The Mathematics of Radioactive Decay
Radioactive decay is a fascinating natural phenomenon where unstable atomic nuclei lose energy by emitting radiation. But how do we quantify this process?
The fundamental law of radioactive decay states that the rate of decay is proportional to the number of undecayed nuclei present. This gives rise to the famous exponential decay formula:
where N(t) is the number of active nuclei at time t, N0 is the initial number of nuclei, and λ is the decay constant.
Tracking the Decayed Nuclei
While N(t) tells us what remains, we are often interested in what has already decayed.
By the principle of conservation of mass, the number of decayed nuclei Nd(t) is simply the initial amount minus the remaining amount:
Nd(t)=N0−N(t)=N0(1−e−λt)
This equation shows that as time progresses, the number of decayed nuclei grows, asymptotically approaching the initial number N0.
The Fraction of Decay
The problem introduces a variable f, defined as the ratio of decayed nuclei to the initial number of nuclei.
This is a dimensionless fraction that tells us the progress of the decay process:
At t=0, f=0 because nothing has decayed yet. As t→∞, f→1 meaning everything has decayed.
Finding the Rate of Change
To find how fast this fraction is changing, we need to differentiate f with respect to time t.
This requires a basic application of calculus, specifically the chain rule for exponential functions:
The derivative of the constant 1 is 0. For the exponential term, the derivative of e−λt is −λe−λt.
Carefully managing the negative signs, we get:
This result is profoundly elegant. It tells us that the rate at which the decayed fraction grows is directly proportional to the fraction of nuclei that are still active.
As the active pool depletes, the rate of new decays slows down. The final answer is λe−λt.