Unit 6 : Worked Problems#
Problem - Alpha decay separation energy
Calculate the separation energy for the alpha decay of \(^{238}\)U.
Calculate the separation energy for the alpha decay of \(^{238}\)U.
For \(\rm ^{238}U \rightarrow ^{234}Th + \alpha\), the separation energy is given by:
where m is the nuclear or atomic mass (interchangeable in this calculation since the mass of the electrons cancels out in the atomic mass).
So
Problem - Nuclear separation distance in alpha decay
Using the separation energy calculated in 6.1.1, calculate the nuclear separation distance of the \(\alpha\) and \(^{234}\)Th daughter nucleus.
Using the separation energy calculated in 6.1.1, calculate the nuclear separation distance of the \(\alpha\) and \(^{234}\)Th daughter nucleus.
Nuclear separation \(\rm R = r_0 (A_{\alpha}^{1/3}+A_d^{1/3})\) where \(A_{\alpha}\) and \(\rm A_d\) are the atomic masses of the alpha and daughter nucleus respectively, and \(\rm r_0 = 1.2\) is a constant of proportionality. Therefore:
Problem - Height of the Coulomb barrier to alpha decay
Calculate the height of the Coulomb barrier to the alpha decay of \(\rm ^{238}U\) at the nuclear separation distance R calculated in 6.1.2.
Calculate the height of the Coulomb barrier to the alpha decay of \(\rm ^{238}U\) at the nuclear separation distance R calculated in 6.1.2.
The height of the barrier at nuclear separation distance R is calculated as the Coulomb potential of point charges Z\(_{\alpha}\)e and Z\(_d\)e, where Z\(_\alpha\) and Z\(_d\) are the atomic numbers of the alpha particle and daughter nucleus. The height of the barrier is therefore:
where \(ke^2=\frac{e^2}{4\pi\epsilon_0}\).
Problem - Outer extent of the Coulomb barrier to alpha decay
Calculate the distance at which the Coulomb potential drops to the energy of the \(\alpha\) particle and, from this, the width of the Coulomb barrier in the alpha decay of \(^{238}\)U using your answers from earlier steps.
Calculate the distance at which the Coulomb potential drops to the energy of the \(\alpha\) particle and, from this, the width of the Coulomb barrier in the alpha decay of \(^{238}\)U using your answers from earlier steps.
The energy of the alpha particle is \(T_e \approx Q = 4.28~\textnormal{MeV}\) (from Example 6.1.1). The distance at which the Coulomb potential R\(_Q\) is equal to Q is given by rearranging the equation for the Coulomb potential:
The width of the Coulomb barrier is therefore \(w = R_Q - R = 60.6~\textnormal{fm} - 9.30~\textnormal{fm} = 51.3~ \textnormal{fm} \).
Problem - Alpha-Coulomb barrier collision frequency
Now find the frequency at which the \(\alpha\) particle collides with the Coulomb barrier in the alpha decay of \(^{238}\)U using your earlier answers.
Now find the frequency at which the \(\alpha\) particle collides with the Coulomb barrier in the alpha decay of \(^{238}\)U using your earlier answers.
Since the alpha particle at this energy is non-relativistic, the velocity of the alpha can be calculated from its kinetic energy \(T_e \approx Q = 4.28~\textnormal{MeV}\):
The frequency of collisions of an alpha particle with this velocity is given by:
Problem - Alpha-Coulomb barrier collision frequency
Now calculate the tunnelling probability of the alpha particle in the decay of \(^{238}\)U by integrating over the Gamow factor.
Now calculate the tunnelling probability of the alpha particle in the decay of \(^{238}\)U by integrating over the Gamow factor.
The tunnelling probability is given by \(P = e^{-2G}\), where G is the Gamow factor:
Evaluating this integral gives us:
where \(x = R/R_Q = Q/V(R)\).
Putting in the numbers, this gives a tunnelling probability of
Problem - Alpha decay constant and half life
Assuming that the preformation probability \(P_\alpha\) of the alpha particle is equal to 1, calculate the decay constant, and therefore half-life of \(^{238}\)U.
Assuming that the preformation probability \(P_\alpha\) of the alpha particle is equal to 1, calculate the decay constant, and therefore half-life of \(^{238}\)U.
The decay constant is given by:
And so the half-life of \(^{238}\)U is
Problem - Differences between calculated and measured half-life
The measured half-life of \(^{238}\)U is approximately \(4.468 \times 10^9\) years. Comment on the difference between this value and the half-life we have calculated.
The measured half-life of \(^{238}\)U is approximately \(4.468 \times 10^9\) years. Comment on the difference between this value and the half-life we have calculated.
The half-life calculated assumed a spherical nucleus and does not take into consideration:
The non-spherical nature of heavy nuclei.
The effects of nuclear angular momentum.
A 4% change in radius can give a factor of 5 difference in half-life, and in fact the measured half-life can be used to infer information about the radius.
Problem - Beta decay selection rules
Use the beta decay selection rules to classify the following transitions:
\(^{76}\)Br(1-) to \(^{76}\)Se(0+)
\(^{22}\)Na(3+) to \(^{22}\)Na(0+)
\(^{40}\)K(4-) to \(^{40}\)Ca(0+)
Use the beta decay selection rules to classify the following transitions:
\(^{76}\)Br(1-) to \(^{76}\)Se(0+)
\(\Delta \pi = -\), so L is odd, since \(\Delta \pi = (-1)^L\).
Since \(\Delta J = L + S = 1\), and L is odd, L = 1 and S = 0 is the only possible combination.
This transition is therefore a 1st forbidden Fermi decay.
\(^{22}\)Na(3+) to \(^{22}\)Na(0+)
There is no change in parity and \(\Delta \pi = +\), so L is even and can be 0, 2, etc.
\(\Delta J = L + S = 3\), so L = 2 and S = 1.
This transition is therefore a 2nd forbidden Gamow-Teller decay.
\(^{40}\)K(4-) to \(^{40}\)Ca(0+)
There is a change in parity and \(\Delta \pi = -\), so L is odd.
\(\Delta J = L + S = 4\), so L = 3 and S = 1.
Therefore this is a 3rd forbidden Gamow-Teller decay
Problem - Beta decay endpoint value
Calculate the endpoint value for the decay of \(^{81}\)Kr by beta minus, beta plus and electron capture, and therefore demonstrate which form of beta decay the isotope undergoes.
Calculate the endpoint value for the decay of \(^{81}\)Kr by beta minus, beta plus and electron capture, and therefore demonstrate which form of beta decay the isotope undergoes.
Beta minus decay \( ^{81}_{36}Kr \rightarrow ^{81}_{37}Rb + \beta^- + \bar{\nu}_e\):
Beta plus decay \( ^{81}_{36}Kr \rightarrow ^{81}_{35}Br + \beta^+ + \nu_e\):
Electron capture \( ^{81}_{36}Kr + e^- \rightarrow ^{81}_{35}Br + \nu_e\)
Therefore, electron capture is the only form of beta decay that \(^{81}\)Kr can undergo.