Nuclear Physics

Radioactive Decay

Unstable nuclei spontaneously transform — alpha, beta, gamma — at rates set by half-life

Radioactive decay is the spontaneous transformation of unstable atomic nuclei. Three main types — alpha (heavy nuclei emit He-4), beta (n→p+e or p→n+e⁺), gamma (excited nucleus emits photon). Each isotope has characteristic half-life — from microseconds to billions of years. Discovered by Becquerel (1896), the Curies. Critical for radiometric dating, medical imaging, nuclear physics.

  • Alpha decayEmits ⁴He nucleus; A→A-4, Z→Z-2
  • Beta-minus decayn → p + e⁻ + ν̄; A unchanged, Z+1
  • Beta-plus decayp → n + e⁺ + ν; A unchanged, Z-1
  • Gamma decayExcited nucleus emits photon; same A and Z
  • Half-lifeTime for half the nuclei to decay (constant for given isotope)
  • DiscoveredBecquerel (1896), Marie & Pierre Curie (1898)

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Decay types

TypeEquationWhat changesExamples
Alpha (α)(A,Z) → (A-4,Z-2) + ⁴HeA−4, Z−2U-238, Ra-226, Th-232
Beta-minus (β⁻)n → p + e⁻ + ν̄A same, Z+1C-14, Sr-90, Cs-137
Beta-plus (β⁺)p → n + e⁺ + νA same, Z−1C-11, F-18, Na-22
Electron capture (EC)p + e⁻ → n + νA same, Z−1K-40, Be-7
Gamma (γ)Nucleus* → Nucleus + γA, Z sameBa-137m → Ba-137 + γ
Spontaneous fissionHeavy nucleus → fragmentsVariousCf-252, U-238 (rare)

Exponential decay law

N(t) = N₀ · e^(-λt)

where λ is the decay constant (per second). Half-life τ:

τ = ln(2) / λ ≈ 0.693 / λ

Activity (decays per second):

A(t) = λ · N(t) = A₀ · e^(-λt)
TimeFraction remaining
0100%
1 half-life50%
2 half-lives25%
5 half-lives3.1%
10 half-lives0.098%
20 half-lives~10⁻⁶

JavaScript — radioactive decay

// Decay constant from half-life
function decayConstant(half_life) {
  return Math.log(2) / half_life;
}

// Number remaining after time t
function remaining(N_0, half_life, t) {
  return N_0 * Math.exp(-Math.log(2) * t / half_life);
}

// Activity at time t (decays/s) for sample with N atoms
function activity(N, half_life) {
  return N * decayConstant(half_life);
}

// Carbon-14 dating
function carbon14Age(remaining_fraction) {
  // remaining = exp(-λt) → t = -ln(remaining) / λ
  const half_life = 5730;  // years
  return -Math.log(remaining_fraction) / decayConstant(half_life);
}

console.log(`50% C-14: ${carbon14Age(0.5).toFixed(0)} years`);  // 5730
console.log(`25% C-14: ${carbon14Age(0.25).toFixed(0)} years`); // 11460
console.log(`12.5% C-14: ${carbon14Age(0.125).toFixed(0)} years`); // 17190

// Tc-99m for medical imaging (6 hr half-life)
function medicalDoseRemaining(initial_activity_MBq, hours) {
  const half_life = 6;  // hours
  return initial_activity_MBq * Math.exp(-Math.log(2) * hours / half_life);
}

console.log(`Tc-99m after 12 hr: ${medicalDoseRemaining(740, 12).toFixed(0)} MBq`);
console.log(`After 24 hr: ${medicalDoseRemaining(740, 24).toFixed(0)} MBq`);  // ~46
console.log(`After 48 hr: ${medicalDoseRemaining(740, 48).toFixed(2)} MBq`);  // ~3

// Ra-226 (1600 yr half-life): activity from 1 g
function radiumActivity(mass_g = 1) {
  // Ra-226 atomic mass = 226 g/mol; 6.022e23 atoms/mol
  const N = mass_g / 226 * 6.022e23;
  const half_life_s = 1600 * 365.25 * 24 * 3600;
  return activity(N, half_life_s);
}

console.log(`1 g Ra-226: ${(radiumActivity() / 1e9).toFixed(1)} GBq`);  // 36.6 (= 1 Ci)

// Half-lives of key isotopes
const isotopes = {
  'C-14': { halflife_yr: 5730, decay: 'beta-minus' },
  'I-131': { halflife_yr: 0.022, decay: 'beta-minus + gamma' },
  'Tc-99m': { halflife_yr: 0.000685, decay: 'gamma' },  // 6 hr
  'Sr-90': { halflife_yr: 28.8, decay: 'beta-minus' },
  'Cs-137': { halflife_yr: 30.2, decay: 'beta-minus + gamma' },
  'Pu-239': { halflife_yr: 24100, decay: 'alpha' },
  'U-235': { halflife_yr: 7.04e8, decay: 'alpha' },
  'U-238': { halflife_yr: 4.5e9, decay: 'alpha' },
  'Po-212': { halflife_yr: 9.5e-15, decay: 'alpha' }
};
console.log(isotopes);

