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intermediate · Physics · Time-Independent Perturbation Theory

Fine Structure Corrections

Beyond the Bohr model

The Bohr / Schrödinger hydrogen levels En=13.6eV/n2E_n = -13.6\,\text{eV}/n^2 ignore two effects that the relativistic treatment includes. Together they constitute the fine structure, and both are computed with perturbation theory because each is small compared to the gross level spacing.

1. The relativistic kinetic correction

The exact relativistic kinetic energy p2c2+m2c4mc2\sqrt{p^2 c^2 + m^2 c^4} - mc^2 expands as p22mp48m3c2+\tfrac{p^2}{2m} - \tfrac{p^4}{8m^3c^2} + \cdots. The leading correction beyond the Schrödinger kinetic term is

H^rel=p^48m3c2.\hat{H}'_{\text{rel}} = -\frac{\hat{p}^4}{8 m^3 c^2}.

2. The spin–orbit coupling

In the electron's rest frame the nucleus orbits it, producing a magnetic field that couples to the electron's spin. After the Thomas factor of 1/21/2, this gives

H^SO=12m2c21rdVdrSL.\hat{H}'_{\text{SO}} = \frac{1}{2 m^2 c^2}\,\frac{1}{r}\frac{dV}{dr}\,\vec{S}\cdot\vec{L}.

The SL\vec{S}\cdot\vec{L} structure is exactly why total angular momentum jj (not ll and ss separately) labels the good states, and why the Landé factor of the previous lesson appears.

The size of the effect

Both corrections turn out to be of the same order and combine into the remarkably compact fine-structure energy

Efs(1)=(En(0))22mc2(34nj+12),E^{(1)}_{\text{fs}} = \frac{(E_n^{(0)})^2}{2 m c^2}\left(3 - \frac{4n}{j + \tfrac12}\right),

which depends on nn and jj but not on ll — a non-trivial cancellation between the two effects.

The crucial scaling is in the prefactor. Since En(0)α2mc2E_n^{(0)} \sim \alpha^2 mc^2 (the Bohr energy in terms of the fine-structure constant α=e2/4πε0c1/137\alpha = e^2/4\pi\varepsilon_0\hbar c \approx 1/137), we have

Efs(1)En(0)En(0)mc2α25.3×105.\frac{E^{(1)}_{\text{fs}}}{E_n^{(0)}} \sim \frac{E_n^{(0)}}{mc^2} \sim \alpha^2 \approx 5.3 \times 10^{-5}.

Fine structure is therefore about five parts in 10510^5 of the gross structure — small enough that first-order perturbation theory is excellent, but large enough to be measured precisely in spectra. This α2\alpha^2 suppression is why the Bohr model works so well despite ignoring relativity and spin.

Try it

Using α=1/137.036\alpha = 1/137.036, compute the order-of-magnitude suppression factor α2\alpha^2 that separates fine structure from the gross structure, and return it as a number.

Run your code to see the quantum state.

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