
Bounded modern-physics survey · Interactive lesson
Magnetic moments, Zeeman splitting and fine structure
Put an atom in a magnet and its lines split; the way they split reads out the angular momentum of every level involved, and tells you whether your field or the atom's own internal field is in charge. Here the current loop becomes Bohr magnetons, spin brings its factor of two, and hydrogen loses the textbook triplet.
UPIII-10.07 · Lesson 7 of 9 in this unit. Position is not a completion score.Bounded modern-physics survey. This modern-physics material is an introductory survey, not a complete course in relativity, quantum, atomic, nuclear or particle physics. Your university determines the required depth and assessment.
Build the model
Two magnetic fields compete: the one you apply and the one the orbit makes.
The key idea
An atom's magnetic moment is tied to its angular momentum, so an applied field B shifts each sublevel by an energy g m μB B, the Zeeman effect, while the electron's spin in the field of its own orbit splits levels of different j with no field applied, which is fine structure.
Example. In 1.00 T a ¹P₁ level splits into three sublevels 5.79 × 10⁻⁵ eV (14.0 GHz) apart, whereas hydrogen's 2p is already split at zero field into ²P₁/₂ and ²P₃/₂, 4.53 × 10⁻⁵ eV (10.9 GHz) apart.
The complete physical model and assumptions
An electron in an orbit is a current loop, and its magnetic moment is locked to its angular momentum by the ratio e/2mₑ, so a quantised Lz means a moment quantised in Bohr magnetons, and a field B shifts each sublevel by mₗ μB B. If spin played no part, every level would split in the same equal steps and every line would become the three-line pattern that a classical bound electron already predicts. Spin breaks this twice. Its moment per unit of angular momentum is twice the orbital one, so the total moment is not parallel to J. And even at B = 0 the spin sits in the magnetic field that the orbiting nucleus produces in the electron's own frame, an energy proportional to L⋅S that splits every l > 0 level by j: fine structure. The size of that internal coupling decides which description is right. While the applied field is weak against it, j and mⱼ are good quantum numbers, each level shifts by gJ mⱼ μB B with its own gJ, and lines break into four, six or more components; this anomalous pattern is what even hydrogen shows. When the applied field wins, L and S decouple, mₗ and mₛ return, and a triplet reappears for a different reason. The model stops at the nucleus and the vacuum: hyperfine structure and the Lamb shift are left out.
1An orbit is a current loop with a fixed ratio
Classically, an electron of charge −e circling at speed v on radius r is a current ev/(2πr) running opposite to its motion around an area πr². Its moment is μ = IA = evr/2, and since L = mₑ v r, μ = −(e/2mₑ)L: a gyromagnetic ratio that does not depend on r or v. Quantum mechanics keeps the ratio, because the probability current of ψₙₗₘ circulates with the same e/2mₑ, so quantising Lz = mₗ ħ quantises μz = −mₗ μB with μB = eħ/(2mₑ) = 9.274 × 10⁻²⁴ J T⁻¹. The magnitude is √(l(l+1)) μB, so a d electron carries 2.45 μB yet can only show 2, 1, 0, −1 or −2 μB along any chosen axis. In energy units μB is 5.788 × 10⁻⁵ eV T⁻¹: even at 10 T, μB B = 5.8 × 10⁻⁴ eV, under 1/17 000 of the 10.2 eV Lyman-α photon. That is why every magnetic shift in this lesson is a small perturbation on the Coulomb levels.
2Spinless levels give the classical three-line pattern
Put B along z. The energy of a moment is U = −μ⋅B = −μz B, so an orbital state moves by mₗ μB B: 2l + 1 sublevels in equal steps of μB B, the same step in every level. If both levels of a transition have total spin S = 0 the moment is purely orbital, and the photon's one unit of angular momentum allows Δm = 0, ±1. However many sublevel pairs there are, only three photon energies occur, E₀ and E₀ ± μB B. At 1.00 T the side lines sit μB B/h = 14.0 GHz from the centre; for cadmium's 643.8 nm ¹D₂ → ¹P₁ line that is 0.019 nm. Planck's constant cancels, since μB B/h = eB/(4πmₑ), which is exactly the Larmor shift Lorentz derived for a classical electron bound by a spring. That correspondence is why the triplet is called normal. Its polarisation is classical too: the Δm = 0 line is linearly polarised along B, and the Δm = ±1 lines are circularly polarised when viewed along B, where the central line vanishes.
