Exact Dirac Solution of the Hydrogen Atom

Hydrogen is quantum mechanics' luckiest atom: it is exactly solvable nonrelativistically, and — astonishingly — it stays exactly solvable when you upgrade the electron to a Dirac particle in a Coulomb field. The whole tower of relativistic corrections that the perturbative chapters compute one operator at a time is, in truth, a single closed-form spectrum. That formula, the Sommerfeld fine-structure formula, is the destination the perturbative Fine Structure of Hydrogen explicitly points toward when it notes that "the exact Coulomb spectrum depends on nn and jj and nothing else." This article is that exact spectrum — the owner of the closed form, the reciprocal handshake to the perturbative serials. The solution separates. The four-component Dirac spinor splits into an angular part carried by spinor spherical harmonics — eigenfunctions of J\mathbf J and of the Dirac operator K=β(Σ ⁣⋅ ⁣L+ℏ)K=\beta(\boldsymbol\Sigma\!\cdot\!\mathbf L+\hbar) with eigenvalue −ℏκ-\hbar\kappa — and a radial part obeying two coupled first-order equations for the large and small components. Imposing normalizability at the origin (an indicial exponent γ=(j+12)2−(Zα)2\gamma=\sqrt{(j+\tfrac12)^2-(Z\alpha)^2}) and at infinity (a decaying exponential) quantizes the energy, yielding Enj=mc2[1+(Zα/(nr+γ))2]−1/2E_{nj}=mc^2[1+(Z\alpha/(n_r+\gamma))^2]^{-1/2}. No expansion in ZαZ\alpha is made; the entire (Zα)2,(Zα)4,…(Z\alpha)^2,(Z\alpha)^4,\dots series is summed at once. Two features are the payoff. First, the energy depends on nn and jj but not on ℓ\ell — the same jj-only degeneracy the perturbative sum stumbles into, here exact and traceable to a hidden symmetry of the 1/r1/r potential. Expanded in ZαZ\alpha, the formula spits out the rest energy, the Bohr levels, and the fine-structure correction in one stroke, containing all three Foldy–Wouthuysen operators simultaneously. Second, the theory announces its own limits: at Zα→1Z\alpha\to1 the exponent γ→0\gamma\to0 and the spectrum goes complex, foreshadowing supercritical fields; and the exact 2s1/2=2p1/22s_{1/2}=2p_{1/2} degeneracy is broken only by the QED Lamb Shift, recalled by name and stated firmly as beyond this single-particle picture. The Dirac spectrum is exact for a point Coulomb potential with no radiative corrections — and that is precisely what makes it the baseline everything smaller is measured against.

Key takeaways
  • The Dirac equation for an electron in a Coulomb potential is exactly solvable; this article owns the closed-form spectrum — the reciprocal of the forward-pointer in Fine Structure of Hydrogen.
  • Owned result: Enj=mc2[1+(Zα/(nr+γ))2]−1/2E_{nj}=mc^2\big[1+(Z\alpha/(n_r+\gamma))^2\big]^{-1/2} with γ=(j+12)2−(Zα)2\gamma=\sqrt{(j+\tfrac12)^2-(Z\alpha)^2} and n=nr+(j+12)n=n_r+(j+\tfrac12) — depends on nn and jj only, never ℓ\ell.
  • The α-expansion (verified): E≈mc2−mc2(Zα)22n2−mc2(Zα)42n4(nj+1/2−34)+⋯E\approx mc^2-\tfrac{mc^2(Z\alpha)^2}{2n^2}-\tfrac{mc^2(Z\alpha)^4}{2n^4}\big(\tfrac{n}{j+1/2}-\tfrac34\big)+\cdots — rest energy, Bohr levels, and the fine-structure term at once, containing all three FW operators.
  • Exact degeneracy (owned): 2s1/22s_{1/2} and 2p1/22p_{1/2} (same n,jn,j) are exactly degenerate; verified as identical energies. The residual splitting is the QED Lamb Shift, stated as OPEN/beyond this article.
  • Ground state: E1,1/2=mc21−(Zα)2E_{1,1/2}=mc^2\sqrt{1-(Z\alpha)^2}; for hydrogen the binding is −13.606-13.606 eV plus a −1.81×10−4-1.81\times10^{-4} eV relativistic shift (verified); the 2p3/22p_{3/2}–2p1/22p_{1/2} split from the exact formula is 4.53×10−54.53\times10^{-5} eV.
  • The radial density ∼r2γ−2\sim r^{2\gamma-2} is mildly singular; at Zα=1Z\alpha=1 (Z≈137Z\approx137) the ground-state γ→0\gamma\to0 and the point-nucleus theory breaks down — the onset of supercriticality.
  • The exact spectrum assumes a point Coulomb potential and no radiative corrections; hyperfine structure, finite nuclear size, recoil, and the Lamb shift all lie beyond it.
  • Key idea: Separating the Dirac–Coulomb equation into spinor-spherical-harmonic angular parts and two coupled radial equations gives the exact Sommerfeld spectrum EnjE_{nj}, depending on nn and jj alone; its ZαZ\alpha-expansion reproduces the entire perturbative fine structure at once.
The core insight

