(a) Show that the Hamiltonian of a free electron in a uniform timeindependent magnetic field $\mathscr{S}_{3}=9_{\xi} \hat{\mathbf{z}}$ is given by $H=H_{x y}+H_{u}$, with
$$
H_{x y}=\frac{1}{2 m}\left(p_{x}^{2}+p_{y}^{2}\right)+\frac{1}{2 m} \omega_{L}^{2}\left(x^{2}+y^{2}\right)
$$
and
$$
H_{z}=\frac{1}{2 m} p_{z}^{2}+\omega_{L}\left(L_{z}+2 S_{z}\right)
$$
where $\omega_{\mathrm{L}}=\left(\mu_{\mathrm{B}} / \hbar\right) \mathscr{B}_{z}=2 \pi v_{\mathrm{L}}$ is the Larmor angular frequency.
(b) Using the fact that $H$ can be written as a square, $H=(\mathbf{p}+e \mathbf{A})^{2} / 2 m$, and that the Hamiltonian $H_{x y}$ of the harmonic motion in the $X Y$ plane is invariant under the reflection $x \rightarrow-x, y \rightarrow-y$, show that the energy eigenvalues are given by
$$
E=\frac{h^{2} k^{2}}{2 m}+\hbar \omega_{L}\left(2 r+2 m_{s}+1\right)
$$
where $-\infty<k<+\infty, r=0,1,2, \ldots$ and $m_{s}=\pm 1 / 2$. For given $k$ and $m_{s}$ the discrete energy levels labelled by the quantum number $r$ are called Landau levels.
(c) In neutron stars magnetic fields of the order of $10^{8} \mathrm{~T}$ may occur. Find the energy separation between the adjacent Landau levels. What is the