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Bounded modern-physics survey · Interactive lesson

Α, β, and gamma decay modes

An unstable nucleus has three ways to lower its mass: shed a helium-4 cluster, turn a neutron into a proton or back, or drop to a lower level by emitting a photon. Learn to predict which way a nuclide will go, where it lands on the chart, and what the emitted energies reveal, including a particle no detector of the 1920s could see.

UPIII-11.03 · Lesson 3 of 9 in this unit. Position is not a completion score.
Starting model: Alpha, beta, and gamma decay modesChart of nuclides near uranium, neutron number N across and proton number Z up, on equal scales; the curve is the liquid-drop valley of stability. From ²³⁸U the dot has made α steps (4 so far), each lowering N and Z by 2, and β⁻ steps (0), each trading a neutron for a proton, to reach Z = 84, N = 138. The dashed segment runs along its isobar to the valley.²³⁸U²⁰⁶Pbvalleyproton number Zneutron number Nfrom ²³⁸U: 4 α, 0 β⁻Z = 84, N = 138A = 222, N − Z = 54valley N − Z = 47.8
Start with a picture. Change the model in the lab below.

Bounded modern-physics survey. This modern-physics material is an introductory survey, not a complete course in relativity, quantum, atomic, nuclear or particle physics. Your university determines the required depth and assessment.

1

Build the model

Three ways down the valley of stability, each leaving its own fingerprint.

The key idea

A decay mode is the route by which an unstable nucleus lowers its mass-energy: α emission removes two protons and two neutrons, β decay turns a neutron into a proton or the reverse at fixed A, and γ emission drops the nucleus to a lower level of the same nuclide.

Example. ¹⁴C (Z = 6, N = 8) β⁻-decays to ¹⁴N (Z = 7, N = 7): A stays 14, and the 0.156 MeV released is split between the electron and an antineutrino in every proportion, so the electrons emerge with any energy from 0 to 0.156 MeV.

The complete physical model and assumptions

For each mass number A there is one proton number Z₀ at which A = Z + N nucleons have least mass. The symmetry energy pulls Z₀ towards A/2, Coulomb repulsion pulls it lower, and the compromise is a valley of stability running from N/Z = 1 in light nuclei to about 1.5 at lead. An unstable nuclide goes downhill only by routes that conserve charge, nucleon number and lepton number. Beta decay converts one kind of nucleon into the other through the weak interaction, so it slides a nuclide along its isobar towards Z₀ at fixed A. Alpha emission removes two protons and two neutrons and pays only in heavy nuclei, where the 28.3 MeV binding of helium-4 exceeds what the parent loses. Gamma emission changes neither Z nor N: it drops the nucleus between its own discrete levels. The products carry fingerprints of the kinematics. Alpha and gamma lines are sharp, since two bodies share energy in a fixed way; beta electrons emerge with a continuous spread, which forced a third, unseen particle into the ledger, the neutrino. Nuclear levels sit keV to MeV apart while chemistry works in eV and kT is 0.026 eV at room temperature, so decay rates ignore chemical state and temperature. The survey says which modes are open and where each lands, not how fast: half-lives span more than thirty orders of magnitude, and only processes that use atomic electrons, electron capture chief among them, can be nudged by chemistry.

1Label the nuclide, then find its valley

Write a nuclide as ᴬX with Z protons and N neutrons, so A = Z + N: ²³⁸U has Z = 92 and N = 146. Z fixes the element and its chemistry; isotopes share Z, isotones share N, isobars share A. The roughly 250 stable nuclides fill a narrow valley on a chart of Z against N. At fixed A the mass is close to a parabola in Z: the symmetry energy, proportional to (N − Z)²/A, is least at N = Z, while the Coulomb energy, proportional to Z²/A¹⁄³, is least at small Z. Set ∂M/∂Z = 0 at fixed A and the bottom lies at Z₀ ≈ A/(1.98 + 0.0155 A²⁄³). That gives Z₀ = 7.7 at A = 16, 50.9 at A = 120 and 82.4 at A = 208, matching ¹⁶O, ¹²⁰Sn and ²⁰⁸Pb, with N/Z climbing from 1 to 1.54. A nuclide off the valley floor is unstable, and the side it sits on decides how it decays.