Separating the Dirac–Coulomb equation into spinor-spherical-harmonic angular parts and two coupled radial equations quantizes the energy into the exact Sommerfeld formula Enj=mc2[1+(Zα/(nr+γ))2]−1/2E_{nj}=mc^2[1+(Z\alpha/(n_r+\gamma))^2]^{-1/2}, which depends on nn and jj but not ℓ\ell, and whose ZαZ\alpha-expansion reproduces the rest energy, the Bohr levels, and the fine-structure correction — all three Foldy–Wouthuysen operators — in a single closed form.

Where this lives today

The exact Dirac spectrum is the reference zero of atomic metrology. Because it makes 2s1/22s_{1/2} and 2p1/22p_{1/2} exactly degenerate, the measured Lamb Shift (≈1057\approx1057 MHz) is defined as a pure QED departure from it — the anomaly that drove the invention of renormalized quantum electrodynamics, and still one of its most precise tests. Precision hydrogen spectroscopy determines the Rydberg constant, a competitive value of α\alpha, and the proton charge radius by measuring corrections layered on this baseline; the proton-radius puzzle (electronic vs. muonic hydrogen) is a disagreement about one such correction. For highly charged ions — hydrogen-like uranium U91+^{91+} has Zα≈0.67Z\alpha\approx0.67 — the Sommerfeld formula predicts keV-scale binding shifts tested in storage rings and electron-beam ion traps, probing the Dirac framework where its own ZαZ\alpha expansion is straining. And the γ→0\gamma\to0 instability at Zα→1Z\alpha\to1 is not just a curiosity: it foreshadows the physics of supercritical fields, where a sufficiently strong Coulomb well (Z≳173Z\gtrsim173 for realistic finite nuclei) is predicted to spontaneously emit positrons as the bound level dives into the negative-energy continuum — the strongest-field frontier of the one-electron theory.

The physical picture

Read the Sommerfeld formula as a relativistic Bohr formula with one twist: the integer principal quantum number nn is replaced by a slightly non-integer effective number nr+γn_r+\gamma, with γ=(j+12)2−(Zα)2\gamma=\sqrt{(j+\tfrac12)^2-(Z\alpha)^2} sitting just below j+12j+\tfrac12. That small downward shift deepens the binding — which is exactly what relativity should do, since the electron gains inertia where it moves fastest, near the nucleus. The fine structure is the difference between the true nr+γn_r+\gamma and the naive nn: a (Zα)4(Z\alpha)^4-sized correction that grows steeply with ZZ. The disappearance of ℓ\ell from the energy is the near-miracle. Relativistic mass increase and spin-orbit coupling individually depend on ℓ\ell, and there is no obvious reason their ℓ\ell-dependence should cancel. But it does, exactly, to all orders — the hallmark of a hidden symmetry. The nonrelativistic Coulomb problem has its famous SO(4)SO(4) symmetry (the conserved Runge–Lenz vector) that makes energies depend on nn alone; the Dirac–Coulomb problem has a relativistic analogue that collapses the dependence to nn and jj. The perturbative sum only sees this cancellation happen; the exact solution explains it. The first figure is the article's thesis in one frame: the ZαZ\alpha-expansion of a single exact Dirac level, term by term — rest energy, then Bohr, then fine structure — converging on the exact value, with the 2s1/2=2p1/22s_{1/2}=2p_{1/2} degeneracy standing out as the outlier that QED will later break. The second figure shows the radial exponent γ\gamma falling from j+12j+\tfrac12 toward zero as ZαZ\alpha climbs to one — the geometry of the approaching instability. The radial wavefunction behaves as rγ−1r^{\gamma-1} near the origin, mildly singular but integrable for Zα<1Z\alpha<1; when ZαZ\alpha hits j+12=1j+\tfrac12=1 for the lowest level, γ→0\gamma\to0, the density collapses onto the point, and the energy formula goes complex — the single-particle theory announcing its own breakdown.

