Nuclear Chemistry

Nuclear Decay

Five ways a nucleus throws away its instability

Nuclear decay is the spontaneous transformation of an unstable nucleus into a more stable one by emitting particles or photons. The five canonical modes — alpha, beta-minus, beta-plus (positron), electron capture, and gamma — each move the nucleus by a fixed change in proton number Z and mass number A on the chart of nuclides. The driving force is energetic stability: each step releases an energy Q equal to the parent-daughter mass difference times c². Alpha emission sheds tightly-bound He-4 nuclei from heavy elements. Beta-minus and beta-plus shuttle between proton- and neutron-rich isotopes. Electron capture is a low-energy alternative to positron emission. Gamma emission de-excites the nuclear state without changing identity. Together, the five modes explain every entry on the chart of nuclides.

  • Alpha (α)Z → Z−2, A → A−4 (emits ⁴He)
  • Beta-minus (β⁻)Z → Z+1, A unchanged (emits e⁻ + ν̄)
  • Beta-plus (β⁺)Z → Z−1, A unchanged (emits e⁺ + ν)
  • Electron capture (EC)Z → Z−1, A unchanged (absorbs e⁻)
  • Gamma (γ)Z, A unchanged (de-excitation)
  • Driving forceQ = (m_parent − m_daughter)·c²

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Why nuclei decay

The chart of nuclides — protons (Z) on one axis, neutrons (N) on the other — shows a narrow valley of stability. About 254 nuclides are stable; thousands of others fall above, below, or beyond the valley. Each unstable nucleus moves toward the valley by a specific decay mode determined by where it sits.

  • Above the valley (too many neutrons): β⁻ decay converts a neutron to a proton.
  • Below the valley (too many protons): β⁺ or electron capture converts a proton to a neutron.
  • Beyond Z = 82 (lead): the Coulomb repulsion of so many protons exceeds the strong force's reach, and α decay sheds tightly-bound He-4 nuclei.
  • Excited states (right energy, wrong configuration): γ emission drops the nucleus to its ground state.

The Q-value of any decay — the energy released — is the parent-daughter mass difference, converted to energy via E = Δm·c². Decay is allowed if Q > 0; the rate depends on quantum-mechanical transition probabilities and barrier penetration.

Alpha decay

An alpha particle is a ⁴He nucleus: 2 protons + 2 neutrons, very tightly bound (28.3 MeV total binding). Alpha decay shifts the parent by Z → Z−2, A → A−4:

      ²³⁸_{92}U  →  ²³⁴_{90}Th  +  ⁴_{2}He   (Q = 4.27 MeV)
      ²²⁶_{88}Ra →  ²²²_{86}Rn  +  ⁴_{2}He   (Q = 4.87 MeV)

The kinetic energy is shared between the alpha (≈ 98 %, since it's much lighter than the daughter) and the recoiling daughter (≈ 2 %). Alpha energies are discrete — typically 4–9 MeV — because the two-body decay leaves no continuous spectrum.

Quantum tunneling sets the rate. The alpha must escape the Coulomb barrier holding it in. Gamow's 1928 calculation showed that

      log₁₀(t_{1/2}) ≈ a·Z/√Q + b      (Geiger–Nuttall law)

so a small change in Q-value swings half-life over many orders of magnitude. ²¹²Po decays in 0.3 µs at Q = 8.95 MeV; ²³²Th lives 1.4 × 10¹⁰ years at Q = 4.08 MeV — five orders of magnitude in Q gives 23 orders of magnitude in half-life.

Penetration: alpha particles are stopped by a sheet of paper or 5 cm of air. Internal exposure is the danger — Po-210 ingested by Alexander Litvinenko in 2006 (estimated 4.4 µg, 1 GBq) caused fatal alpha damage to bone marrow.

Beta-minus decay

A neutron in a neutron-rich nucleus converts to a proton, emitting an electron (β⁻) and an antineutrino:

      n  →  p  +  e⁻  +  ν̄_e

      ¹⁴_{6}C  →  ¹⁴_{7}N  +  e⁻  +  ν̄_e   (Q = 0.156 MeV, t_{1/2} = 5,730 y)
      ¹³⁷_{55}Cs →  ¹³⁷ᵐ_{56}Ba + e⁻ + ν̄_e (Q = 0.514 MeV; daughter γ-decays)
      ⁹⁰_{38}Sr →  ⁹⁰_{39}Y  +  e⁻  +  ν̄_e  (Q = 0.546 MeV)

Mass number A stays the same; Z increases by 1. The decay energy is shared between the electron and antineutrino, giving a continuous energy spectrum from 0 up to Q for the electron. (The antineutrino was first proposed by Pauli in 1930 specifically to fix the apparent energy non-conservation.)

