−4t = \dfrac{-\ln 0.22}{\lambda} = \dfrac{1.514}{1.210\times10^{-4}}.
AnswerAbout 1.25×1041.25\times10^{4} years.

Equation recap

A=λNA = \lambda N
Activity.
N=N0e−λtN = N_{0}e^{-\lambda t}
Exponential decay.
λt1/2=ln⁡2\lambda t_{1/2} = \ln 2
Half-life.

Common mistakes to avoid

Thinking after two half-lives none remains.
A quarter remains; decay never reaches exactly zero.
Mixing units of λ\lambda and tt.
Use consistent time units in the exponent.
Saying heating a source speeds up decay.
Decay is spontaneous and unaffected by physical conditions.
Unbalanced nucleon or proton numbers in decay equations.
Check both top and bottom numbers sum equally on each side.

Key takeaways

  • Alpha, beta and gamma differ in nature, ionising power and penetration.
  • Decay is random and spontaneous; activity A=λNA = \lambda N.
  • N=N0e−λtN = N_{0}e^{-\lambda t}; a ln⁡N\ln N–tt graph has gradient −λ-\lambda.
  • Half-life is constant, with λt1/2=ln⁡2\lambda t_{1/2} = \ln 2.
  • After nn half-lives, a fraction (12)n(\tfrac12)^{n} remains.

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