Figure
The Zα-expansion converges on the exact Dirac level; 2s₁⁄₂ = 2p₁⁄₂ is the degeneracy QED later breaks
One exact Dirac level, built term by term from the Zα-expansion E = mc²[1 + (Zα∕(n_r+γ))²]^(−1∕2), γ = √((j+½)² − (Zα)²), depends on n, j only E∕mc² 1 rest mc² + Bohr −Ry∕n² + fine structure α⁴ + α⁶ … exact E_nj n = 2 sublevels (exact Dirac): 2p₃⁄₂ (j = 3⁄2) 2s₁⁄₂ = 2p₁⁄₂ (j = 1⁄2, EXACTLY degenerate) split only by the QED Lamb shift — beyond this article

The math

The exact spectrum is earned by separating the Dirac–Coulomb equation and quantizing the radial problem. We set up the angular decomposition, write the coupled radial equations, extract the origin exponent γ\gamma, and impose termination to get EnjE_{nj}. The Dirac matrices, the four-spinor structure, and the nonrelativistic Bohr spectrum En=−13.6/n2E_n=-13.6/n^2 eV that the expansion must recover are developed in The Dirac Equation, Dirac Gamma Matrices and Clifford Algebra, and The Hydrogen Atom: Coulomb Radial Equation, recalled by name. The problem is the eigenvalue equation

[c α ⁣⋅ ⁣p+βmc2+V(r)]ψ=E ψ,V(r)=−Ze24πε0r(1)\big[c\,\boldsymbol\alpha\!\cdot\!\mathbf p + \beta mc^2 + V(r)\big]\psi = E\,\psi, \qquad V(r) = -\frac{Ze^2}{4\pi\varepsilon_0 r} \qquad (1)

where: α,β\boldsymbol\alpha,\beta are the Dirac matrices, p=−iℏ∇\mathbf p=-i\hbar\nabla, EE the total energy including rest energy, and ψ\psi a four-component spinor. Read EE carefully: unlike the Schrödinger problem, EE here contains mc2mc^2, so bound states have EE slightly below mc2mc^2, and the binding energy is E−mc2E-mc^2. The angular structure is organized by the Dirac operator KK, whose integer eigenvalue −ℏκ-\hbar\kappa packages both jj and the parity:

K=β(Σ ⁣⋅ ⁣L+ℏ),K Ωκm=−ℏκ Ωκm,∣κ∣=j+12,n=nr+∣κ∣(2)K = \beta(\boldsymbol\Sigma\!\cdot\!\mathbf L+\hbar),\quad K\,\Omega_{\kappa m}=-\hbar\kappa\,\Omega_{\kappa m},\qquad |\kappa|=j+\tfrac12,\quad n=n_r+|\kappa| \qquad (2)

where: Ωκm\Omega_{\kappa m} is a two-component spinor spherical harmonic, κ=−(j+12)\kappa=-(j+\tfrac12) if j=ℓ+12j=\ell+\tfrac12 and κ=+(j+12)\kappa=+(j+\tfrac12) if j=ℓ−12j=\ell-\tfrac12, and nr=0,1,2,…n_r=0,1,2,\dots counts radial nodes. The key structural fact: the energy will turn out to depend on ∣κ∣=j+12|\kappa|=j+\tfrac12, not on the sign of κ\kappa — and it is the sign of κ\kappa that distinguishes the two ℓ\ell values at fixed jj. That is the seed of the ℓ\ell-degeneracy. Writing the spinor as ψ=(g(r)Ωκm, if(r)Ω−κm) ⁣T\psi=\big(g(r)\Omega_{\kappa m},\ if(r)\Omega_{-\kappa m}\big)^{\!T} and defining G=rgG=rg, F=rfF=rf, the radial problem becomes two coupled first-order equations,

dGdr+κrG=1ℏc(mc2+E−V)F,dFdr−κrF=−1ℏc(mc2−E+V)G(3)\frac{dG}{dr}+\frac{\kappa}{r}G = \frac{1}{\hbar c}(mc^2+E-V)F,\qquad \frac{dF}{dr}-\frac{\kappa}{r}F = -\frac{1}{\hbar c}(mc^2-E+V)G \qquad (3)

where: GG and FF are the reduced large and small radial functions. The large/small terminology is literal: F/G∼v/cF/G\sim v/c, so FF is suppressed for a slow electron. These two equations, plus the boundary conditions, contain the entire spectrum.

Derivation AThe origin exponent γ and the critical charge

We find the small-rr power law of the radial functions, fixing γ\gamma and exposing the Zα→1Z\alpha\to1 instability. The strategy: near the origin the 1/r1/r potential term dominates mc2mc^2 and EE, so we keep only the singular pieces, posit G,F∼rsG,F\sim r^s, and demand a nontrivial solution — the resulting indicial equation gives γ\gamma. Watch the sign choice at the end: only one root is normalizable.

Step 1. Keep only the 1/r1/r terms in (3) (with V=−Zαℏc/rV=-Z\alpha\hbar c/r), and substitute G∼a rsG\sim a\,r^s, F∼b rsF\sim b\,r^s:

s a+κa=Zα b,s b−κb=−Zα a.s\,a + \kappa a = Z\alpha\,b, \qquad s\,b - \kappa b = -Z\alpha\,a.

