Fine Structure and the Dirac Atom/The Relativistic Kinetic-Energy Correction

Lesson 3.1940 words

The Relativistic Kinetic-Energy Correction

The Bohr energies treat the electron as slowly moving, but its speed is of order αc, so the kinetic energy needs a relativistic correction. Expanding √(p²c²+m²c⁴) to order (v/c)² produces the perturbation −p⁴/8m³c², whose first-order shift on a hydrogenic state is evaluated with the trick p²=2m(E−V).

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The gross structure of hydrogen, the ladder produced by solving the radial equation, rests on the non-relativistic kinetic energy . That expression is the first term of an expansion. The electron in the ground state moves with a characteristic speed , where is the fine-structure constant, so is a small but nonzero fraction. Keeping the next term in the relativistic kinetic energy shifts every level by a fractional amount of order , splitting lines that the gross theory leaves coincident. This lesson computes that shift for hydrogenic states; the spin-orbit and Darwin corrections, of the same order, follow in the next two lessons.

The size of the effect

The Bohr model fixes the electron's speed. In the -th circular orbit the quantized angular momentum and the force balance combine to

For hydrogen () in the ground state, , so . The relativistic correction to the kinetic energy is smaller than the kinetic energy itself by this factor, and the kinetic energy is comparable to the binding energy, so the level shifts land near . That number sets the scale of fine structure and explains why the effect is invisible in the coarse Balmer spectrum and prominent only under high resolution.

The electron's orbital speed as a fraction of c falls as Zα/n; the relativistic correction scales as its square, so it is largest for the tightly bound low-n, high-Z states.

Expanding the relativistic kinetic energy

The exact relativistic energy of a free particle of rest mass and momentum magnitude is

The kinetic energy is this minus the rest energy . Factor out and expand the square root in the small parameter :1

Written out in powers of ,

The leading term is the familiar non-relativistic kinetic energy already in the hydrogen Hamiltonian. The next term is the lowest relativistic correction,

a perturbation to be added to the unperturbed hydrogen Hamiltonian . The relative size of the two, versus the correction, is , confirming the estimate above.

The exact kinetic energy √(p²c²+m²c⁴)−mc² (solid) bends below the parabola p²/2m (dashed); the gap is the −p⁴/8m³c² correction, quadratic in the small quantity p²/m²c².

First-order shift and the p⁴ trick

Because hydrogen's gross-structure levels are degenerate in and , one might worry about degenerate perturbation theory. The saving fact is that commutes with and : it is built from , a scalar under rotations, and carries no spin or angular dependence beyond what already respects. The unperturbed eigenstates are therefore already the good states that diagonalize within each degenerate shell, and ordinary first-order theory applies:1

Evaluating directly requires four derivatives of the wave function and is laborious. The efficient route uses the unperturbed Schrödinger equation to trade momentum for energy. Since and ,

The operator is Hermitian, so it may act to the left on the bra and to the right on the ket:

This replaces the fourth-order differential operator with a simple function of , at the cost of needing two radial expectation values. Expanding the square,

The p⁴ matrix element is reduced by splitting p²·p², replacing each factor with 2m(E−V) using the eigenvalue equation, leaving expectation values of powers of the Coulomb potential.

Evaluating on Coulomb states

For a hydrogenic atom the potential is . Write , so and , . The two radial expectation values are the standard hydrogenic results

with the Bohr radius. Two identities streamline the algebra. First, , and comparing with gives once is carried inside . Concretely,

The first is the virial theorem in disguise: and . Substituting both into the bracket,

The second form uses , which recasts as . The correction is manifestly of order times the gross energy , the promised fine-structure scale.

Dependence on n and ℓ

The shift lowers every level, but not uniformly. At fixed the magnitude falls as grows, because shrinks and high- states are held away from the nucleus by the centrifugal barrier, where the electron moves slower and the relativistic correction is weaker. The penetrating states, which sample the region of large near the origin, are pulled down the most.

The relativistic shift within the n=3 shell, in units of (Zα)⁴mc²/n⁴; s (ℓ=0) drops furthest, d (ℓ=2) least, tracking 1/(ℓ+½).

A short table makes the pattern quantitative. Writing the shift as with :

The bare -dependence here is not the full story: the spin-orbit correction carries its own -dependence of the same size, and when the two are added the combined shift reorganizes to depend only on and the total angular momentum . The relativistic term taken alone does not respect that final simplicity, so its -pattern is physical only in combination with the others.

Where it sits among the corrections

The relativistic kinetic term is one of three corrections of order that together make up the fine structure. It is worth fixing the hierarchy of scales before the pieces are assembled, because the same power counting recurs for hyperfine structure and the Lamb shift.

The ladder of energy scales in hydrogen: each rung is smaller than the one above by roughly α², so gross structure (10 eV) sits far above fine structure (10⁻⁴ eV) and hyperfine structure (~10⁻⁶ eV).

Because all three fine-structure terms scale as , none can be neglected relative to the others; the Darwin term acts only on states, the spin-orbit term only on , and the relativistic term on all of them. The remarkable outcome, derived once all three are in hand, is that their sum collapses to the single fine-structure formula depending on and alone, the same expression that the exact Dirac equation reproduces to this order. The relativistic kinetic correction is the piece that carries the velocity content of that agreement: it is what the term of the classical energy becomes once the electron is quantized.

Footnotes

  1. Griffiths & Schroeter, Introduction to Quantum Mechanics, 3rd ed., §7.3.1 — expansion of the relativistic kinetic energy, the perturbation , the reduction of , and the closed result . 2

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