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Physics IV course sequence · Interactive lesson

Identical particles and exchange symmetry

Electrons carry no serial numbers. Follow that one fact through and you get the Pauli principle for free, an apparent force that appears nowhere in the Hamiltonian, and the 0.80 eV that puts triplet helium below singlet helium.

UPIV-11.01 · Lesson 1 of 9 in this unit. Position is not a completion score.
Starting model: Identical particles and exchange symmetryPair density |Ψ(x₁,x₂)|²L² against x₂, for two electrons in the ψ₁ and ψ₂ orbitals of a box of width L, with electron 1 pinned at x₁ = 0.30L. Dashed is the direct part alone; solid adds the exchange cross-term for cosθ ψ₁(1)ψ₂(2) + sinθ ψ₂(1)ψ₁(2) at θ = 45°. At x₂ = x₁ the solid is 2.00 times the dashed.electron 1 pinned at x₁ = 0.30Lθ = 45°solid |cosθ ψ₁(1)ψ₂(2) + sinθ ψ₂(1)ψ₁(2)|²dashed direct part only|Ψ|² L²420Lx₁position of electron 2
Start with a picture. Change the model in the lab below.
1

Build the model

Swap two electrons and the state must change sign. Everything else follows.

The key idea

Exchange symmetry is the requirement that the state of two identical particles either keeps its sign or reverses it when the two particle labels are swapped — symmetric for bosons, antisymmetric for fermions — because the labels themselves are not observable.

Example. Helium 1s2s: the spin triplet must carry the antisymmetric spatial factor and sits 19.820 eV above the ground state, while the singlet carries the symmetric one and sits 20.616 eV up — a 0.796 eV gap that the ordinary Coulomb repulsion produces only because the two spatial symmetries differ.

The complete physical model and assumptions

Two electrons are not two objects wearing faint name tags. Write ψₐ(r₁)ψb(r₂) and you have already said more than you can measure — that the electron you called 1 is the one in orbital a. Since only |Ψ|² is observable and relabelling cannot change it, Ψ(2,1) = e(iφ)Ψ(1,2); swapping twice must return the original state, so e(2iφ) = 1 and in three dimensions the only options are Ψ → +Ψ and Ψ → −Ψ. Which one a species takes is fixed by its spin — integer symmetric, half-integer antisymmetric — a result imported here from relativistic quantum field theory rather than derived. For electrons the whole state, space times spin, must change sign, and that single constraint does most of atomic physics. The antisymmetric combination vanishes identically when both orbitals are the same, which is the Pauli principle arriving as a corollary rather than a postulate. And because a symmetric spatial factor draws the electrons together while an antisymmetric one holds them apart, the ordinary Coulomb repulsion returns two different energies for the two spin arrangements: in helium's 1s2s configuration, 0.796 eV apart with the spin triplet lower. What it costs you is correlation. A symmetrised product of orbitals is still an independent-particle guess, and the electrons' real, instant-by-instant avoidance of each other is nowhere inside it.

1The label is yours, not nature's

A two-particle wavefunction Ψ(r₁, r₂) carries labels 1 and 2 that no apparatus can read. Define the exchange operator by P₁₂Ψ(1,2) = Ψ(2,1). For identical particles the Hamiltonian is symmetric in those labels — same mass, same charge, same interaction — so [H, P₁₂] = 0 and the exchange symmetry is a constant of the motion: decided once, kept for all time. Because swapping twice restores the original arrangement, P₁₂² = 1, so the eigenvalues are +1 and −1 and nothing else. That is why 'somewhere in between' is not on offer. A state that was neither symmetric nor antisymmetric would make |Ψ|² change when you relabelled, which is the same as saying the labels are measurable. Particles taking +1 are bosons and those taking −1 are fermions; that the choice follows the spin — integer or half-integer — is the spin-statistics theorem, proved inside relativistic quantum field theory and imported here without proof.

