Understanding Radioactive Decay
Radioactivity is a fascinating phenomenon where unstable atomic nuclei release energy by emitting radiation. To quantify how quickly a radioactive substance decays, we use a parameter called the decay constant, denoted by λ. This constant represents the probability of decay per unit time for a single nucleus.
The Concept of Half-Life
Imagine you have a large sample of radioactive atoms. You might wonder, "How long will it take for exactly half of these atoms to decay?" This specific duration is known as the half-life (T1/2).
Mathematically, the radioactive decay law is given by:
N(t)=N0e−λt
where
N0 is the initial number of nuclei and
N(t) is the number of nuclei remaining at time
t.
To find the half-life, we set
N(t)=2N0:
2N0=N0e−λT1/2
Taking the natural logarithm on both sides:
ln(21)=−λT1/2
This formula beautifully connects the macroscopic observable (half-life) with the microscopic probability (decay constant).
The Concept of Mean-Life
While half-life is incredibly useful, physicists also use another measure called the mean-life (τ). Think of it as the average lifespan of all the radioactive nuclei in the sample. Some nuclei will decay almost immediately, while others might survive for a very long time. If you were to average the lifetimes of every single nucleus, you would get the mean-life.
Through integration of the decay probability over all time from zero to infinity, the mean-life is calculated as the reciprocal of the decay constant:
τ=λ1
Conclusion
By comparing the two derived expressions, we can clearly see the relationship between them. The half-life is λln2 and the mean-life is λ1. Since ln2≈0.693, the half-life is approximately 69.3% of the mean-life.
Returning to our question, we are asked for the half-life and mean-life respectively. The correct pair is λln2 and λ1, which corresponds to option (b).