Penetration: a few mm of aluminum or 1 m of air for typical 1 MeV β⁻. Sr-90 and its daughter Y-90 are bone-seekers in fallout because Sr substitutes for Ca in bone; the high-energy beta from Y-90 (Q = 2.28 MeV) reaches up to 11 mm in tissue.

Beta-plus (positron) decay

In proton-rich nuclei, a proton converts to a neutron, emitting a positron (β⁺) and a neutrino:

      p  →  n  +  e⁺  +  ν_e

      ¹⁸_{9}F  →  ¹⁸_{8}O   +  e⁺  +  ν_e   (Q = 0.634 MeV, t_{1/2} = 109.7 min)
      ²²_{11}Na →  ²²_{10}Ne  +  e⁺  +  ν_e   (t_{1/2} = 2.602 y)
      ¹¹_{6}C  →  ¹¹_{5}B   +  e⁺  +  ν_e   (t_{1/2} = 20.4 min)

Z decreases by 1; A unchanged. There is a 1.022 MeV threshold — the parent mass must exceed the daughter mass by at least 2·m_e (the rest mass of the created e⁺ pair). Below this threshold only electron capture is energetically allowed.

The emitted positron travels a few mm in tissue, then annihilates with an electron to produce two 511 keV photons emitted back-to-back. PET (positron emission tomography) detects these coincident gamma pairs to localize tracer concentration. ¹⁸F-FDG (fluorodeoxyglucose) is the most common PET tracer; cancer cells accumulate it because of high glucose uptake.

Electron capture

An inner-shell (usually K) electron is absorbed by the nucleus; a proton converts to a neutron and a neutrino is emitted:

      p  +  e⁻  →  n  +  ν_e

      ⁷_{4}Be  +  e⁻  →  ⁷_{3}Li  +  ν_e        (t_{1/2} = 53.22 d)
      ⁵⁵_{26}Fe + e⁻  →  ⁵⁵_{25}Mn + ν_e        (t_{1/2} = 2.74 y)
      ⁴⁰_{19}K + e⁻   →  ⁴⁰_{18}Ar + ν_e        (10.7 % branch; rest is β⁻)

Like β⁺, Z drops by 1 and A is unchanged. Unlike β⁺, there is no 1.022 MeV threshold — EC is the only option for low-Q proton-rich decays. The K-shell hole left behind fills with an outer electron, emitting a characteristic X-ray (or, by the Auger effect, ejecting a second electron). EC daughters are detected by these X-rays.

EC is the only decay whose rate has a (tiny) chemical sensitivity: changing the electron density at the nucleus by altering the daughter's chemical bonding shifts the rate by ~1 %. ⁷Be in metallic Be vs in BeF₂ has measurably different t1/2 — about 0.83 % difference, the largest known chemical effect on a decay rate.

Gamma decay

An excited nucleus drops to a lower-energy state, emitting a gamma photon. Z and A unchanged:

      ⁹⁹ᵐ_{43}Tc  →  ⁹⁹_{43}Tc  +  γ (140.5 keV)   (t_{1/2} = 6.01 h)
      ⁶⁰_{28}Ni*  →  ⁶⁰_{28}Ni  +  γ (1.17, 1.33 MeV)  (after ⁶⁰Co β⁻)

Most gamma emission follows alpha or beta decay within picoseconds — the daughter lands excited, then de-excites. A few "metastable" excited states (isomers) live longer because the transition is angular-momentum forbidden. Tc-99m's 6-hour metastable lifetime makes it the most-used isotope in nuclear medicine; injected, imaged, and gone within a day.

Gamma photons from MeV-scale transitions are highly penetrating: a few cm of lead halve them. They are the source of external dose from ¹³⁷Cs and ⁶⁰Co in radiation oncology and food irradiation.

The five decay modes side by side

ModeWhat's emittedΔZΔADriving forcePenetrationCanonical example
Alpha (α)⁴He nucleus (2p+2n)−2−4Z > 82, Coulomb repulsion vs. tight α binding (28.3 MeV)Sheet of paper / 5 cm air²³⁸U → ²³⁴Th + ⁴He, 4.27 MeV
Beta-minus (β⁻)e⁻ + antineutrino+10Excess neutrons (above stability valley)~ 1 cm Al / few m air¹⁴C → ¹⁴N + e⁻ + ν̄, 0.156 MeV
Beta-plus (β⁺)e⁺ + neutrino−10Proton excess; Q > 1.022 MeV requiredAnnihilation: 2 × 511 keV γ¹⁸F → ¹⁸O + e⁺ + ν, 0.634 MeV
Electron capture (EC)Neutrino + characteristic X-ray−10Proton excess; Q < 1.022 MeV (β⁺ forbidden)Detect via emitted X-ray⁷Be + e⁻ → ⁷Li + ν, t1/2 = 53.2 d
Gamma (γ)High-energy photon00Excited nuclear state from prior α or β decayFew cm lead halves; very penetrating⁹⁹ᵐTc → ⁹⁹Tc + γ at 140 keV
Spontaneous fission (rare)Two daughter nuclei + 2–3 neutronsvariesvariesZ² /A > 47 (very heavy nuclei)Two large fragments, neutrons²⁵²Cf, t1/2 = 2.65 y, 3 % SF branch