2Two combinations, and one of them can vanish

Take two orthonormal one-particle orbitals ψₐ and ψb. The plain product ψₐ(r₁)ψb(r₂) is not an eigenstate of P₁₂, but the two combinations ψ±(r₁, r₂) = [ψₐ(r₁)ψb(r₂) ± ψb(r₁)ψₐ(r₂)]/√2 are, with eigenvalues ±1. Now set b = a. The symmetric state survives as ψₐ(r₁)ψₐ(r₂), while the antisymmetric one collapses to ψₐ(r₁)ψₐ(r₂) − ψₐ(r₁)ψₐ(r₂) = 0 at every point. There is no state at all — not a forbidden one, an absent one. That is the Pauli exclusion principle, and notice where it came from: not from a rule about how many electrons a level holds, but from antisymmetry, which came from indistinguishability. Written for N particles the same object is a Slater determinant, and a determinant with two equal rows vanishes for exactly this reason. Bosons, taking the plus sign, carry no such restriction, and pile into a single mode happily.

3Space and spin trade signs

The antisymmetry demanded of electrons applies to the whole state, spin included. Two spin-half particles combine into one antisymmetric singlet, χ = (↑↓ − ↓↑)/√2 with S = 0, and three symmetric triplet states, ↑↑, (↑↓ + ↓↑)/√2 and ↓↓, with S = 1. If the state factorises as Ψ = ψ(space)⋅χ(spin), the two factors must carry opposite exchange signs, because their product has to be antisymmetric. So a spin singlet is locked to the symmetric spatial function and a spin triplet to the antisymmetric one — para and ortho helium in the older spectroscopic language, two families whose separate line series once looked like two different gases. Nothing here says that spin interacts with anything. Spin is the bookkeeping partner: fixing S fixes the spatial symmetry, and it is the spatial symmetry that the Coulomb energy actually sees.

4The exchange force is a consequence of counting

Work out the mean-square separation of the two symmetrised states in one dimension and the algebra returns ⟨(x₁−x₂)²⟩± = ⟨x²⟩ₐ + ⟨x²⟩b − 2⟨x⟩ₐ⟨x⟩b ∓ 2|⟨x⟩ab|², where ⟨x⟩ab = ∫ψₐ*(x) x ψb(x) dx. The first three terms are what two distinguishable particles would give. The last term is new, and its sign is set by the exchange symmetry: symmetric states sit closer together, antisymmetric states further apart. Two consequences follow. First, no force has been introduced — the Hamiltonian is untouched, and what changed is which configurations the wavefunction permits. Second, the effect requires overlap, because ⟨x⟩ab integrates over the region where both orbitals are appreciable. Two electrons in orbitals that never overlap — one here, one on the Moon — feel nothing from each other's statistics, and symmetrising them is a formality with no measurable consequence.

5Helium: one repulsion, two answers

Take helium's 1s2s configuration and treat the electron-electron repulsion V = e²/4πε₀r₁₂ as a first-order perturbation on ψ±. The expectation value splits into two integrals. The direct integral J = ⟨ab|V|ab⟩ is the electrostatic repulsion of the two charge clouds and is identical for both states. The exchange integral K = ⟨ab|V|ba⟩ multiplies the cross term and so enters with the exchange sign, giving E± = Eₐ + Eb + J ± K. For the Coulomb repulsion K is positive — a property of the 1/r₁₂ kernel itself, not merely of V being positive — so the triplet, carrying the minus sign, lies 2K below the singlet. Experiment agrees: the 2³S level sits 19.820 eV above helium's ground state and the 2¹S sits 20.616 eV, so 2K = 0.796 eV and K = 0.398 eV. Evaluating K with unscreened hydrogenic Z = 2 orbitals gives (16/729)Z hartree = 1.19 eV — right sign, right order, three times too big, because the real 2s electron is screened toward Zeff ≈ 1, so its orbital is about twice as wide and overlaps the 1s far less.