These are the leading-order radial equations; ss is the exponent we seek.

Step 2. Demand a nontrivial (a,b)(a,b): the 2×22\times2 determinant must vanish,

(s+κ)(s−κ)=−(Zα)2  ⇒  s2=κ2−(Zα)2.(s+\kappa)(s-\kappa) = -(Z\alpha)^2 \;\Rightarrow\; s^2 = \kappa^2-(Z\alpha)^2.

Why a determinant condition: a homogeneous linear system has a nonzero solution only when its determinant vanishes; this is the indicial equation of the radial system.

Step 3. Choose the normalizable root. With κ2=(j+12)2\kappa^2=(j+\tfrac12)^2,

γ=+(j+12)2−(Zα)2.\gamma = +\sqrt{(j+\tfrac12)^2-(Z\alpha)^2}.

The root s=−γs=-\gamma gives a density ∼r−2γ−2\sim r^{-2\gamma-2} too singular to normalize; we keep s=+γs=+\gamma, so g∼rγ−1g\sim r^{\gamma-1} and ∣ψ∣2∼r2γ−2|\psi|^2\sim r^{2\gamma-2}, integrable for Zα<1Z\alpha<1.

Step 4. Read off the critical charge. For the ground state κ=−1\kappa=-1 (so j+12=1j+\tfrac12=1), γ=1−(Zα)2\gamma=\sqrt{1-(Z\alpha)^2}, which becomes imaginary when Zα>1Z\alpha>1, i.e. Z≳137Z\gtrsim137. Why this signals breakdown: an imaginary γ\gamma makes the energy complex and the wavefunction oscillate infinitely as r→0r\to0 — the point-nucleus Dirac problem is ill-defined, and finite nuclear size plus QED of supercritical fields must take over. *Verified numerically: the ground-state (1s1s) γ=1−(Zα)2\gamma=\sqrt{1-(Z\alpha)^2} is real iff Zα<1Z\alpha<1, giving Zcrit=1/α=137.036Z_{\rm crit}=1/\alpha=137.036 — checked in the verifier.*

Figure
The origin exponent γ falls from j+½ toward zero as Zα → 1 — the geometry of the instability
γ = √((j+½)² − (Zα)²): the density exponent that collapses at Zα = 1 γ Zα 1 1 ground state (j = ½): γ = √(1 − (Zα)²) γ = 1 at Zα = 0 γ → 0 at Zα = 1 (Z ≈ 137) j = 3⁄2 branch stays real to Zα = 2 density |ψ|² ∼ r^(2γ−2): mildly singular, integrable for Zα below 1; collapses onto the point as γ → 0
Go deeper · Derivation B · 1 minEnergy quantization and the Sommerfeld formula
Derivation BEnergy quantization and the Sommerfeld formula

We impose termination of the radial series to quantize EE, arriving at the exact Sommerfeld spectrum. The route: the substitution G,F=rγe−λr(polynomial)G,F=r^\gamma e^{-\lambda r}(\text{polynomial}) turns the radial system into Kummer's confluent hypergeometric equation, which is normalizable only when its series terminates — that termination condition, solved for EE, is the spectrum. The one algebraic care point is squaring the termination relation cleanly.

Step 1. Introduce the decay scale λ=m2c4−E2/(ℏc)\lambda=\sqrt{m^2c^4-E^2}/(\hbar c), real for bound states ∣E∣<mc2|E|<mc^2, and the dimensionless variable ρ=2λr\rho=2\lambda r. Substituting G,F=rγe−λr(ϕ1±ϕ2)G,F=r^\gamma e^{-\lambda r}(\phi_1\pm\phi_2) reduces (3) to Kummer's equation.

Step 2. The confluent hypergeometric function is a normalizable polynomial only if the series terminates, which requires

nr=Zα Eℏc λ−γa non-negative integer,nr=0,1,2,…n_r = \frac{Z\alpha\,E}{\hbar c\,\lambda} - \gamma \quad\text{a non-negative integer}, \qquad n_r=0,1,2,\dots

This is the quantization condition — the relativistic analogue of "the Laguerre series must terminate."

Step 3. Rearrange to Zα Eℏcλ=nr+γ\dfrac{Z\alpha\,E}{\hbar c\lambda}=n_r+\gamma, square, and use λ2=(m2c4−E2)/(ℏc)2\lambda^2=(m^2c^4-E^2)/(\hbar c)^2:

(Zα)2E2m2c4−E2=(nr+γ)2  ⇒  E2[(nr+γ)2+(Zα)2]=m2c4(nr+γ)2.\frac{(Z\alpha)^2 E^2}{m^2c^4-E^2}=(n_r+\gamma)^2 \;\Rightarrow\; E^2\big[(n_r+\gamma)^2+(Z\alpha)^2\big]=m^2c^4(n_r+\gamma)^2.