2Beta decay slides a nuclide along its isobar

A neutron-rich nuclide lowers its mass by converting a neutron, n → p + e⁻ + ν̄ₑ, taking (Z, N) to (Z + 1, N − 1) at fixed A. A proton-rich one runs the reverse, p → n + e⁺ + νₑ, which a free proton cannot do, being 1.293 MeV lighter than a neutron; inside a nucleus the gain in binding pays for it. Each step moves one place down the isobar's mass parabola, so an odd-A chain ends on a single stable isobar: ¹⁰¹Mo β⁻-decays to ¹⁰¹Tc and then to ¹⁰¹Ru, and Z₀(101) = 43.6 rounds to ruthenium's 44. β⁺ must also create a positron, which with atomic masses means M(A, Z) − M(A, Z − 1) > 2mₑ, or 1.022 MeV/c². Below that gap electron capture, p + e⁻ → n + νₑ, is the only route: ⁷Be lies 0.862 MeV above ⁷Li and decays by capture alone. Even-A isobars sit on two parabolas split by pairing, which is why odd-odd ⁴⁰K goes both ways: β⁻ in 89% of decays, capture in 11%.

3A continuous spectrum demands a third particle

Let a nucleus at rest split into two bodies and momentum conservation sends them back to back with fixed shares of Q. For ²¹⁰Bi, Q = 1.162 MeV, so every electron would carry 1.162 MeV less 6.5 eV of recoil: one sharp line. Instead the electrons emerge with every energy from zero to a sharp endpoint at Q, averaging 0.39 MeV. Calorimetry in 1927 showed the missing energy was not being lost inside the source, and angular momentum failed too: ²¹⁰Bi has spin 1 and ²¹⁰Po spin 0, and an electron's spin ½ plus any whole-number orbital angular momentum can never make up a whole number. Pauli's answer in 1930 was a third particle, neutral, spin ½ and nearly massless, that shares the energy with the electron in any proportion: Kₑ + Kν + KR = Q. The endpoint is where the neutrino takes almost nothing. Reines and Cowan detected reactor antineutrinos in 1956, and the shape of tritium's spectrum just below its 18.6 keV endpoint now holds the neutrino mass below 0.45 eV/c².

4Alpha emission: why a heavy nucleus sheds helium-4

Emitting any cluster costs the binding the parent loses and returns the cluster's own: Q = B(daughter) + B(cluster) − B(parent), with B = 0 for a lone nucleon. For ²³⁸U, losing a neutron costs 6.15 MeV, so that is forbidden. Losing two protons and two neutrons costs 1801.69 − 1777.66 = 24.03 MeV, but helium-4 returns 28.30 MeV, so Qα = +4.27 MeV. Put another way, Qα ≈ 28.3 MeV − 4 ∂B/∂A along the α path, positive only once a nucleon costs less than 7.07 MeV to remove, which happens in heavy nuclei, above roughly A ≈ 150, where B/A is falling. The α and the daughter are two bodies, so α energies come as sharp lines. Q only opens the door. At the surface of ²³⁴Th the Coulomb barrier is about 28 MeV, over six times the α's 4.2 MeV, so the α must tunnel, and the rate is exquisitely sensitive to Q: ²¹²Po, with Qα = 8.95 MeV, has a half-life of about 0.3 μs, while ²³⁸U, at 4.27 MeV, has one of 4.5 × 10⁹ years: a factor of 2 in Q, a factor near 5 × 10²³ in lifetime.

5Alpha steps push heavy nuclei off the valley

An α removes equal numbers of protons and neutrons, so N − Z is unchanged while A falls by 4. The valley wants less neutron excess at smaller A: A − 2Z₀ is 53.2 at A = 238 but only 42.5 at A = 206. So each α step leaves the daughter about two-thirds of a proton further to the neutron-rich side of its isobar's valley point, and β⁻ decays, each cutting N − Z by 2, must follow. The ledger for ²³⁸U → ²⁰⁶Pb is exact. A falls by 32, so there are 8 α decays. N − Z must fall from 54 to 42, so there are 6 β⁻ decays. Charge closes: 92 − 16 + 6 = 82. Because only α changes A, and always by 4, every heavy nuclide belongs to one of four families, A = 4n, 4n + 1, 4n + 2 or 4n + 3, ending on ²⁰⁸Pb, ²⁰⁹Bi, ²⁰⁶Pb and ²⁰⁷Pb. β⁺ essentially never appears in these chains: the α steps only ever push the nuclides the other way.