6What the symmetrised product still leaves out

Two debts stay outstanding. The first is spin-statistics itself: nothing in non-relativistic quantum mechanics forces half-integer spin to take the minus sign. It follows from demanding a relativistic field theory with an energy bounded below whose observables commute at spacelike separation. In two spatial dimensions, where exchanging twice need not restore the state, the choice is no longer limited to two signs, which is how anyons become possible. The second is correlation. Even after symmetrising, ψ± is assembled from single-particle orbitals, so each electron moves in an average field. Real electrons dodge one another instant by instant, digging a Coulomb hole around each that no single determinant can reproduce. The exchange hole is real but partial — it separates parallel-spin electrons and does nothing for antiparallel ones. Helium's exact non-relativistic ground state is −79.01 eV against −77.87 eV at the Hartree-Fock limit, and that 1.14 eV shortfall is precisely what the term 'correlation energy' names.

2

Key equations

Read the units, assumptions and limits before substituting.

Exchange operator and its two eigenvalues

P₁₂Ψ(1,2) = Ψ(2,1)P₁₂² = 1 ⇒ P₁₂Ψ = ±Ψ

+1 for bosons, −1 for fermions. In three dimensions there is no third option to take.

[H, P₁₂] = 0 for identical particles, so the sign is a constant of the motion

Symmetrised two-particle spatial state

ψ±(r₁, r₂) = [ψₐ(r₁)ψb(r₂) ± ψb(r₁)ψₐ(r₂)] / √2

ψ₋ vanishes identically when a = b — exclusion drops out of this line, it is not assumed.

ψₐ and ψb orthonormal and distinct; the 1/√2 is the wrong constant if a = b

Space and spin trade signs

Ψ = ψ₊⋅χsinglet (para, S = 0) or ψ₋⋅χₜᵣᵢₚₗₑₜ (ortho, S = 1)

Only the product must be antisymmetric, so choosing S chooses the spatial symmetry.

χsinglet = (↑↓ − ↓↑)/√2; χₜᵣᵢₚₗₑₜ = ↑↑, (↑↓ + ↓↑)/√2, ↓↓

Direct and exchange integrals

J = ⟨ab|V|ab⟩, K = ⟨ab|V|ba⟩, with V = e²/4πε₀r₁₂

J is the classical repulsion of two charge clouds; K has no classical counterpart at all.

J and K in joules or eV; r₁₂ = |r₁ − r₂| in metres; K > 0 for a Coulomb kernel

First-order energy of the two terms

E± = Eₐ + Eb + J ± K, so E(singlet) − E(triplet) = 2K

Helium 1s2s measures 2K = 0.796 eV, so K = 0.398 eV and the triplet is the lower term.

+ for the symmetric space state (singlet), − for the antisymmetric one (triplet)

Mean-square separation of the pair

⟨(x₁−x₂)²⟩± = ⟨x²⟩ₐ + ⟨x²⟩b − 2⟨x⟩ₐ⟨x⟩b ∓ 2|⟨x⟩ab|²

Symmetric pairs sit closer, antisymmetric pairs further apart — no force, only counting.

⟨x⟩ab = ∫ψₐ*(x) x ψb(x) dx, in metres; the last term dies without orbital overlap
3

Interactive lab

Predict first. Explore the model. Compare the result.

Explore the model

0.30 L
0.05 to 0.95 L; steps of 0.05.
45 °
0 to 180 °; steps of 5.

Try this. Set θ = 45°, the symmetric spatial factor that pairs with the spin singlet, and the solid curve doubles the dashed one exactly at x₂ = x₁. Set θ = 135°, the antisymmetric factor the triplet needs, and it drops to zero there — the exchange hole. No θ in between is an eigenstate of the swap.

Live results

PAIR DENSITY AT x₂ = x₁
4.74
DIRECT PART THERE
2.37
RATIO AT x₂ = x₁
2.00
OVERLAP ψ₁(x₁)ψ₂(x₁)L
1.54

Results follow this lesson’s model and assumptions. Displayed values are rounded.

