3. Fine Structure of Hydrogen
Reading time: ~36 minutes | Pages: 9
Relativistic corrections to hydrogen spectrum: small splittings revealing deeper physics.
The Fine Structure Constant
Dimensionless constant characterizing electromagnetic interaction strength
Fine structure corrections are of order $\alpha^2 \approx 5 \times 10^{-5}$
Three Relativistic Corrections
Perturbations to non-relativistic hydrogen:
- Relativistic kinetic energy correction
- Spin-orbit coupling
- Darwin term (contact interaction)
1. Relativistic Kinetic Energy
Relativistic energy-momentum relation:
Perturbation Hamiltonian:
Energy correction:
2. Spin-Orbit Coupling
Interaction between electron spin and orbital angular momentum:
For Coulomb potential $V = -ke^2/r$:
Using total angular momentum $\vec{J} = \vec{L} + \vec{S}$:
Total Angular Momentum
Quantum number $j$ labels total angular momentum:
- For $\ell = 0$: only $j = 1/2$
- For $\ell > 0$: both $j = \ell + 1/2$ and $j = \ell - 1/2$
Spin-orbit energy correction:
3. Darwin Term
Correction for s-waves ($\ell = 0$) only:
Energy correction:
Origin: "Zitterbewegung" - rapid quantum fluctuations of electron position
Combined Fine Structure Formula
Total fine structure correction:
Remarkably, depends only on $n$ and $j$, not on $\ell$ separately!
Energy Levels with Fine Structure
Spectroscopic notation: $n^{2s+1}L_j$
- $n = 2, \ell = 0, j = 1/2$: $2^2S_{1/2}$
- $n = 2, \ell = 1, j = 1/2$: $2^2P_{1/2}$
- $n = 2, \ell = 1, j = 3/2$: $2^2P_{3/2}$
Example: n=2 Level Splitting
Without fine structure: all 4 states at same energy
With fine structure:
- $2^2S_{1/2}$ and $2^2P_{1/2}$: degenerate (same $j = 1/2$)
- $2^2P_{3/2}$: split by $\Delta E \approx 4.5 \times 10^{-5}$ eV
This is the sodium D-line doublet splitting!
Lamb Shift
Fine structure predicts $2^2S_{1/2}$ = $2^2P_{1/2}$, but experiment shows tiny splitting:
Requires quantum electrodynamics (QED) - vacuum fluctuations of EM field
Hyperfine Structure
Even smaller splitting from nuclear spin $\vec{I}$ coupling to electron:
Famous example: 21 cm line of hydrogen ($F = 1 \leftrightarrow F = 0$ transition)
Critical for radio astronomy and mapping galactic structure