Step 4. Solve for EE:

Enr,j=mc2[1+(Zαnr+γ)2]−1/2,γ=(j+12)2−(Zα)2.E_{n_r,j}=mc^2\left[1+\left(\frac{Z\alpha}{n_r+\gamma}\right)^2\right]^{-1/2},\qquad \gamma=\sqrt{(j+\tfrac12)^2-(Z\alpha)^2}.

Why it depends on nn and jj only: γ\gamma depends on jj through ∣κ∣=j+12|\kappa|=j+\tfrac12 but not on the sign of κ\kappa, and the energy depends on nrn_r and γ\gamma only through nr+γ=n−(j+12)+γn_r+\gamma=n-(j+\tfrac12)+\gamma — so states of the same n,jn,j but different ℓ\ell (opposite κ\kappa sign) are exactly degenerate.

Step 5. Expand in ZαZ\alpha (with n=nr+∣κ∣n=n_r+|\kappa|):

E≈mc2−mc2(Zα)22n2−mc2(Zα)42n4(nj+12−34)+⋯E\approx mc^2-\frac{mc^2(Z\alpha)^2}{2n^2}-\frac{mc^2(Z\alpha)^4}{2n^4}\Big(\frac{n}{j+\tfrac12}-\frac34\Big)+\cdots

— rest energy, Bohr levels, and the fine-structure correction, the last matching the perturbative sum of the mass-velocity, spin-orbit, and Darwin terms. Verified numerically: the ZαZ\alpha-expansion to order α4\alpha^4 equals 1−(Zα)22n2−(Zα)42n4(nj+1/2−34)1-\tfrac{(Z\alpha)^2}{2n^2}-\tfrac{(Z\alpha)^4}{2n^4}(\tfrac{n}{j+1/2}-\tfrac34) for several (n,j)(n,j); the leading binding is −13.606-13.606 eV; and 2s1/2=2p1/22s_{1/2}=2p_{1/2} exactly — all checked in the verifier.

Limiting cases

caseresultmeaning
rest energyE→mc2E\to mc^2the (Zα)0(Z\alpha)^0 term; absent in nonrelativistic treatments
Bohr spectrumE−mc2→−mc2(Zα)22n2E-mc^2\to -\tfrac{mc^2(Z\alpha)^2}{2n^2}order (Zα)2(Z\alpha)^2: the Schrödinger levels, depending on nn only
fine structureΔEfs=−mc2(Zα)42n4(nj+1/2−34)\Delta E_{\rm fs}=-\tfrac{mc^2(Z\alpha)^4}{2n^4}\big(\tfrac{n}{j+1/2}-\tfrac34\big)order (Zα)4(Z\alpha)^4: lifts ℓ\ell-degeneracy through jj; contains all three FW operators
c→∞c\to\infty (α→0\alpha\to0)pure Schrödinger Coulomb spectrumall relativistic corrections vanish
Zα→1Z\alpha\to1 (Z≈137Z\approx137)γ→0\gamma\to0, energy complexpoint-nucleus theory breaks down; supercriticality
2s1/22s_{1/2} vs 2p1/22p_{1/2}exactly degeneratesame n,jn,j; split only by QED (Lamb shift), beyond this article

Worked examples

Example 1 — the ground state and its relativistic shift (confidence builder). Compute the exact Dirac ground-state energy of hydrogen and the size of its relativistic correction to the Bohr value.

Step 1. Set up. The ground state is 1s1/21s_{1/2}: n=1n=1, j=12j=\tfrac12, so nr=0n_r=0 and γ=1−(Zα)2\gamma=\sqrt{1-(Z\alpha)^2}. With nr=0n_r=0, E1,1/2=mc2[1+(Zα/γ)2]−1/2E_{1,1/2}=mc^2[1+(Z\alpha/\gamma)^2]^{-1/2}, which simplifies to E1,1/2=mc21−(Zα)2=mc21−α2E_{1,1/2}=mc^2\sqrt{1-(Z\alpha)^2}=\boxed{mc^2\sqrt{1-\alpha^2}} for Z=1Z=1.

Step 2. Numeric value. With α=1/137.036\alpha=1/137.036, α2=5.325×10−5\alpha^2=5.325\times10^{-5}, so 1−α2=0.99997337\sqrt{1-\alpha^2}=0.99997337. Then E1,1/2=0.99997337 mc2E_{1,1/2}=0.99997337\,mc^2, and the binding energy is E1,1/2−mc2=(0.99997337−1)(5.110×105)E_{1,1/2}-mc^2=(0.99997337-1)(5.110\times10^5) eV =−13.606 eV=\boxed{-13.606\ \text{eV}} — the Bohr value, recovered exactly at leading order.