6Gamma emission, and why chemistry cannot reach the nucleus

α and β decays often leave the daughter in an excited level, and it falls to the ground state by emitting photons, A and Z unchanged: ¹³⁷Cs β⁻-decays mostly to a ¹³⁷Ba level 0.662 MeV up, whose 662 keV gamma ray calibrates detectors worldwide. Why MeV, when hydrogen's lines are eV? Confine a nucleon to R ≈ 5 fm and its energy scale is (ħc)²/(2mc²R²) = (197 MeV fm)² / (2 × 939 MeV × 25 fm²) ≈ 0.8 MeV. That scale also walls the nucleus off. Chemical bonds shift energies by a few eV, parts per million of a typical Q. Heat can populate a level ΔE up only with Boltzmann factor e(−ΔE/kT): for ΔE = 100 keV at 300 K the exponent is −3.9 × 10⁶, and even in the Sun's 1.5 × 10⁷ K core it is −77, a factor of 10⁻³⁴. So a half-life is a constant of the nuclide. The exceptions use atomic electrons, electron capture chief among them: it needs an atomic electron at the nucleus, so ⁷Be's half-life shifts by up to about 1% between chemical settings, and a bare ⁷Be ion cannot decay at all.

2

Key equations

Read the units, assumptions and limits before substituting.

Valley of stability, liquid-drop estimate

Z₀ ≈ A / (1.98 + 0.0155 A²⁄³)

Z₀ = 25.4 at A = 56 and 82.4 at A = 208. Coulomb energy grows as Z²/A¹⁄³, so heavy nuclei need N/Z ≈ 1.5 where light ones sit near 1.

A = Z + N nucleons; Z₀ the proton number of least mass at that A. Pure counts, no units; good to about ±1

Alpha emission energetics

Qα = B(A − 4, Z − 2) + B(⁴He) − B(A, Z)

For ²³⁸U, Qα = +4.27 MeV, while shedding one neutron costs 6.15 MeV: helium-4 is bound so tightly that it can leave where a lone nucleon cannot.

B the binding energies in MeV, B(⁴He) = 28.30 MeV; the daughter has Z − 2 and N − 2; allowed only if Qα > 0

Β-minus conversion

n → p + e⁻ + ν̄ₑ

Allowed whenever the atomic mass falls, M(A, Z) > M(A, Z + 1). A free neutron does it with Q = 0.782 MeV and a half-life of 10.2 min.

In a nucleus (Z, N) → (Z + 1, N − 1) at fixed A. Charge 0 = +1 − 1; lepton number 0 = +1 − 1

Β-plus conversion

p → n + e⁺ + νₑ

Below that gap only electron capture, p + e⁻ → n + νₑ, is open: ⁷Be lies 0.862 MeV above ⁷Li and decays purely by capture.

Inside a nucleus only: (Z, N) → (Z − 1, N + 1). Needs M(A, Z) − M(A, Z − 1) > 2mₑ, that is 1.022 MeV/c², in atomic masses

Three-body energy sharing in β decay

Kₑ + Kν + KR = Qβ

A third body makes the split free, so Kₑ runs continuously from 0 to the endpoint Qβ. Two bodies would give one line: 1.162 MeV for every ²¹⁰Bi electron.

Kₑ, Kν, KR the kinetic energies of electron, neutrino and recoiling daughter, in MeV; KR is only eV to keV, far below Qβ

Gamma photon between nuclear levels

Eγ = Eᵢ − Ef − Eγ²/(2Mc²)

The recoil term is 15.9 eV for the 1.3325 MeV line of ⁶⁰Ni, about 1 part in 10⁵, so γ energies read a nucleus's level scheme almost directly.

Eᵢ and Ef the level energies, M the emitting nucleus's mass, energies in MeV; A and Z are unchanged
3

Interactive lab

Predict first. Explore the model. Compare the result.

Explore the model

4
0 to 8; steps of 1.
0
0 to 6; steps of 1.

Try this. Take all eight α steps with no β⁻: N − Z stays 54 while the valley's falls to 42.5, leaving the dot 5.7 protons short of the valley. Then add β⁻ steps: each cuts N − Z by 2, and the sixth lands on ²⁰⁶Pb, the stable end of the chain.

Live results

MASS NUMBER A
222
PROTON NUMBER Z
84
NEUTRON EXCESS N − Z
54
OFF THE VALLEY Z − Z₀
-3.1

Results follow this lesson’s model and assumptions. Displayed values are rounded.