Interactive Physics IV modelPair density |Ψ(x₁,x₂)|²L² against x₂, for two electrons in the ψ₁ and ψ₂ orbitals of a box of width L, with electron 1 pinned at x₁ = 0.30L. Dashed is the direct part alone; solid adds the exchange cross-term for cosθ ψ₁(1)ψ₂(2) + sinθ ψ₂(1)ψ₁(2) at θ = 45°. At x₂ = x₁ the solid is 2.00 times the dashed.electron 1 pinned at x₁ = 0.30Lθ = 45°solid |cosθ ψ₁(1)ψ₂(2) + sinθ ψ₂(1)ψ₁(2)|²dashed direct part only|Ψ|² L²420Lx₁position of electron 2
Pair density |Ψ(x₁, x₂)|²L² against x₂, for two electrons in the ψ₁ and ψ₂ orbitals of a box of width L, with electron 1 pinned at x₁ = 0.30L. Dashed is the direct part alone; solid adds the exchange cross-term for cosθ ψ₁(1)ψ₂(2) + sinθ ψ₂(1)ψ₁(2) at θ = 45°. At x₂ = x₁ the solid is 2.00 times the dashed.

Predict → change one variable → check

Plan a change before running it. Every other input stays at the saved baseline.

Saved baseline. Electron 1 position x₁/L: 0.30 L; Exchange mixing angle θ: 45 °

Baseline 0.30; choose 0.05 to 0.95, in steps of 0.05.
4. Compared with the saved baseline, this result will…

This experiment is kept only while this page is open. It does not change saved course progress.

4

Catch the common trap

The 0.796 eV between helium's singlet and triplet is not magnetic. The temptation is to say that parallel spins are parallel magnets and magnets know about each other — but the dipole-dipole energy of two electron moments 0.1 nm apart is μ₀μB²/4πr³ ≈ 5 × 10⁻⁵ eV, four orders of magnitude too small, and the Hamiltonian that produced the splitting contains no spin operator at all. Spin enters only as a label: fixing S fixes the exchange symmetry of the spin factor, that forces the opposite symmetry on the spatial factor, that changes how close the two electrons sit, and that changes the ordinary electrostatic repulsion. The energy is Coulomb from start to finish. "Exchange force" names a consequence of symmetry, not a fifth interaction — and it switches off entirely once the orbitals stop overlapping, because K is an overlap integral.

5

Practice & worked examples

3 authored examples. Make an attempt, then reveal the reasoning one step at a time.

EasyExample 1

Two electrons occupy the n = 1 and n = 2 levels of a one-dimensional infinite square well of width L = 1.0 nm, in a spin-triplet state. Write down the spatial wavefunction with the correct exchange symmetry, show what happens if both electrons are put in n = 1 instead, and give the total energy of the pair, ignoring their mutual repulsion.

Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.

0 of 4 steps revealed.

MediumExample 2

Helium's 2³S₁ level lies 19.820 eV above the ground state and its 2¹S₀ level lies 20.616 eV above it; both belong to the 1s2s configuration. Find the exchange integral K for this configuration, then compare it with the unscreened hydrogenic prediction K(1s,2s) = (16/729)Z hartree, taking 1 hartree = 27.2114 eV.

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.

HardExample 3

Two electrons sit in the n = 1 and n = 2 levels of an infinite well of width L = 1.0 nm. Using ⟨x⟩ₙ = L/2, ⟨x²⟩ₙ = L²[1/3 − 1/(2n²π²)] and ⟨x⟩₁₂ = −16L/9π², find the root-mean-square separation for the unsymmetrised product, for the symmetric spatial state and for the antisymmetric one, and say which spin state each belongs to.

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.

6

Quick check

Select an answer and explain it before checking.

In helium's 1s2s configuration the spin triplet lies 0.80 eV below the singlet. What sets that gap?
7

Review & continue

Exchange symmetry is the requirement that the state of two identical particles either keeps its sign or reverses it when the two particle labels are swapped — symmetric for bosons, antisymmetric for fermions — because the labels themselves are not observable.

  • 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.

Extra challenging questions

Connect several ideas, explore supplied data, and compare your reasoning with a worked solution.