Decay chain: ²³⁸U series

  ²³⁸U  ──α──►  ²³⁴Th ──β⁻──►  ²³⁴Pa ──β⁻──►  ²³⁴U  ──α──►  ²³⁰Th
   4.5e9 y       24.1 d         6.7 h           245,500 y      75,400 y

         ──α──►  ²²⁶Ra ──α──►  ²²²Rn ──α──►  ²¹⁸Po ──α──►  ²¹⁴Pb
                  1,600 y      3.82 d         3.10 min       26.8 min

         ──β⁻──► ²¹⁴Bi ──β⁻──► ²¹⁴Po ──α──►  ²¹⁰Pb ──β⁻──► ²¹⁰Bi
                  19.9 min     163 µs          22.3 y         5.01 d

         ──β⁻──► ²¹⁰Po ──α──►  ²⁰⁶Pb (stable)
                  138.4 d

14 steps from ²³⁸U to stable ²⁰⁶Pb, alternating α (8 steps) and β⁻ (6 steps), shedding 8·4 + 0 = 32 amu and 8·2 − 6·1 = 10 protons (matching A = 238 − 32 = 206 and Z = 92 − 10 = 82). Half-lives span 12 orders of magnitude. Radon-222 in basements is a member: it diffuses out of uranium-bearing rock and lodges in lungs, where its α-emitting daughters cause an estimated 21,000 lung cancer deaths per year in the US (EPA 2003 estimate).

Real isotopes and where they live

  • ²¹⁰Po (Litvinenko, 2006). Pure α emitter, t1/2 = 138.4 d, Q = 5.41 MeV. About 4.4 µg (1 GBq) was lethal because alpha damage in bone marrow is extreme when the source is internal.
  • ¹³¹I (Chernobyl, 1986). β⁻ + γ, t1/2 = 8.02 d. Decayed within months but caused thousands of pediatric thyroid cancers in Belarus and Ukraine. Iodine prophylaxis (KI tablets) saturates the thyroid with stable iodine.
  • ¹³⁷Cs (Chernobyl/Fukushima long-term). β⁻ + γ via metastable ¹³⁷ᵐBa, t1/2 = 30.07 y. Dominates persistent contamination; 40 years post-Chernobyl, ¹³⁷Cs activity is at 0.5⁴⁰⁄³⁰·⁰⁷ ≈ 40 % of 1986 levels.
  • ⁶⁰Co (radiotherapy, sterilization). β⁻ + 1.17 + 1.33 MeV γ, t1/2 = 5.27 y. Standard external-beam radiotherapy source from the 1950s through 1980s, still used in lower-resource countries; now mostly supplanted by linac X-ray.
  • ⁹⁹ᵐTc (medical imaging). Pure isomeric γ at 140 keV, t1/2 = 6.01 h. Made from ⁹⁹Mo (t1/2 = 66 h) cow generators; used in ~ 30 million scans per year worldwide.
  • ¹⁸F-FDG (PET). β⁺, t1/2 = 109.7 min. Annihilation gammas at 511 keV imaged in coincidence; standard for cancer staging and brain metabolism.
  • ⁴⁰K (banana radiation). 89.3 % β⁻ to ⁴⁰Ca, 10.7 % EC to ⁴⁰Ar, t1/2 = 1.248 × 10⁹ y. Naturally present in all biological potassium; ~ 15 Bq per banana.

Conservation laws in nuclear decay

Every nuclear decay conserves: (i) electric charge — total Z + emitted lepton charge balanced; (ii) baryon number — A counts protons + neutrons, conserved across α, β, γ; (iii) lepton number — the antineutrino in β⁻ matches the electron, the neutrino in β⁺ matches the positron; (iv) energy — Q-value equals total kinetic energy plus rest masses of products; (v) momentum — daughter recoils opposite the emitted particle(s); (vi) angular momentum and parity — selection rules govern allowed vs. forbidden transitions and explain isomers.

