Study the influence of the spin--orbit interaction
H2=2m2c21S⋅Lr1drdV(r)
on the energy spectrum \left(E_{n,l} = \hbar\omega\left(l + 2n + \frac{3}{2}\right), compare problem 17.1\right) of a three-dimensional isotropic harmonic oscillator. Discuss the degeneracy of the energy levels without and with the spin--orbit interaction. Note: ψnlm(x)=Rnl(r)Ylm(ϑ,φ).