3The orbit's own field acts on the spin
Spin adds a moment μₛ, z = −gₛ mₛ μB with gₛ ≈ 2: twice as much moment per unit of angular momentum as the orbit. It also has something to couple to with no applied field. In the electron's rest frame the nucleus circles it, and that moving charge makes a field Bᵢₙₜ = (1/(e mₑ c² r))(dU/dr) L, parallel to L. The spin's energy −μₛ⋅Bᵢₙₜ, halved by Thomas precession because that frame accelerates, is HSO = (1/(2mₑ²c²))(1/r)(dU/dr) L⋅S. It depends on the angle between L and S, so neither Lz nor Sz is conserved any more; only J = L + S and its projection mⱼ are. Writing L⋅S = ½(J² − L² − S²) turns it into ESO = (A/2)[j(j+1) − l(l+1) − s(s+1)]. A p electron has j = 3/2 at +A/2 and j = ½ at −A, a doublet 3A/2 apart. Sodium's D lines at 588.995 nm and 589.592 nm put that gap at 2.13 × 10⁻³ eV, and equating it to 2μB Bᵢₙₜ gives an internal field of about 18 T.
4Term symbols and hydrogen's fine structure
A level is labelled (2S+1)LJ: the multiplicity 2S + 1, the letter S, P, D, F for L = 0, 1, 2, 3, and J as a subscript. One electron outside closed shells has S = ½, so its terms are doublets: 2p gives ²P₁/₂ and ²P₃/₂. In hydrogen, spin–orbit coupling arrives with two relativistic corrections of the same size, the (v/c)² correction to kinetic energy and the Darwin term, and together they give Dirac's Eₙⱼ = −(13.6 eV/n²)[1 + (α²/n²)(n/(j + ½) − ¾)]. The spin–orbit part alone, using hydrogen's ⟨1/r³⟩, gives A = α⁴mec²/[2n³l(l + ½)(l + 1)] = 3.02 × 10⁻⁵ eV for 2p, so the 2p doublet is 3A/2 = 4.53 × 10⁻⁵ eV (10.9 GHz) wide, matching the formula. Two checks: the correction is of order α² = 5.3 × 10⁻⁵ of the gross structure, as a (v/c)² effect should be when v/c = α in the ground state; and α → 0 returns Bohr's −13.6 eV/n². Because only n and j appear, 2s₁/₂ and 2p₁/₂ are predicted degenerate; the 4.4 × 10⁻⁶ eV Lamb shift that parts them is quantum electrodynamics, outside this model.
5Weak field: each level gets its own gJ
While μB B is small against the fine-structure gap, the internal coupling wins: L and S precess rapidly about J, and J precesses slowly about B. The total moment μ = −(μB/ħ)(L + 2S) = −(μB/ħ)(J + S) is not parallel to J, because the spin counts double, and only its component along J survives the fast precession. Projecting with S⋅J = ½(J² + S² − L²) gives ΔE = gJ mⱼ μB B with gJ = 1 + [j(j+1) + s(s+1) − l(l+1)]/[2j(j+1)]. For S = 0 this is 1 in every level, and the normal triplet follows. For one electron it is 2 in ²S₁/₂, 2/3 in ²P₁/₂ and 4/3 in ²P₃/₂. Upper and lower levels now split at different rates, so the photon shifts (g′m′ − g″m″)μB B, primes marking the upper and lower level, no longer collapse: ²P₁/₂ → ²S₁/₂ gives four lines at ±2/3 and ±4/3 of μB B, and ²P₃/₂ → ²S₁/₂ gives six at ±1/3, ±1 and ±5/3. Every hydrogen level has S = ½, so hydrogen has no normal Zeeman effect at all: its weak-field splitting is anomalous.
