Nuclear radius (AQA A-Level Physics): Revision Notes
Nuclear radius
Understanding the size of a nucleus
When we model the nucleus as a collection of tightly packed protons and neutrons (collectively called nucleons), we can explore the relationship between nuclear size and the number of nucleons present. The volume of a nucleus with nucleon number A (mass number) is directly proportional to the number of nucleons it contains:
This relationship tells us that each nucleon occupies approximately the same amount of space within the nucleus, regardless of which element we consider. This fundamental principle leads to the important conclusion that nuclei have a constant density.
Deriving the nuclear radius formula
If we treat the nucleus as spherical with radius , its volume can be expressed using the standard formula for the volume of a sphere:
Since the total nuclear volume equals the nucleon number multiplied by the volume of a single nucleon, we can write:
Rearranging this expression gives:
This can be simplified to:
If we assume that the volume occupied by each nucleon remains constant across all nuclei, then is proportional to . This leads to the relationship:
This proportionality is typically written as:
where is the constant of proportionality. Experimental measurements have determined that fm (where fm stands for femtometre, equal to m).
This formula tells us that nuclear radius increases with the cube root of the nucleon number, rather than directly with itself. This means that doubling the number of nucleons does not double the radius, but only increases it by a factor of .
Experimental methods to measure nuclear radius
Historical approach - Rutherford's alpha scattering
Rutherford's famous alpha particle scattering experiment, which involved firing alpha particles at thin gold foil, provided an early estimate for nuclear size. By analyzing the electrostatic repulsion between alpha particles and gold nuclei, Rutherford established an upper limit for the gold nucleus radius of approximately m. However, this method could not provide precise measurements of nuclear radii for different elements.
Modern approach - electron diffraction
A more accurate and versatile method uses high-energy electron beams directed at thin samples of various elements. The electrons scatter through different angles, and detectors count the number of electrons scattered at each angle within a specified time interval. This produces a diffraction pattern with characteristic maxima (peaks) and minima (troughs).
The scattering occurs because electrons carry charge and experience an attractive electromagnetic force when passing near the positively charged protons in the nucleus. The resulting diffraction pattern depends on the size of the nucleus, and by analyzing the angles at which minima occur, we can determine nuclear radii for different elements.
Why electrons are superior to alpha particles
Electrons offer several advantages over alpha particles as probing particles:
Interaction mechanism: Electrons, being leptons with no internal structure, interact with nuclei solely through the electromagnetic force arising from their charge. This interaction is well understood theoretically. Alpha particles, being composite particles made of protons and neutrons (hadrons), also interact via the strong nuclear force, which is less well understood and complicates the analysis.
Particle mass: Electrons have a much smaller mass than alpha particles. When accelerated to very high speeds in a particle accelerator, electrons can achieve de Broglie wavelengths comparable to nuclear dimensions.
De Broglie wavelength matching: The de Broglie wavelength of electrons accelerated through a potential difference of 400 MV is approximately m, which matches the typical size of nuclear radii. This similarity is essential for producing clear diffraction patterns. When a wave encounters an obstacle of similar size to its wavelength, it produces pronounced diffraction effects that can be analyzed to determine the size of the obstacle.
Why wavelength matching matters:
The de Broglie wavelength ( m) must be comparable to nuclear dimensions for effective diffraction. If the wavelength is too large compared to the nucleus, the electrons would not "see" the nuclear structure clearly. This wavelength matching is the key reason why high-energy electrons are needed for nuclear radius measurements.
Experimental results
When electron diffraction data from many different elements are collected and plotted as a graph of nuclear radius against , the result is a straight line passing through the origin. The gradient of this line is 1.05 fm, confirming the relationship where fm. This experimental verification supports the theoretical prediction that nuclear radius depends on the cube root of the nucleon number.
Nuclear density
Calculating nuclear density
The density of any material is defined as its mass divided by its volume:
For a nucleus containing nucleons, where each nucleon has an atomic mass unit (u) equal to kg, the total mass is:
The volume of the nucleus, using , is:
Therefore, the density becomes:
Notice that the nucleon number appears in both the numerator and denominator, so it cancels out:
Substituting m:
The constant density result
This remarkable result shows that the density of a nucleus does not depend on the nucleon number. Whether we examine a light nucleus like carbon or a heavy nucleus like uranium, the density remains the same at approximately kg m. This confirms our initial assumption that nucleons are packed together with constant density throughout the nucleus.
Comparison with ordinary matter:
This nuclear density is extraordinarily large compared with the densest naturally occurring element on Earth, osmium, which has a density of only kg m. Nuclear matter is roughly times denser than ordinary matter. This enormous difference exists because atoms are mostly empty space - the electrons occupy regions far from the tiny, dense nucleus.
Worked Example: Copper-63 Nucleus
Let's apply these concepts to calculate the radius and density of a copper-63 nucleus, assuming fm.
Step 1: Calculating the radius
Using the formula :
R &=& 1.05 \times 10^{-15} \times 63^{1/3} \\ R &=& 1.05 \times 10^{-15} \times 3.98 \\ R &=& 4.2 \times 10^{-15} \text{ m} \end{array}$$ **Step 2: Finding the mass of one copper-63 atom** The mass equals the molar mass divided by Avogadro's constant: $$\text{Mass of one copper atom} = \frac{63}{6.02 \times 10^{23}} = 1.05 \times 10^{-22} \text{ g} = 1.05 \times 10^{-25} \text{ kg}$$ For the purposes of calculating nuclear density, we can assume the mass of the copper nucleus equals the mass of the copper atom (since electron mass is negligible compared to nuclear mass). **Step 3: Calculating the density** $$\begin{array}{rcl} \rho &=& \frac{M}{V} = \frac{M}{\frac{4}{3}\pi(4.2 \times 10^{-15})^3} \\ \rho &=& \frac{1.05 \times 10^{-25}}{\frac{4}{3}\pi(4.2 \times 10^{-15})^3} \\ \rho &=& 3.4 \times 10^{17} \text{ kg} \cdot \text{m}^{-3} \end{array}$$ :success[This confirms that the density matches the constant value we derived earlier], demonstrating that nuclear density is independent of the specific nucleus being examined.Key Points to Remember:
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Nuclear radius follows the relationship where fm, meaning radius increases with the cube root of nucleon number rather than linearly with .
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Electron diffraction provides accurate measurements of nuclear radii because electrons interact via electromagnetic force only, have small mass allowing high-speed acceleration, and possess de Broglie wavelengths (approximately m) comparable to nuclear dimensions.
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All nuclei have the same density of approximately kg m, regardless of their size or nucleon number, because nucleons are packed together with constant density.
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Nuclear density is about times greater than the densest ordinary matter, reflecting the fact that atoms are mostly empty space while nuclei are extremely compact.
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The relationship can be verified experimentally by plotting versus , which produces a straight line through the origin with gradient 1.05 fm.