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Rutherford scattering and nuclear radiusAQA A-Level Physics: Revision notes

Section 1

Rutherford scattering

In the Geiger–Marsden experiment, a narrow beam of alpha particles was fired at very thin gold foil in a vacuum, and the number scattered through different angles was counted. The foil is thin so that each alpha particle is scattered by a single nucleus, and a vacuum prevents absorption by air.

Observations and conclusions:

  • Most alpha particles pass straight through, so most of an atom is empty space.
  • A small fraction (about 1 in 8000) is deflected through more than 90°, so the positive charge and almost all the mass are concentrated in a tiny nucleus, which repels the positive alpha particles.
  • The scattering matches the inverse-square electric repulsion between nucleus and alpha particle.
Key termsRutherford scatteringnucleus
Common mistake

The alpha particles are repelled by the nucleus, not attracted. Both are positively charged, and very few get anywhere near it.

Section 2

How our model of the nucleus has changed

Ideas about the atom have developed as new evidence appeared:

  • Plum pudding model (Thomson): a sphere of positive charge with electrons embedded in it. It predicts only small deflections of alpha particles.
  • Nuclear model (Rutherford): a small, dense, positive nucleus, with electrons orbiting at a much larger distance.
  • Neutron discovered by Chadwick, explaining the extra mass of nuclei.
  • Quarks: high-energy electron scattering showed that protons and neutrons are not fundamental but have internal structure.

A theory is accepted until new evidence cannot be explained by it.

Key termsplum pudding model

Section 3

Estimating nuclear size from closest approach

A head-on alpha particle slows as it approaches a nucleus, because of the electric repulsion. At the distance of closest approach it is momentarily at rest, so all its kinetic energy has become electric potential energy:

Ek=Qq4πε0rE_k = \frac{Qq}{4\pi\varepsilon_0 r} so r=Qq4πε0Ekr = \frac{Qq}{4\pi\varepsilon_0 E_k}

where QQ and qq are the charges of the nucleus and the alpha particle. Because the alpha particle never touches the nucleus, rr is an upper limit to the nuclear radius.

Worked example: 7.7 MeV alpha particle on gold (Z=79Z = 79): Ek=7.7×106×1.60×10−19=1.23×10−12E_k = 7.7\times10^6 \times 1.60\times10^{-19} = 1.23\times10^{-12} J, so r=(2e)(79e)4πε0Ek=3.0×10−14r = \frac{(2e)(79e)}{4\pi\varepsilon_0 E_k} = 3.0\times10^{-14} m.

Key termsdistance of closest approach
Exam tip

Convert MeV to J by multiplying by 1.60 × 10⁻¹³. Charges are 2e for an alpha particle and Ze for the nucleus.

Section 4

Electron diffraction

High-energy electrons (hundreds of MeV) have a de Broglie wavelength λ=h/p\lambda = h/p about the size of a nucleus (around 10−1510^{-15} m). For such electrons, p≈E/cp \approx E/c.

When the beam is scattered by a nucleus, a diffraction pattern appears: the intensity of scattered electrons plotted against angle falls to a first minimum and then rises to a smaller maximum. The first minimum is at

sin⁡θ≈1.22λD\sin\theta \approx \frac{1.22\lambda}{D}

where DD is the nuclear diameter, so the radius is D/2D/2. Electron diffraction gives a more accurate radius than closest approach, because electrons do not feel the strong force.

Key termsdiffraction patternde Broglie wavelength
Common mistake

Do not say electrons are used because they penetrate the nucleus. They are used because their wavelength is similar to the size of the nucleus.

Section 5

Nuclear radius and density

Typical nuclear radii are between about 1 fm and 8 fm (10−1510^{-15} m), around 10⁵ times smaller than an atom.

Experiments show that the radius depends on nucleon number AA:

R=R0A1/3R = R_0A^{1/3} with R0≈1.2R_0 \approx 1.2 fm

Since volume ∝R3∝A\propto R^3 \propto A and mass ∝A\propto A, the density is the same for all nuclei: the equation is evidence that nuclear matter has constant density.

ρ=Au43πR03A=3u4πR03≈2.3×1017\rho = \frac{Au}{\frac{4}{3}\pi R_0^3 A} = \frac{3u}{4\pi R_0^3} \approx 2.3\times10^{17} kg m⁻³

Key termsnucleon numbernuclear density

Section 6

Worked example: radius of an iron nucleus

For ⁵⁶Fe: R=R0A1/3=1.2×10−15×561/3=1.2×10−15×3.83=4.6×10−15R = R_0A^{1/3} = 1.2\times10^{-15}\times56^{1/3} = 1.2\times10^{-15}\times3.83 = 4.6\times10^{-15} m.

The nuclear density of 2.3×10172.3\times10^{17} kg m⁻³ is about 3 × 10¹³ times the density of ordinary solids such as iron (7.9×1037.9\times10^3 kg m⁻³), because an atom is almost entirely empty space around a tiny nucleus.

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Exam questions on Rutherford scattering and nuclear radius

  1. In an alpha particle scattering experiment, a narrow beam of alpha particles from a radioactive source is fired at a thin gold foil inside an evacuated chamber. A detector counts the alpha particles scattered through different angles. Almost all the particles pass through the foil, but about 1 in 8000 is scattered through an angle greater than 90°.
    The gold foil used is only a few hundred atoms thick. Explain why a much thicker foil would make the results difficult to interpret.2 marks
  2. An alpha particle of kinetic energy 7.7 MeV is fired directly towards the centre of a stationary gold nucleus, which has proton number 79. The alpha particle is brought momentarily to rest at a distance r from the centre of the nucleus before it is repelled. The gold nucleus can be assumed to remain at rest.
    The distance of closest approach for this alpha particle is 3.0 × 10⁻¹⁴ m. Explain why this gives only an upper limit for the radius of the gold nucleus.2 marks
  3. A beam of electrons of kinetic energy 420 MeV is directed at a thin target of carbon-12 nuclei. The scattered electrons are detected at different angles and the intensity shows a diffraction pattern, with the first minimum at 40° to the original direction. For these electrons, use E = pc. The first minimum occurs when sin θ = 1.22λ/D, where λ is the electron wavelength and D is the diameter of the nucleus.
    Calculate the wavelength of the electrons.3 marks
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Written by the Exaim team, led by Shaun Daswani (Head of Upper Secondary, Improve ME Institute; MSc Financial Mathematics, Imperial College London; BSc, UCL) and Jason Daswani (operational lead, Improve ME Institute; LSE).