Step 3. The relativistic shift. Expand 1−α2≈1−12α2−18α4\sqrt{1-\alpha^2}\approx1-\tfrac12\alpha^2-\tfrac18\alpha^4; the binding is −Ry(1+14α2)-\text{Ry}(1+\tfrac14\alpha^2), so the α4\alpha^4 shift beyond Bohr is −14Ry α2=−14(13.606)(5.325×10−5)-\tfrac14\text{Ry}\,\alpha^2=-\tfrac14(13.606)(5.325\times10^{-5}) eV =−1.81×10−4 eV=\boxed{-1.81\times10^{-4}\ \text{eV}}. The exact ground state is bound more tightly than Bohr by this amount — the mass-velocity correction near the nucleus, computed here in one line rather than as a sum of three perturbative operators (verified).

Example 2 — the exact 2s₁⁄₂ = 2p₁⁄₂ degeneracy and the 2p splitting (exam level). Show that the exact Dirac energies of 2s1/22s_{1/2} and 2p1/22p_{1/2} are identical, and compute the 2p3/22p_{3/2}–2p1/22p_{1/2} splitting from the exact formula.

Step 1. Identify the states. 2s1/22s_{1/2}: n=2n=2, ℓ=0\ell=0, j=12j=\tfrac12 (so κ=−1\kappa=-1, nr=1n_r=1). 2p1/22p_{1/2}: n=2n=2, ℓ=1\ell=1, j=12j=\tfrac12 (so κ=+1\kappa=+1, nr=1n_r=1). Both have n=2n=2 and j=12j=\tfrac12; they differ only in the sign of κ\kappa.

Step 2. Evaluate the formula. Since EnjE_{nj} depends on γ=(j+12)2−(Zα)2\gamma=\sqrt{(j+\tfrac12)^2-(Z\alpha)^2} and nrn_r, and both states share j=12j=\tfrac12 (same γ\gamma) and nr=1n_r=1, they give identical energies: E(2s1/2)=E(2p1/2)=mc2[1+(Zα/(1+γ))2]−1/2E(2s_{1/2})=E(2p_{1/2})=mc^2[1+(Z\alpha/(1+\gamma))^2]^{-1/2} with γ=1−α2\gamma=\sqrt{1-\alpha^2}. The sign of κ\kappa never enters the energy, so the degeneracy is exact\boxed{\text{exact}} — verified as bit-identical energies.

Step 3. The 2p3/22p_{3/2} energy. For 2p3/22p_{3/2}: n=2n=2, j=32j=\tfrac32 (so ∣κ∣=2|\kappa|=2, nr=0n_r=0), γ=4−α2\gamma=\sqrt{4-\alpha^2}. Evaluating E2,3/2/mc2=0.999993344E_{2,3/2}/mc^2=0.999993344 versus E2,1/2/mc2=0.999993343E_{2,1/2}/mc^2=0.999993343 — a tiny gap.

Step 4. The splitting. Multiply the gap by mc2mc^2: ΔE(2p3/2−2p1/2)=(0.999993344−0.999993343)(5.110×105)\Delta E(2p_{3/2}-2p_{1/2})=(0.999993344-0.999993343)(5.110\times10^5) eV =4.53×10−5 eV=0.365 cm−1=\boxed{4.53\times10^{-5}\ \text{eV}}=0.365\ \text{cm}^{-1}. This is identical to the perturbative fine-structure result — the exact formula packages the mass-velocity, spin-orbit, and Darwin terms and reproduces their sum exactly (verified). The residual 2s1/22s_{1/2}–2p1/22p_{1/2} splitting — zero here — is the QED Lamb Shift, developed under that name and beyond this single-particle spectrum.

Historical development

Origins · 1 minfine-structure constant and how this was discovered
FC
fine-structure constant
α ≈ 1∕137, named 1916 · Munich, the number that runs the expansion

The exact hydrogen spectrum is really the story of one number. In 1916 Arnold Sommerfeld, refining the Bohr model with elliptical relativistic orbits, found that the level splittings were governed by a new dimensionless combination α=e2/(4πε0ℏc)≈1/137\alpha=e^2/(4\pi\varepsilon_0\hbar c)\approx1/137, which he named the fine-structure constant because it set the scale of the fine structure. His formula for the levels was, astonishingly, exactly right — even though his model had no spin and treated the electron as a point charge on a classical orbit. It took Dirac's 1928 equation to explain why: the same formula falls out of the relativistic wave equation, now with the correct spin content and the quantum-number labeling (nn and jj) that Sommerfeld's orbits could only mimic. That α\alpha controls the entire expansion — each successive term carrying two more powers of ZαZ\alpha — is why hydrogen is a laboratory for measuring α\alpha itself, and why the expansion's breakdown at Zα→1Z\alpha\to1 marks the edge of the single-particle theory. Sommerfeld got the right answer for the wrong reason; the Dirac equation made the number mean what it means.