6Strong field: Paschen–Back, where LS coupling ends
The coupled picture lasts only while the applied field is weak against the internal one. Once μB B exceeds the fine-structure gap, B turns L and S about itself faster than they can turn about each other; J stops being conserved and mₗ and mₛ become the good quantum numbers again. Then ΔE = (mₗ + 2mₛ)μB B + A mₗ mₛ, with spin–orbit coupling reduced to a first-order correction. Electric-dipole photons do not act on spin, so Δmₛ = 0 and Δmₗ = 0, ±1: a p → s line returns to a triplet spaced μB B, each outer line split into a doublet A apart. The crossover sits near μB B ≈ ΔEfs: 0.78 T for hydrogen's 2p, inside any laboratory magnet, but 37 T for sodium's 3p, so sodium stays anomalous in every ordinary field and hydrogen does not. In between, only mⱼ stays good: neither j nor the pair mₗ, mₛ does, so each pair of states sharing mⱼ must be diagonalised exactly, as the figure does. Nuclear moments are smaller by mₑ/mₚ ≈ 1/1836, so hyperfine structure is a further, finer splitting left out here along with the Lamb shift.
Key equations
Read the units, assumptions and limits before substituting.
Orbital moment in Bohr magnetons
μz = −(e/2mₑ) Lz = −mₗ μB
The ratio e/2mₑ is a classical current loop's and survives quantum mechanics, so quantised Lz gives μz in whole steps of μB; the minus sign is the electron's charge.
μz in J T⁻¹; μB = eħ/(2mₑ) = 9.274 × 10⁻²⁴ J T⁻¹ = 5.788 × 10⁻⁵ eV T⁻¹; mₗ an integer, |mₗ| ≤ lEnergy of a moment in a field
U = −μ⋅B = −μz B
With S = 0 every level splits in equal steps μB B, so Δm = 0, ±1 photons give only three lines spaced μB B/h, 14.0 GHz for every tesla: Lorentz's classical Larmor shift.
U in J, μ in J T⁻¹, B in T taken along z; an orbital moment gives U = mₗ μB BSpin–orbit energy
ESO = (A/2)[j(j+1) − l(l+1) − s(s+1)]
Levels j and j − 1 sit A j apart, the interval rule. A p electron splits into j = 3/2 at +A/2 and j = ½ at −A, and the (2j + 1)-weighted centre stays put: 4(A/2) + 2(−A) = 0.
A the level's spin–orbit constant in eV; uses L⋅S = ½(J² − L² − S²); one electron has s = ½ and j = l ± ½Hydrogen fine structure (Dirac)
Eₙⱼ = −(13.6 eV/n²)[1 + (α²/n²)(n/(j + ½) − ¾)]
2p₃/₂ lies 4.53 × 10⁻⁵ eV (10.9 GHz) above 2p₁/₂, a fraction of order α² of the gross structure; 2s₁/₂ and 2p₁/₂ coincide, and α → 0 returns Bohr's levels.
α = 1/137.04, dimensionless; depends on n and j only; spin–orbit, relativistic and Darwin terms together, Lamb shift omittedWeak-field (anomalous) Zeeman shift
ΔE = gJ mⱼ μB B
gJ is 2 for ²S₁/₂, 2/3 for ²P₁/₂ and 4/3 for ²P₃/₂. Unequal g in the two levels breaks one line into 4 or 6; only S = 0 forces gJ = 1, the normal case.
gJ = 1 + [j(j+1) + s(s+1) − l(l+1)]/[2j(j+1)] with gₛ = 2; −j ≤ mⱼ ≤ j; needs μB B ≪ the fine-structure gapStrong-field (Paschen–Back) shift
ΔE = (mₗ + 2mₛ) μB B + A mₗ mₛ
Photons leave mₛ alone, so a p → s line returns to a triplet spaced μB B, its outer lines split by A. Hydrogen's 2p crosses over near 0.78 T; sodium's 3p only near 37 T.
mₗ and mₛ are good quantum numbers again; A as in the spin–orbit card; needs μB B ≫ the fine-structure gapInteractive lab
Predict first. Explore the model. Compare the result.
