Radioactive Decay — Question 1

Section 42-3 · Physics pages 7032–7033

Question 1 Constant decay probability produces exponential survival Each undecayed nucleus has probability λ dt of decaying in a short interval dt, independent of its age. A sample initially contains N0 nuclei. λt N/N0 Schematic; labels, not drawing lengths, specify the data. (a) Derive the population law and half-life. (b) Find the fraction that decays between one and three half-lives, and the time required for 99 percent to decay.
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Question 1 - Solution Constant decay probability produces exponential survival λt N/N0 (a) Method and calculation dN = −λNdt ⇒ ∫N N0 dN′ N′ = −λt ⇒N = N0e−λt . N(T1/2) = N0/2 ⇒T1/2 = ln 2/λ . (b) Interpretation and further calculation [N(T1/2) −N(3T1/2)]/N0 = 1/2 −1/8 = 3/8 . t99 = ln 100/λ = 6.644T1/2 . Physical check The probability per unit time is constant, but the number of decays per unit time decreases because fewer parent nuclei remain.

Question 1

Constant decay probability produces exponential survival

Each undecayed nucleus has probability λdt\lambda\,dt of decaying in a short interval dt, independent of its age. A sample initially contains N0N_0 nuclei.

Diagram shown in the original SVG worksheet.

  1. Derive the population law and half-life.

  2. Find the fraction that decays between one and three half-lives, and the time required for 99 percent to decay.

Question 1 - Solution

Constant decay probability produces exponential survival

Diagram shown in the original SVG worksheet.

(a) Method and calculation

dN=−λNdt⇒∫N0NdN′N′=−λt⇒N=N0e−λt.dN=-\lambda Ndt\Rightarrow\int_{N_0}^N\frac{dN\prime}{N\prime}=-\lambda t\Rightarrow\boxed{N=N_0e^{-\lambda t}}.N(T1/2)=N0/2⇒T1/2=ln⁡2/λ.N(T_{1/2})=N_0/2\Rightarrow\boxed{T_{1/2}=\ln2/\lambda}.

(b) Interpretation and further calculation

[N(T1/2)−N(3T1/2)]/N0=1/2−1/8=3/8.\boxed{[N(T_{1/2})-N(3T_{1/2})]/N_0=1/2-1/8=3/8}.t99=ln⁡100/λ=6.644T1/2.\boxed{t_{99}=\ln100/\lambda=6.644T_{1/2}}.

Physical check

The probability per unit time is constant, but the number of decays per unit time decreases because fewer parent nuclei remain.