Published by Patrick Mutisya · 14 days ago
To define the concept of half‑life and understand how it is used to describe radioactive decay.
Radioactive decay is a random process by which an unstable nucleus transforms into a more stable configuration, emitting particles or electromagnetic radiation. The number of undecayed nuclei, \$N\$, decreases exponentially with time.
The rate of decay is proportional to the number of nuclei present:
\$\frac{dN}{dt} = -\lambda N\$
where \$\lambda\$ is the decay constant (s\(^{-1}\)). Integrating gives the exponential law:
\$N(t) = N_0 e^{-\lambda t}\$
\$N_0\$ is the initial number of nuclei at \$t = 0\$.
The half‑life, denoted \$t{1/2}\$, is the time required for half of the original nuclei to decay. Mathematically it is defined by the condition \$N(t{1/2}) = \frac{1}{2}N_0\$.
Substituting into the exponential law:
\$\frac{1}{2}N0 = N0 e^{-\lambda t_{1/2}}\$
Solving for \$t_{1/2}\$ yields:
\$t_{1/2} = \frac{\ln 2}{\lambda} \approx \frac{0.693}{\lambda}\$
| Radionuclide | Decay Mode | Half‑life |
|---|---|---|
| Carbon‑14 | β‑decay | 5,730 years |
| Iodine‑131 | β‑decay | 8.0 days |
| Uranium‑238 | α‑decay | 4.5 × 10⁹ years |
| Polonium‑212 | α‑decay | 0.3 µs |