Common misconceptions

  • "Beta decay emits an electron from the nucleus." The electron is created at the moment of decay (along with the antineutrino), not pre-existing in the nucleus. Same for the positron in β⁺.
  • Confusing β⁺ and EC. Both increase neutron count and decrease Z, but β⁺ requires Q > 1.022 MeV and emits a detectable positron; EC has no threshold and emits only a neutrino plus characteristic X-rays.
  • Treating gamma decay as separate. Pure isomeric transitions exist (e.g., Tc-99m), but most gammas are de-excitations of daughters from prior α or β. The cesium-137 "γ source" is really β⁻ to metastable Ba-137 followed by γ.
  • Equating activity with danger. A tiny ²¹⁰Po speck has lower activity than a smoke detector's ²⁴¹Am, but ingested ²¹⁰Po is far more dangerous because of the dose distribution. Penetration, route of exposure, and biological half-life all matter.
  • Assuming all alpha emitters are heavy. Mostly true (Z > 82), but a few light nuclei α-decay too: ⁵Li → ⁴He + ¹H (unbound), and ⁸Be → 2 × ⁴He (Q = 92 keV, t1/2 = 8 × 10⁻¹⁷ s, the basis of stellar carbon synthesis).
  • Confusing decay rate with half-life sensitivity. A 1 % shift in alpha Q-value can change t1/2 by several orders of magnitude (Geiger–Nuttall). Beta decay rates are much less sensitive to Q.

Frequently asked questions

What's the difference between alpha and beta decay?

Alpha decay emits a ⁴He nucleus (2 protons + 2 neutrons), reducing the parent's mass number by 4 and atomic number by 2. It's typical of heavy nuclei (Z > 82) where the strong force can't keep large nuclei together — uranium-238 alpha-decays to thorium-234. Beta-minus decay emits an electron and antineutrino as a neutron converts to a proton; mass number unchanged, atomic number up by 1. It's typical of neutron-rich nuclei. Cesium-137 beta-decays to barium-137. The two have completely different penetration: alpha stops at a sheet of paper, beta penetrates a few millimeters of aluminum.

Why does beta decay produce a continuous energy spectrum?

The decay energy is shared between the emitted electron and an antineutrino. Since the (anti)neutrino flies off undetected, the electron's energy varies from zero up to the maximum decay energy Q. Pauli proposed the neutrino in 1930 specifically to explain this continuous spectrum — without a third particle, conservation of energy and momentum would have forced a discrete electron energy, which experiment ruled out.

What's the difference between positron emission and electron capture?

Both convert a proton to a neutron, lowering Z by 1 and keeping A unchanged. Positron emission ejects a positron (β⁺) and a neutrino; the daughter mass plus 2·m_e c² (1.022 MeV) must equal or be less than the parent. Electron capture absorbs an inner-shell (usually K-shell) electron and emits only a neutrino — no 1.022 MeV threshold, so it's the only option for decay energies below that. Heavy proton-rich nuclei often do both. Both daughters can also emit characteristic X-rays as outer electrons fill the K-shell hole.

Is gamma decay a separate decay or part of others?

It's almost always a follow-up. After alpha or beta decay, the daughter often lands in an excited state. Gamma emission de-excites it within picoseconds without changing Z or A. Some isomers (metastable states) wait longer — Tc-99m has 6-hour half-life before its gamma transition, the basis of medical imaging. Pure gamma decay (isomeric transition) is a transition between nuclear energy levels of the same isotope; the prompt gammas after fission and the after-decay gammas observed in radioactive tracers are the same physics.

Why do heavy elements all undergo alpha decay?

The strong nuclear force is short-range (~ 1 fm); the Coulomb repulsion among protons is long-range. As nuclei get heavier, every proton repels every other proton (~ Z² electrostatic energy) but only feels strong attraction from neighbors. Beyond Z = 82 (lead), the strong force can't quite balance Coulomb, and alpha emission lets the nucleus shed two protons and two neutrons in one tightly-bound, low-mass package. The 28.3 MeV binding energy of the alpha particle makes this energetically favorable — no other multi-nucleon emission has that combination.

What's a decay chain?

A sequence of decays from an unstable parent to a stable daughter, passing through unstable intermediates. The 4n+2 chain starting at ²³⁸U passes through 14 steps — Th-234, Pa-234, U-234, Th-230, Ra-226, Rn-222, Po-218, Pb-214, Bi-214, Po-214, Pb-210, Bi-210, Po-210 — to land on stable Pb-206. Each step has its own half-life and decay mode (mostly alpha and beta-minus). At secular equilibrium, every member of the chain has the same activity as the long-lived parent. The ²²²Rn in basements is a member of this chain.