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Half-life

A single nucleus decays at a random moment — no one can predict which second. But a sample holds billions of nuclei, and statistics takes over: in a fixed time, always half of whatever is currently there decays. That fixed time is the half-life, t1/2t_{1/2}. Carbon-14’s is 5,730 years; fluorine-18’s is 110 minutes; uranium-238’s is 4.5 billion years. Same rule, wildly different clocks.

Everything below is one formula, used forwards and backwards:

N=N0(12)t/t1/2N = N_0 \left(\tfrac{1}{2}\right)^{t / t_{1/2}}

N0N_0 is what you start with, NN is what remains after time tt. The exponent n=t/t1/2n = t / t_{1/2} is simply the number of half-lives that elapsed — whole or fractional.

Worked problem 1 — whole half-lives, going forwards

Section titled “Worked problem 1 — whole half-lives, going forwards”

Start with 80 g80\ \mathrm{g} of carbon-14 (t1/2=5,730t_{1/2} = 5{,}730 years). How much remains after 17,19017{,}190 years?

First say it in words: each 5,730-year block halves whatever survived the previous block. Three blocks fit into 17,190 years, so the sample halves three times: 80→40→20→10 g80 \to 40 \to 20 \to 10\ \mathrm{g}.

As a formula: n=17,190/5,730=3n = 17{,}190 / 5{,}730 = 3, and N=80×(12)3=80×18=10 gN = 80 \times (\tfrac{1}{2})^3 = 80 \times \tfrac{1}{8} = 10\ \mathrm{g}.

The classic trap: if a half-life is 10 years, is everything gone after 20? No — after two half-lives 14\tfrac{1}{4} is still there (100→50→25100 \to 50 \to 25). Halving never reaches zero; it just keeps halving the remainder.

Try it. Iodine-131 (t1/2=8t_{1/2} = 8 days), 96 MBq96\ \mathrm{MBq} to start. After 24 days (n=3n = 3): 96×18=12 MBq96 \times \tfrac{1}{8} = 12\ \mathrm{MBq}.

Worked problem 2 — counting half-lives backwards

Section titled “Worked problem 2 — counting half-lives backwards”

A phosphorus-32 sample (t1/2=14t_{1/2} = 14 days) drops from 200200 counts/min to 2525. How much time passed?

Reason it out first: 2525 is 18\tfrac{1}{8} of 200200, and 18=(12)3\tfrac{1}{8} = (\tfrac{1}{2})^3, so three half-lives elapsed. Three blocks of 14 days is 3×14=423 \times 14 = 42 days.

In symbols: N/N0=25/200=0.125=(12)nN/N_0 = 25/200 = 0.125 = (\tfrac{1}{2})^n, so n=3n = 3 and t=3×14=42t = 3 \times 14 = 42 days. Whenever the remaining fraction is a clean power of 12\tfrac{1}{2} (12,14,18,116\tfrac{1}{2}, \tfrac{1}{4}, \tfrac{1}{8}, \tfrac{1}{16}…), you can read nn off by counting without any logs.

Try it. A source falls to 116\tfrac{1}{16} of its activity. That is (12)4(\tfrac{1}{2})^4, so n=4n = 4 half-lives. With t1/2=4t_{1/2} = 4 hours, that is 16 hours.

Worked problem 3 — fractional half-lives, going forwards

Section titled “Worked problem 3 — fractional half-lives, going forwards”

Most real times are not whole blocks. Fluorine-18 has t1/2=110t_{1/2} = 110 min. After 240240 min, how much of a 60 MBq60\ \mathrm{MBq} dose is left for the PET scan?

Compute the exponent: n=240/110≈2.18n = 240 / 110 \approx 2.18 half-lives. Then N=60×(12)2.18N = 60 \times (\tfrac{1}{2})^{2.18}. Since (12)2.18≈0.22(\tfrac{1}{2})^{2.18} \approx 0.22, about 60×0.22≈13.2 MBq60 \times 0.22 \approx 13.2\ \mathrm{MBq} remains. In words: a little more than two halvings happened, so a little less than a quarter survives — the calculator just makes “a little less” precise. Any scientific calculator does (12)2.18(\tfrac{1}{2})^{2.18} directly with the xyx^y key.

Try it. Same isotope, 9090 min elapsed (n≈0.82n \approx 0.82). (12)0.82≈0.57(\tfrac{1}{2})^{0.82} \approx 0.57, so ~57% remains — more than half, as expected for less than one half-life.

Worked problem 4 — solving for time with logs

Section titled “Worked problem 4 — solving for time with logs”

An iodine-131 spill (t1/2=8t_{1/2} = 8 days) must decay to 12%12\% before cleanup ends. How long is the wait?

Set up the sentence first: we need the nn such that (12)n=0.12(\tfrac{1}{2})^n = 0.12. Because nn is trapped in the exponent, take logs of both sides — base 10 is fine:

0.12=(12)n0.12 = (\tfrac{1}{2})^n log⁡10(0.12)=n⋅log⁡10(0.5)\log_{10}(0.12) = n \cdot \log_{10}(0.5) n=log⁡10(0.12)log⁡10(0.5)≈−0.921−0.301≈3.06n = \frac{\log_{10}(0.12)}{\log_{10}(0.5)} \approx \frac{-0.921}{-0.301} \approx 3.06

Then convert blocks to days: t=3.06×8≈24.5t = 3.06 \times 8 \approx 24.5 days. Sanity-check it: 12%12\% sits between 18\tfrac{1}{8} (12.5%12.5\%, 3 half-lives) and 116\tfrac{1}{16}, so nn just over 3 is exactly right — the logs only refined what the fractions already suggested.

If your class writes N=N0e−λtN = N_0 e^{-\lambda t} instead, it is the same formula rearranged, with λ=ln⁡2/t1/2\lambda = \ln 2 / t_{1/2}. Halving form and exponential form always agree: (12)t/t1/2=e−λt(\tfrac{1}{2})^{t/t_{1/2}} = e^{-\lambda t}.

Try it. A cobalt-60 source (t1/2=5.27t_{1/2} = 5.27 years) must fall to 5%5\%. n=log⁡(0.05)/log⁡(0.5)≈4.32n = \log(0.05)/\log(0.5) \approx 4.32 half-lives, so t≈4.32×5.27≈22.8t \approx 4.32 \times 5.27 \approx 22.8 years.

Uranium-238’s 4.5-billion-year half-life means half your atoms are thorium-234 (decaying on down the chain toward lead-206) after one block. Because heat, pressure, and compounds barely touch nuclear energies — except ~0.1% electron-capture nudges — that clock runs steady enough to date rocks and carbon-date artifacts. Randomness per atom, reliability per gram: that is the whole idea of half-life.

That finishes the nuclear-decay lesson. Four decays, the math to balance them, what happens inside, and how fast.