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Half-Life

Reading time: 7 minConfidence: HighLast verified: July 2026

Half-life is the time required for half of a sample of a radioactive substance to decay — a fixed, characteristic property of each radioactive isotope, independent of the sample's size, age, or surrounding conditions, and directly related to the isotope's decay constant.

Curious

One sentence that captures itEvery radioactive substance has its own fixed "half gone" time — wait that long, and exactly half of whatever amount you started with will have decayed, no matter how much you started with.

Half-life is the most intuitive way to describe how quickly a radioactive substance decays. Start with any amount of a radioactive isotope, wait one half-life, and exactly half of it will have decayed into something else, leaving half remaining. Wait a second half-life, and half of what's left decays too, leaving a quarter of the original amount — and so on, indefinitely.

Half-lives vary enormously between different radioactive isotopes — from tiny fractions of a second for some highly unstable nuclei, to billions of years for others, like uranium-238's half-life of about 4.5 billion years, roughly the age of the Earth itself. This huge range reflects the sensitivity of the underlying quantum tunnelling process (for alpha decay in particular) to the exact height and width of the nuclear potential barrier each specific isotope's nucleons must tunnel through.

Exploring

Real-world exampleCarbon-14, used in radiocarbon dating, has a half-life of about 5,730 years — precisely known and calibrated against independently dated samples (like tree rings), making it possible to estimate the age of organic remains up to roughly 8–10 half-lives (around 50,000 years) before the remaining carbon-14 becomes too sparse to measure reliably.
t_½ = ln(2)/λ
SymbolNameSI Unit
t_½Half-lifesecond (s), or any convenient time unit
λDecay constants⁻¹
ln(2)Natural logarithm of 2 ≈ 0.6931dimensionless
Common mistake — Commonly ConfusedAfter two half-lives, a sample does not have zero material remaining — it has one quarter of the original amount (half of the remaining half), and technically never reaches exactly zero in finite time under the idealised exponential decay law, only approaching it asymptotically. Students sometimes assume "two half-lives = fully decayed," which is incorrect; roughly ten half-lives leaves less than 0.1% of the original material, a practical (not exact) threshold for "essentially gone."

Worked example: A sample has a half-life of 8 days (approximately iodine-131's half-life). Its decay constant is λ = ln(2)/t_½ = 0.6931/8 ≈ 0.0866 per day. After 24 days (exactly 3 half-lives), the fraction remaining is (1/2)³ = 1/8 = 12.5% of the original amount.

Deep Dive

Primary sourceLibby, W.F. (1946). "Atmospheric Helium Three and Radiocarbon from Cosmic Radiation." Physical Review, 69(11–12), 671–672.

Willard Libby's development of radiocarbon dating in the late 1940s, building on the earlier discovery of carbon-14, provided archaeology and geology with an unprecedented, physics-based tool for absolute dating of organic material — a technique that transformed both fields and earned Libby the 1960 Nobel Prize in Chemistry. Modern radiocarbon dates are additionally calibrated against independent chronologies (tree-ring dating, ice cores) to correct for small historical variations in atmospheric carbon-14 production, refining the technique's accuracy considerably beyond Libby's original method.

Relationship to mean lifetime: Half-life is related to, but numerically distinct from, the mean lifetime τ = 1/λ (the average time a given unstable nucleus survives before decaying) — the two are related by t_½ = τ ln(2) ≈ 0.693τ, meaning the mean lifetime is always somewhat longer than the half-life. Both quantities describe exactly the same underlying exponential decay process; the choice between them is largely a matter of convention and convenience for different applications (half-life is more common in dating and medical contexts, while mean lifetime appears more often in particle physics).

Medical applications of radioactive isotopes (nuclear medicine imaging and radiation therapy) require careful selection of isotopes with half-lives matched to their intended use — short enough that radioactivity doesn't linger dangerously in a patient's body long after treatment, but long enough to remain useful for the required imaging or therapeutic window; technetium-99m, with a half-life of about 6 hours, is a widely used example specifically chosen for this balance.

Sources

  • Libby, W.F. (1946). Physical Review, 69(11–12), 671–672.
  • Krane, K.S. (1987). Introductory Nuclear Physics. Wiley, Ch. 6.
Last verified: July 2026 · Source: Libby (1946); Krane (1987) · Confidence: high