Explore the model
Try this. At Δ = 45 μeV, hydrogen's 2p, drag B from 0 to 2 T: the ²P₃/₂, mⱼ = +½ slope climbs from 0.67 (gJ mⱼ) towards 1 (mₗ + 2mₛ). Raise Δ to 100 μeV and the same field bends the lines less: a stronger internal field keeps LS coupling alive longer.
Live results
- FIELD RATIO μB B/Δ
- 0.39
- ZEEMAN ENERGY μB B
- 17.4 μeV
- SLOPE, ²P₃/₂ mⱼ = +½
- 0.80 μB
- SLOPE, ²P₁/₂ mⱼ = +½
- 0.20 μB
Results follow this lesson’s model and assumptions. Displayed values are rounded.
Predict → change one variable → check
Plan a change before running it. Every other input stays at the saved baseline.
Saved baseline. Applied field B: 0.30 T; Fine-structure splitting Δ: 45 μeV
This experiment is kept only while this page is open. It does not change saved course progress.
Catch the common trap
The usual first-year picture is that a field splits every level into 2l + 1 sublevels exactly μB B apart, so every line becomes three equally spaced lines. That holds only when both levels have total spin S = 0. The spacing inside a level is gJ μB B, and gJ depends on l, s and j, because spin carries twice the moment per unit of angular momentum and pulls the total moment off the direction of J. Different levels then split at different rates and the photon shifts no longer collapse onto three values: sodium's D₁ line gives four components and D₂ gives six. Hydrogen, with S = ½ in every level, never shows the normal triplet in a weak field. Normal is the historical name for what a classical bound electron predicts, not the typical case, and three lines seen in a strong field are the Paschen–Back effect, not evidence that S = 0.
Practice & worked examples
3 authored examples. Make an attempt, then reveal the reasoning one step at a time.
EasyExample 1
The calcium resonance line at 422.67 nm is a ¹P₁ → ¹S₀ transition. In a 1.40 T field, how many Zeeman components appear, how far apart are they in frequency and in wavelength, and what resolving power λ/Δλ separates them?
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 5 steps revealed.
- Both levels have S = 0, so the moment is purely orbital and g = 1: a sublevel shifts by m μB B. The ¹S₀ level has J = 0, one sublevel that does not move; ¹P₁ splits into m = −1, 0, +1.
- Spacing: μB B = 5.788 × 10⁻⁵ eV T⁻¹ × 1.40 T = 8.10 × 10⁻⁵ eV, so Δf = μB B/h = 14.00 GHz T⁻¹ × 1.40 T = 19.6 GHz.
- Δm = 0, ±1 lets all three upper sublevels decay to the single lower one, giving lines at f₀ and f₀ ± 19.6 GHz.
- In wavelength, Δλ = λ²Δf/c = (422.67 × 10⁻⁹ m)² × 1.959 × 10¹⁰ Hz ÷ 2.998 × 10⁸ m s⁻¹ = 1.17 × 10⁻¹¹ m = 11.7 pm.
- Resolving power: λ/Δλ = 422.67 nm ÷ 0.0117 nm = 3.6 × 10⁴, within reach of a good grating or a Fabry–Pérot etalon.
Answer. Three components, 19.6 GHz (11.7 pm) apart; a resolving power of about 3.6 × 10⁴ separates them.
MediumExample 2
Hydrogen's n = 3 level lies at −1.512 eV in the Bohr model. List its fine-structure terms, use the Dirac formula to find how far each value of j sits below −1.512 eV, and give the gaps between them in GHz. Which terms remain degenerate in this model?
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 5 steps revealed.
- l = 0, 1, 2 with s = ½: 3s gives ²S₁/₂, 3p gives ²P₁/₂ and ²P₃/₂, and 3d gives ²D₃/₂ and ²D₅/₂. Five terms share three values of j: ½, 3/2 and 5/2.
