The standard way of writing a nuclide is
\[
^{A}_{Z}\!X
\]
where
Example: carbon‑12 is written \(^{12}{6}\!C\). The same element with a different number of neutrons, carbon‑13, is written \(^{13}{6}\!C\).
\[
A = Z + N
\]
| Aspect | Proton number (\(Z\)) | Nucleon number (\(A\)) |
|---|---|---|
| What it counts | Protons only | Protons + neutrons |
| Symbol | \(Z\) | \(A\) |
| Determines | Chemical element (e.g. carbon, oxygen) | Specific isotope (e.g. \(^{12}\)C vs \(^{13}\)C) |
| Typical natural range | 1 – 118 (known elements) | 1 – ≈ 300 (heaviest naturally occurring nuclides) |
| Conservation in reactions | Conserved unless a nuclear transmutation changes the element | Conserved in every nuclear reaction |
| Radiation | Particle emitted | Charge | Mass (u) | Typical energy | Effect on \(A\) and \(Z\) | Penetration / shielding |
|---|---|---|---|---|---|---|
| α (alpha) | \(^{4}_{2}\!He\) (helium nucleus) | +2 e | 4 u | ≈ 5 MeV | \(A\) − 4, \(Z\) − 2 | Stopped by a sheet of paper or a few cm of air |
| β⁻ (beta‑minus) | Electron \(e^{-}\) | −1 e | ≈ 0 u | ≈ 0.1–10 MeV | \(A\) unchanged, \(Z\) + 1 | Requires a few mm of aluminium or plastic |
| β⁺ (beta‑plus, positron emission) | Positron \(e^{+}\) | +1 e | ≈ 0 u | ≈ 0.1–10 MeV | \(A\) unchanged, \(Z\) − 1 | Similar shielding to β⁻ (aluminium, plastic) |
| γ (gamma) | High‑energy photon | 0 e | ≈ 0 u | ≈ 0.1–10 MeV (often higher) | \(A\) and \(Z\) unchanged | Requires dense material – lead or several cm of concrete |
All of the following obey the conservation of \(A\) and \(Z\).
\[
^{238}{92}\!U \;\longrightarrow\; ^{234}{90}\!Th \;+\; ^{4}_{2}\!\alpha
\]
\(A: 238 \to 234+4\) \(Z: 92 \to 90+2\)
\[
^{14}{6}\!C \;\longrightarrow\; ^{14}{7}\!N \;+\; e^{-} \;+\; \bar\nu_{e}
\]
\(A\) unchanged (14) \(Z\) increases from 6 to 7.
\[
^{18}{9}\!F \;\longrightarrow\; ^{18}{8}\!O \;+\; e^{+} \;+\; \nu_{e}
\]
\(A\) unchanged (18) \(Z\) decreases from 9 to 8.
\[
^{60}{27}\!Co^{*} \;\longrightarrow\; ^{60}{27}\!Co \;+\; \gamma
\]
Both \(A\) and \(Z\) remain 60 and 27; only excess nuclear energy is released as a photon.
The mass of a nucleus is slightly less than the sum of the individual masses of its protons and neutrons. This “mass defect” \(\Delta m\) is released as binding energy:
\[
E_{\text{binding}} = \Delta m \, c^{2}
\]
Binding energy explains why nuclear reactions (e.g. fission, fusion) can release large amounts of energy compared with chemical reactions.
- α particles – used in smoke detectors (‑\(^{241}\)Am source).
- β⁻ emitters – radiotracers in medical imaging (e.g., \(^{14}\)C‑labelled compounds).
- β⁺ emitters – positron emission tomography (PET) scanners use \(^{18}\)F.
- γ rays – radiotherapy for cancer, sterilisation of medical equipment, and industrial radiography.
Balance the following nuclear equation and state how \(A\) and \(Z\) change:
\[
^{226}{88}\!Ra \;\longrightarrow\; \; ? \;+\; ^{4}{2}\!\alpha
\]
Solution: The daughter nucleus is \(^{222}_{86}\!Rn\). \(A\) decreases by 4 and \(Z\) decreases by 2, consistent with α‑decay.
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