History
1913
— Bohr's model gives the gross spectrum E_n = −13.6 eV∕n²
1916
— Sommerfeld derives the fine-structure formula from relativistic orbits and names α
1928
— Dirac's equation reproduces the Sommerfeld formula with correct spin and n, j labeling
1947
— Lamb and Retherford measure the 2s₁⁄₂–2p₁⁄₂ splitting, exposing the exact degeneracy's QED breaking
1969
— Pieper and Greiner analyze supercritical fields as the Zα → 1 continuation of the Dirac problem

Going further

References. Bjorken & Drell, Relativistic Quantum Mechanics, §4 · Sakurai, Advanced Quantum Mechanics, Ch. 3 · Greiner, Relativistic Quantum Mechanics: Wave Equations, Ch. 9 · Sakurai & Napolitano, Modern Quantum Mechanics, 2nd ed. · Bethe & Salpeter, Quantum Mechanics of One- and Two-Electron Atoms · Sommerfeld, Ann. Phys. 51, 1 (1916); Dirac, Proc. R. Soc. A 117, 610 (1928).

Provenance. The Sommerfeld formula and quantum-number labeling are verified against Bjorken–Drell §4, Sakurai Advanced QM Ch. 3, and Greiner Ch. 9. Owned and shown here: (i) the origin exponent γ=(j+12)2−(Zα)2\gamma=\sqrt{(j+\tfrac12)^2-(Z\alpha)^2} from the indicial equation, with the ground-state γ\gamma real iff Zα<1Z\alpha<1 (Zcrit=1/α=137.036Z_{\rm crit}=1/\alpha=137.036); (ii) the quantization nr=ZαE/(ℏcλ)−γn_r=Z\alpha E/(\hbar c\lambda)-\gamma and the exact spectrum Enj=mc2[1+(Zα/(nr+γ))2]−1/2E_{nj}=mc^2[1+(Z\alpha/(n_r+\gamma))^2]^{-1/2}; (iii) the ZαZ\alpha-expansion reproducing 1−(Zα)22n2−(Zα)42n4(nj+1/2−34)1-\tfrac{(Z\alpha)^2}{2n^2}-\tfrac{(Z\alpha)^4}{2n^4}(\tfrac{n}{j+1/2}-\tfrac34) for several (n,j)(n,j), i.e. rest energy + Bohr + fine structure; (iv) the ground-state binding −13.606-13.606 eV with relativistic shift −1.81×10−4-1.81\times10^{-4} eV; (v) the exact 2s1/2=2p1/22s_{1/2}=2p_{1/2} degeneracy and the 2p3/22p_{3/2}–2p1/22p_{1/2} splitting 4.53×10−54.53\times10^{-5} eV =0.365=0.365 cm−1^{-1}. This article is the reciprocal of the forward-pointer in Fine Structure of Hydrogen (whose jj-only master formula is the leading shadow of this exact spectrum); the perturbative operators it packages are owned by Relativistic Kinetic Energy Correction, Spin-Orbit Coupling, and Darwin Term by name; the residual 2s1/22s_{1/2}–2p1/22p_{1/2} splitting is the QED Lamb Shift, stated as OPEN and beyond this single-particle theory; the Bohr spectrum it recovers is owned by The Hydrogen Atom: Coulomb Radial Equation by name. All numbers CODATA-standard; verifier `verify_aq-qm-exact-dirac-hydrogen-atom.py`.

Builds on: The Dirac Equation · Dirac Gamma Matrices and Clifford Algebra · Spin from the Dirac Equation · Dirac Spinors and Plane-Wave Solutions · The Hydrogen Atom: Coulomb Radial Equation

Leads to: Fine Structure of Hydrogen · Lamb Shift · Supercritical Fields and Zα→1Z\alpha\to1 · Charge Conjugation and the Positron

How can the hydrogen atom be exactly solvable relativistically when almost nothing else is?

It comes down to the special symmetry of the 1/r1/r potential plus the separability of the Dirac equation in a central field. The angular part separates cleanly using spinor spherical harmonics (eigenfunctions of the Dirac KK operator), leaving two coupled first-order radial equations that reduce to a confluent hypergeometric (Kummer) equation — the same class that makes the nonrelativistic Coulomb and harmonic-oscillator problems solvable. Most potentials do not separate the Dirac equation or do not reduce to a solvable radial equation, so hydrogen is genuinely special. The deeper reason the energies come out so simple (depending on n,jn,j only) is the relativistic analogue of the Coulomb SO(4)SO(4) symmetry — an extra hidden conserved quantity that collapses what would otherwise be ℓ\ell-dependence.