- The shift from Bohr is δE = −(13.6 eV/n⁴) α² [n/(j + ½) − ¾]. For n = 3 the prefactor is (13.606 eV/81) × 5.325 × 10⁻⁵ = 8.945 × 10⁻⁶ eV.
- Brackets: j = ½ gives 3 − 0.75 = 2.25; j = 3/2 gives 1.5 − 0.75 = 0.75; j = 5/2 gives 1 − 0.75 = 0.25. So δE = −20.1 μeV, −6.71 μeV and −2.24 μeV.
- Gaps: 13.42 μeV between j = ½ and 3/2, and 4.47 μeV between 3/2 and 5/2. Dividing by h = 4.136 × 10⁻¹⁵ eV s gives 3.24 GHz and 1.08 GHz.
- Degenerate pairs: 3s₁/₂ with 3p₁/₂, and 3p₃/₂ with 3d₃/₂; the Lamb shift parts them, outside this model. Check: the largest shift is 1.3 × 10⁻⁵ of 1.512 eV, the α² scale, and every shift vanishes as α → 0.
Answer. j = ½, 3/2 and 5/2 sit 20.1, 6.71 and 2.24 μeV below −1.512 eV, with gaps of 3.24 GHz and 1.08 GHz; 3s₁/₂ with 3p₁/₂ and 3p₃/₂ with 3d₃/₂ stay degenerate.
HardExample 3
Hydrogen's 2p level has fine-structure splitting Δ = 45.3 μeV, so A = 2Δ/3 = 30.2 μeV. In a 1.00 T field, find the exact energies of the two mⱼ = +½ states, measured from the zero-field centre of 2p, and decide whether the weak-field gJ formula or the Paschen–Back formula is the better approximation.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 6 steps revealed.
- μB B = 57.88 μeV, so μB B/Δ = 1.28: neither limit is safe. Work in the mⱼ = +½ pair |mₗ = 0, mₛ = +½⟩ and |mₗ = 1, mₛ = −½⟩, which only the spin–orbit term connects.
- Diagonal terms (mₗ + 2mₛ)μB B + A mₗ mₛ: 57.88 + 0 = 57.88 μeV, and 0 − A/2 = −15.10 μeV. Off-diagonal: (A/2)√2 = 21.35 μeV, from the L₊S₋ part of L⋅S.
- Eigenvalues: centre (57.88 − 15.10)/2 = 21.39 μeV, half-gap (57.88 + 15.10)/2 = 36.49 μeV, so E = 21.39 ± √(36.49² + 21.35²) = 21.39 ± 42.28, giving +63.67 μeV and −20.89 μeV.
- Weak field, Eⱼ + gJ mⱼ μB B: Δ/3 + (4/3)(½)(57.88) = 15.10 + 38.59 = +53.69 μeV, and −2Δ/3 + (2/3)(½)(57.88) = −30.20 + 19.29 = −10.91 μeV. Each is 9.98 μeV off.
- Strong field, (mₗ + 2mₛ)μB B + A mₗ mₛ: +57.88 μeV and −15.10 μeV. Each is 5.79 μeV off, equal and opposite because the trace of the 2 × 2 block is fixed.
- Limits: B → 0 returns Δ/3 and −2Δ/3, the j = 3/2 and j = ½ levels; as B → ∞ the slopes tend to 1 and 0, the values of mₗ + 2mₛ for the two states.
Answer. +63.7 μeV and −20.9 μeV. Paschen–Back is closer (5.8 μeV off, against 10.0 μeV for gJ), but at 1.00 T hydrogen's 2p needs the exact 2 × 2 treatment.
Quick check
Select an answer and explain it before checking.
Review & continue
An atom's magnetic moment is tied to its angular momentum, so an applied field B shifts each sublevel by an energy g m μB B, the Zeeman effect, while the electron's spin in the field of its own orbit splits levels of different j with no field applied, which is fine structure.
- Explain the relationship without looking at the equation.
- Check a sign, a unit and a model assumption in your working.
- Return to the lab or worked example if a step is still unclear.