Randomness and Probability: Radioactive decay is a stochastic process. It is impossible to predict exactly when a specific nucleus will decay, but for a large population, the probability of decay remains constant.
Independence of External Conditions: The half-life of an isotope is an intrinsic property. It is not affected by physical changes (like temperature or pressure) or chemical changes (like bonding or state of matter).
The 'Never Zero' Principle: Because the amount of radioactive material halves in each period, the quantity theoretically never reaches zero. In practice, after many half-lives, the activity becomes indistinguishable from background radiation.
| Feature | Activity | Half-Life |
|---|---|---|
| Definition | Rate of decay (decays per second) | Time taken for activity to halve |
| Unit | Becquerels (Bq) | Seconds, Hours, Years, etc. |
| Change over time | Decreases as the sample decays | Remains constant for the isotope |
| Dependency | Depends on the number of nuclei present | Independent of the sample size |
Check the Units: Always ensure the time units on the x-axis match the units requested in the answer (e.g., converting days to hours if necessary).
Background Radiation: In practical scenarios, detectors measure 'total count rate'. You must subtract the background radiation count before calculating the half-life to get the corrected count rate.
Multiple Halvings: To increase accuracy when reading a graph, check the time it takes to drop from to , and then from to . These intervals should be identical; averaging them reduces reading errors.
Sanity Check: If a question asks for the amount remaining after 3 half-lives, your answer must be exactly (or ) of the starting value. If your calculated value is higher than the starting value, you have likely multiplied where you should have divided.