Why does the exact energy depend on j and not ℓ, when spin-orbit coupling clearly depends on ℓ?

Individually, the mass-velocity correction and the spin-orbit coupling each depend on ℓ\ell — but their ℓ\ell-dependence cancels exactly when summed, to all orders, not just at O(α4)O(\alpha^4). In the exact solution this shows up structurally: the energy enters only through ∣κ∣=j+12|\kappa|=j+\tfrac12, and the sign of κ\kappa (which is what distinguishes the two ℓ\ell values at fixed jj) never appears in the spectrum. So 2s1/22s_{1/2} (κ=−1\kappa=-1) and 2p1/22p_{1/2} (κ=+1\kappa=+1) get bit-identical energies. The perturbative treatment only watches the ℓ\ell-dependence cancel; the exact solution shows it was never really there — it is a hidden symmetry, the relativistic cousin of the SO(4)SO(4) that makes nonrelativistic hydrogen depend on nn alone.

If the Dirac spectrum is exact, why doesn't it match experiment perfectly?

Because "exact" here means exact for a very specific idealized problem: a single electron in a point Coulomb potential, with no quantized electromagnetic field. Real hydrogen has more physics. The proton has finite size (a volume shift), finite mass (recoil and reduced-mass corrections), and spin (hyperfine structure). And the electromagnetic field is quantized, producing radiative QED corrections — most famously the Lamb shift that splits 2s1/22s_{1/2} from 2p1/22p_{1/2}, exactly degenerate in the Dirac spectrum. Each of these is a small, calculable departure from the Dirac baseline. The value of the exact spectrum is precisely that it is the sharp zero against which all these smaller effects are defined and measured — it is a foundation, not the whole building.

What is κ, and why is it more natural than ℓ in the Dirac problem?

κ\kappa is the integer eigenvalue (up to a sign and ℏ\hbar) of the Dirac operator K=β(Σ ⁣⋅ ⁣L+ℏ)K=\beta(\boldsymbol\Sigma\!\cdot\!\mathbf L+\hbar), and it packages both the total angular momentum jj and the parity/orbital character in one number: κ=−(j+12)\kappa=-(j+\tfrac12) for j=ℓ+12j=\ell+\tfrac12 and κ=+(j+12)\kappa=+(j+\tfrac12) for j=ℓ−12j=\ell-\tfrac12. It is more natural than ℓ\ell because in a relativistic problem ℓ\ell is not a good quantum number for the full four-spinor — the large and small components have different orbital angular momenta (ℓ\ell and ℓ±1\ell\pm1). What is conserved is jj and the parity, and κ\kappa encodes exactly that. Its magnitude ∣κ∣=j+12|\kappa|=j+\tfrac12 is what enters γ\gamma and the energy; its sign distinguishes the two ℓ\ell values that turn out degenerate.

Does the exact solution predict the breakdown at Z ≈ 137, and is that physical?

Yes, it predicts it, and yes, it is physical — though the exact critical charge depends on the nuclear model. For a point nucleus the ground-state exponent γ=1−(Zα)2\gamma=\sqrt{1-(Z\alpha)^2} vanishes at Zα=1Z\alpha=1, i.e. Z≈137Z\approx137, and beyond that the energy goes complex — the single-particle theory is telling you it has failed. For a realistic finite-size nucleus the breakdown is postponed to Z≈173Z\approx173, where the 1s1s bound level is predicted to "dive" into the negative-energy continuum and the vacuum becomes unstable to spontaneous positron emission — the physics of supercritical fields. So the Zα→1Z\alpha\to1 singularity is not an artifact but a genuine signal that at strong enough fields you must go beyond one-particle quantum mechanics to quantum field theory. It is the exact spectrum honestly marking the edge of its own validity.

Is the Sommerfeld formula really the same as Dirac's, given Sommerfeld had no spin?

The energy formula is the same; the reasoning is completely different, and that difference matters. Sommerfeld (1916) got the levels from relativistic elliptical orbits with an azimuthal quantum number, no spin — and by a remarkable coincidence, his azimuthal number plays the role that j+12j+\tfrac12 plays in the Dirac formula, so the numbers came out right. But his interpretation was wrong: he had no spin, no correct degeneracy structure, and no explanation for the selection rules. Dirac (1928) reproduced the identical formula from a proper relativistic wave equation, now with spin-12\tfrac12, the correct (n,j)(n,j) labeling, and the right multiplicities. It is a classic case of "right answer, wrong reason": the agreement was a lucky signpost that the deeper theory would vindicate, not evidence that the old-quantum picture was correct.

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