Interactive Physics III modelChart of nuclides near uranium, neutron number N across and proton number Z up, on equal scales; the curve is the liquid-drop valley of stability. From ²³⁸U the dot has made α steps (4 so far), each lowering N and Z by 2, and β⁻ steps (0), each trading a neutron for a proton, to reach Z = 84, N = 138. The dashed segment runs along its isobar to the valley.²³⁸U²⁰⁶Pbvalleyproton number Zneutron number Nfrom ²³⁸U: 4 α, 0 β⁻Z = 84, N = 138A = 222, N − Z = 54valley N − Z = 47.8
Chart of nuclides near uranium, neutron number N across and proton number Z up, on equal scales; the curve is the liquid-drop valley of stability. From ²³⁸U the dot has made α steps (4 so far), each lowering N and Z by 2, and β⁻ steps (0), each trading a neutron for a proton, to reach Z = 84, N = 138. The dashed segment runs along its isobar to the valley.

Predict → change one variable → check

Plan a change before running it. Every other input stays at the saved baseline.

Saved baseline. α decays taken: 4; β⁻ decays taken: 0

Baseline 4; choose 0 to 8, in steps of 1.
4. Compared with the saved baseline, this result will…

This experiment is kept only while this page is open. It does not change saved course progress.

4

Catch the common trap

The commonest slip is to picture the β⁻ electron as a particle that was sitting inside the nucleus, or as one of the atom's own electrons knocked loose. Neither survives a number. An electron confined to a nucleus of radius 5 fm needs momentum of order ħ/R, so pc ≈ 197 MeV fm ÷ 5 fm ≈ 40 MeV and its kinetic energy is near 39 MeV, yet β electrons usually leave with only a few MeV, and no known force could hold one that energetic. The shell-electron picture fails differently: the daughter has Z + 1, a new element, and the electron's energy runs to MeV, not the eV of atomic binding. Nor is a neutron a proton and an electron stuck together: two spin-½ particles plus any orbital motion give a whole-number spin, and the neutron's is ½. The electron and antineutrino are created in the decay, as a d quark becomes a u quark, just as an atom creates the photon it emits rather than storing it.

5

Practice & worked examples

3 authored examples. Make an attempt, then reveal the reasoning one step at a time.

EasyExample 1

⁶⁰Co (Z = 27) decays by β⁻ with Q = 2.8228 MeV, almost always to a level of its daughter at 2.5057 MeV, which reaches the ground state by emitting a 1.1732 MeV and then a 1.3325 MeV gamma ray. Identify and balance the decay, find the endpoint of the electron spectrum, check the cascade against the level, and find the recoil energy of the daughter (M = 59.93 u) when it emits the 1.3325 MeV photon.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

MediumExample 2

²¹⁰Po (Z = 84, N = 126) has binding energy 1645.213 MeV. With B(²⁰⁹Po) = 1637.554 MeV, B(²⁰⁹Bi) = 1640.229 MeV, B(²⁰⁷Pb) = 1629.062 MeV, B(²⁰⁶Pb) = 1622.325 MeV, B(³He) = 7.718 MeV and B(⁴He) = 28.296 MeV, decide which of a neutron, a proton, a ³He nucleus and an α particle it can emit, say why, and compare the α's Q with the Coulomb barrier at contact.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 5 steps revealed.

HardExample 3

Tritium β⁻-decays to ³He with Q = 18.59 keV. Model the electron spectrum as dP/dK = C √K (Q − K)² for 0 ≤ K ≤ Q, neglecting recoil and the daughter's Coulomb pull. Normalise it, then find the most probable and the mean electron energy, the mean energy carried off by the antineutrino, and the fraction of electrons above Q/2. Compare the mean with the measured 5.69 keV.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 6 steps revealed.

6

Quick check

Select an answer and explain it before checking.

²¹⁰Bi decays by β⁻ to ²¹⁰Po with Q = 1.162 MeV. Its electrons emerge with every kinetic energy from nearly zero up to 1.162 MeV, and a thick calorimeter around the source, which absorbs the electrons together with any energy they lose inside it, records an average of only 0.39 MeV per decay. What must be true?
7

Review & continue

A decay mode is the route by which an unstable nucleus lowers its mass-energy: α emission removes two protons and two neutrons, β decay turns a neutron into a proton or the reverse at fixed A, and γ emission drops the nucleus to a lower level of the same nuclide.

  • Explain the relationship without looking at the equation.
  • Check a sign, a unit and a model assumption in your working.
  • Return to the lab or worked example if a step is still unclear.

Optional supporting lessons

These chapter resources can help with earlier ideas; they are not additional required Physics III completion tasks.

Extra challenging questions

Connect several ideas, explore supplied data, and compare your reasoning with a worked solution.