distinguish between nucleon number and proton number

Atoms, Nuclei and Radiation

1. Nuclide notation

The standard way of writing a nuclide is

\[

^{A}_{Z}\!X

\]

where

  • \(Z\) – proton number (also called the atomic number)
  • \(A\) – nucleon number (mass number)
  • \(X\) – chemical symbol of the element
  • \(N = A - Z\) – neutron number

Example: carbon‑12 is written \(^{12}{6}\!C\). The same element with a different number of neutrons, carbon‑13, is written \(^{13}{6}\!C\).

2. Proton number (\(Z\)) and nucleon number (\(A\))

  • Proton number (\(Z\)) – the total count of protons in the nucleus. It uniquely determines the chemical element.
  • Nucleon number (\(A\)) – the total count of nucleons (protons + neutrons). It distinguishes between isotopes of the same element.
  • The three numbers are related by

\[

A = Z + N

\]

3. Quick comparison

AspectProton number (\(Z\))Nucleon number (\(A\))
What it countsProtons onlyProtons + neutrons
Symbol\(Z\)\(A\)
DeterminesChemical element (e.g. carbon, oxygen)Specific isotope (e.g. \(^{12}\)C vs \(^{13}\)C)
Typical natural range1 – 118 (known elements)1 – ≈ 300 (heaviest naturally occurring nuclides)
Conservation in reactionsConserved unless a nuclear transmutation changes the elementConserved in every nuclear reaction

4. Conservation laws

  • Conservation of nucleon number (\(A\)): the total mass number on the left‑hand side of a nuclear equation equals that on the right‑hand side.
  • Conservation of proton number (\(Z\)): the total atomic number is also conserved, except when the reaction involves a change of element (e.g. β‑decay).
  • Both laws must be satisfied when writing or balancing any nuclear equation.

5. Types of nuclear radiation

RadiationParticle emittedChargeMass (u)Typical energyEffect on \(A\) and \(Z\)Penetration / shielding
α (alpha)\(^{4}_{2}\!He\) (helium nucleus)+2 e4 u≈ 5 MeV\(A\) − 4, \(Z\) − 2Stopped 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, \(Z\) + 1Requires a few mm of aluminium or plastic
β⁺ (beta‑plus, positron emission)Positron \(e^{+}\)+1 e≈ 0 u≈ 0.1–10 MeV\(A\) unchanged, \(Z\) − 1Similar shielding to β⁻ (aluminium, plastic)
γ (gamma)High‑energy photon0 e≈ 0 u≈ 0.1–10 MeV (often higher)\(A\) and \(Z\) unchangedRequires dense material – lead or several cm of concrete

6. Antiparticles and neutrinos in β‑decay

  • In β⁻ decay a neutron converts to a proton, emitting an electron and an antineutrino \(\bar\nu_{e}\).
  • In β⁺ decay a proton converts to a neutron, emitting a positron and a neutrino \(\nu_{e}\).
  • Neutrinos (\(\nu{e}\)) and antineutrinos (\(\bar\nu{e}\)) carry away the missing energy and momentum; they have essentially zero mass and do not affect \(A\) or \(Z\).

7. Sample nuclear equations

All of the following obey the conservation of \(A\) and \(Z\).

  • α‑decay (e.g. uranium‑238)

    \[

    ^{238}{92}\!U \;\longrightarrow\; ^{234}{90}\!Th \;+\; ^{4}_{2}\!\alpha

    \]

    \(A: 238 \to 234+4\) \(Z: 92 \to 90+2\)

  • β⁻ decay (e.g. carbon‑14)

    \[

    ^{14}{6}\!C \;\longrightarrow\; ^{14}{7}\!N \;+\; e^{-} \;+\; \bar\nu_{e}

    \]

    \(A\) unchanged (14) \(Z\) increases from 6 to 7.

  • β⁺ decay (e.g. fluorine‑18)

    \[

    ^{18}{9}\!F \;\longrightarrow\; ^{18}{8}\!O \;+\; e^{+} \;+\; \nu_{e}

    \]

    \(A\) unchanged (18) \(Z\) decreases from 9 to 8.

  • γ emission (often follows α or β decay)

    \[

    ^{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.

8. Mass defect and nuclear binding energy

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.

9. Real‑world applications

  • 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.

10. Practice question

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.

Suggested diagram: a schematic nucleus showing red circles for protons, blue circles for neutrons, with labels for \(Z\), \(N\) and \(A\). Place the notation \(^{A}_{Z}\!X\) beside the drawing.