Where decay matters

  • Radiometric dating. C-14 (recent organics), U-Pb (rocks, billions of years), Ar-Ar (volcanic), tritium (water).
  • Medical imaging. SPECT (Tc-99m), PET (F-18), nuclear medicine.
  • Cancer therapy. Brachytherapy seeds; external beam (Co-60, accelerator-based).
  • Nuclear power. Reactor fuel cycle, fuel longevity, waste handling.
  • Industrial. Sterilization, gauging (thickness, density), tracers in pipelines.
  • Smoke detectors. Most use small Am-241 source (alpha emitter).
  • Geochemistry. Dating of sediments, magmatic events, climate proxies.

Common mistakes

  • Treating all radiation as equally dangerous. Alpha — heavy, short range; only dangerous if ingested/inhaled. Beta — moderate range, can be stopped by aluminum. Gamma — long range, needs lead/concrete shielding.
  • Assuming half-life can be controlled. Half-life is constant; not affected by chemistry, temperature, pressure (within physical limits).
  • Linear extrapolation of N vs t. Decay is exponential, not linear. After 10 half-lives, ~0.1% remains, not 0%.
  • Confusing activity with dose. Activity (Bq, Ci) — decays per second. Dose (Sv, rem) — biological effect. Same activity gives different dose depending on radiation type and exposure conditions.
  • Forgetting parent-daughter chains. U-238 decays through 14 daughter isotopes before reaching stable Pb-206. All members contribute to total radioactivity.
  • Treating radiation phobia as proportional to risk. Background and medical exposures small fraction of cancer risk. Major events (Chernobyl, Fukushima) had quantified, geographically-limited impacts.

Frequently asked questions

What types of radioactive decay exist?

Three primary — Alpha (α): nucleus ejects ⁴He (2 p + 2 n). Mass # decreases by 4, atomic # by 2. Heavy nuclei (U, Th). Beta-minus (β⁻): neutron converts to proton + electron + antineutrino. Z increases by 1, A unchanged. Beta-plus (β⁺): proton → neutron + positron + neutrino. Z decreases by 1. Gamma (γ): excited nucleus drops to lower state, emits photon. No change in A or Z. Other modes — electron capture, internal conversion, fission, etc.

What's a half-life?

Time for half of a sample's nuclei to decay. After one half-life: 50% remain. Two half-lives: 25%. Three: 12.5%. Etc. Half-life is constant for a given isotope — independent of temperature, pressure, chemistry. Derived from N(t) = N₀·exp(-λt); half-life = ln(2)/λ.

Why does radioactive decay happen?

Nuclei seek lower energy / higher binding energy per nucleon. Heavy nuclei (mass # > ~60) are over-binded — fission or alpha decay releases energy. Neutron-rich nuclei: β⁻ decay converts n to p. Proton-rich: β⁺ or electron capture. Excited states: gamma decay. Quantum mechanical — tunneling through Coulomb barrier (alpha), weak force interaction (beta).

How fast can decay be?

Half-lives range from picoseconds to billions of years. Po-212: 0.3 µs. I-131: 8 days. Sr-90: 29 yr. Cs-137: 30 yr. C-14: 5730 yr. U-238: 4.5 Gyr. Geiger-Nuttall rule — alpha half-lives have logarithmic dependence on Q-value (energy released). Larger Q → faster decay (exponentially).

How is decay used in dating?

Carbon-14 dating — atmospheric C-14 / C-12 ratio constant; living organisms incorporate this; after death, C-14 decays. Measure remaining C-14, compute age (5730-yr half-life). Useful 0-50,000 years. Older — uranium-lead, potassium-argon, samarium-neodymium dating. Earth's age (4.5 billion years) determined this way.

How is radioactivity used medically?

Imaging — Tc-99m (6-hr half-life) for SPECT scans. F-18 in FDG for PET. Therapy — I-131 for thyroid cancer. Co-60 gamma for cancer treatment. Brachytherapy — radioactive seeds implanted in tumors. Sterilization of medical equipment via gamma rays.

How dangerous is radiation?

Depends on dose, type, duration. Acute high doses (> 1 Sv) — radiation sickness, possibly fatal. Chronic low doses — increased cancer risk. Background radiation — ~3 mSv/year (cosmic + terrestrial + medical). LNT (Linear No-Threshold) model — risk proportional to total dose. Hormesis (low doses beneficial) is debated. Always ALARA (As Low As Reasonably Achievable).