Half-life is an essential concept in radioactive decay. It represents the time required for half of the radioactive nuclei in a sample to decay. This doesn't mean that after one half-life all of the nuclei are gone; instead, the process is exponential. Each half-life results in half of the remaining radioactive atoms decaying, but the other half stays intact.
For example, if you start with 100 nuclei, after one half-life, 50 would remain. After two half-lives, 25 would remain, and so on. It’s a continuous and ongoing process. This characteristic makes half-life a reliable way to predict how long a radioactive material will remain active and how it will decrease over time.
Half-life is calculated using the decay constant, with the formula:
- \[T = \frac{\ln 2}{\lambda}\]
where \(T\) is the half-life and \(\lambda\) is the decay constant.
The half-life of a material such as Americium-241 is crucial because it helps us understand the timeframe over which the material will remain active, like in smoke detectors.