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Advanced Quantum Mechanics course sequence · Interactive lesson

What orbital energies mean: Koopmans and Brillouin

Every Hartree-Fock run prints a column of orbital energies. Here we earn the right to read them: as the cost of pulling one electron out of a frozen atom, never as shares of the total energy, and only for canonical orbitals. Then we see why the converged determinant ignores single excitations, and how far measured spectra bear −εᵢ out.

UAQM-10.07 · Lesson 7 of 9 in this unit. Position is not a completion score.
Starting model: What orbital energies mean: Koopmans and BrillouinEnergy against the angle θ through which one occupied orbital turns into a virtual, both with gap Δ = 44 eV. Left, the N-electron determinant: slope 2b = 0.0 eV at θ = 0, zero for converged Hartree-Fock orbitals. Right, Koopmans' frozen ion: the hole's pull v = 8.4 eV tilts it, and relaxing lowers it by 1.55 eV, relaxation's share of −εₖ's overshoot.N electrons: E(θ) − E₀N − 1: E(θ) − (E₀ − εₖ)slope at 0: 2b = 0.0 eVion relaxes by 1.55 eVrelaxed ionθ = −45°+45°θ = −45°+45°
Start with a picture. Change the model in the lab below.
1

Build the model

An orbital energy prices one removal; their sum counts every repulsion twice.

The key idea

Koopmans' theorem: with every other orbital frozen, removing an electron from canonical Hartree-Fock orbital k costs −εₖ. Brillouin's theorem: H has no matrix element between the converged determinant and any singly excited one.

Example. Closed-shell helium has ε₁ₛ = −0.91796 Eₕ = −24.98 eV, so Koopmans predicts an ionisation energy of 24.98 eV against the measured 24.587 eV, while its total energy is −77.87 eV, not 2ε = −49.96 eV.

The complete physical model and assumptions

Hartree-Fock returns two kinds of number, a total energy and a list of orbital energies, and this topic says what the second kind is worth. Freeze every orbital, annihilate the electron in occupied orbital k, and the contractions of topic 10.05 show the energy rising by exactly −εₖ: an orbital energy is the price of removing one electron while the others stand still. That is Koopmans' theorem, and adding an electron to a virtual orbital a is priced by εₐ in the same way. The reading explains at once why the εᵢ do not add up to the total energy, since each contains the repulsion with every other electron, and why only canonical orbitals carry the meaning: they are the ones whose removal energy is stationary. Brillouin's theorem is the same stationarity read off as a matrix element. H links the converged determinant to no single excitation, so the first correction to Hartree-Fock is built from doubles. The model stops where freezing stops being harmless. The ion's orbitals relax towards the hole and lower its energy, while correlation, absent from one determinant, lowers the neutral atom more than the ion. The two errors have opposite signs and largely cancel for valence electrons, leaving helium 0.39 eV off; a core hole relaxes by some 20 eV, and for electron affinities the two errors add.

1Remove an electron and freeze the rest

Work in SI units with energies in eV, using the hartree Eₕ = 27.211 eV for atomic values; nothing here is relativistic, so the course metric diag(1, −1, −1, −1) never enters. Take topic 10.06's converged determinant |Φ₀⟩ with canonical orbitals, f|i⟩ = εᵢ|i⟩ and εᵢ = hᵢᵢ + Σⱼ (Jᵢⱼ − Kᵢⱼ), quoted. Annihilate orbital k and keep every other orbital as it was: |Φₖ⟩ = cₖ|Φ₀⟩. Topic 10.05's contractions give its energy with k simply absent. hₖₖ leaves the one-body sum, and the pairs (k, j) and (j, k), each weighted ½, leave the two-body sum. What leaves is hₖₖ + Σⱼ (Jₖⱼ − Kₖⱼ) = εₖ, so E(N − 1; k) = EHF − εₖ, derived. The same contraction with c†ₐ on a virtual gives E(N + 1; a) = EHF + εₐ, the affinity version. Dimensions: every term is an energy. Limit: a single electron has nobody to repel, so ε = h = E and the theorem is exact; hydrogen's −ε = 13.606 eV becomes the measured 13.598 eV once the reduced mass is put in.

2Why the total energy is not the sum of the εᵢ

Add the orbital energies over occupied spin-orbitals: Σεᵢ = Σhᵢᵢ + Σᵢⱼ (Jᵢⱼ − Kᵢⱼ). The determinant's energy carries the same pair sum with a factor ½, so EHF = Σεᵢ − ½Σᵢⱼ (Jᵢⱼ − Kᵢⱼ) = ½Σᵢ (hᵢᵢ + εᵢ), derived. The cause is bookkeeping, not approximation: εᵢ prices electron i in the field of all the others, so the repulsion between i and j sits in εᵢ and again in εⱼ. Closed-shell helium makes it concrete. Its two spin-orbitals share ε = −0.91796 Eₕ = −24.98 eV and EHF = −2.86168 Eₕ = −77.87 eV, values topic 10.08 computes; 2ε = −49.96 eV lies J = 2ε − EHF = 1.02577 Eₕ = 27.91 eV above it, the one 1s-1s repulsion that both orbital energies contain. For one electron the pair sum is empty and E = ε, as it should be. The same arithmetic forbids adding ionisation energies read from one calculation. The first electron costs about 25 eV, the second 54.42 eV from He⁺, whose orbital has contracted, and only their measured sum, 79.0 eV, is the atom's binding energy.

3Canonical orbitals are the ones with an ionisation energy

EHF does not care which orthonormal basis of the occupied space you use: a unitary mixing U of occupied orbitals multiplies the determinant by det U, a phase. Orbital energies do care. Remove instead a normalised mixture u = Σₖ Uₖ φₖ, freezing the rest, and the same contraction raises the energy by −⟨u|f|u⟩ = −Σ Uₖ* Fₖₗ Uₗ, minus a Rayleigh quotient of the occupied block of the Fock matrix. It is stationary under every small change of U exactly when F U = ε U, that is, when u is a canonical orbital, derived. That was Koopmans' own 1934 result. Canonical orbitals are therefore not one choice among equals: they are the orbitals whose removal energy is stationary, and the ones a photoelectron spectrum sees. Methane shows it. Four equivalent C-H bond orbitals describe its ground state exactly as well as the canonical a₁ and t₂ orbitals, yet the measured spectrum has two valence bands, near 23 eV and 14 eV, in a one-to-three pattern, and no band for a single bond.

4Brillouin's theorem is the stationarity condition

Put occupied orbital i into virtual a: |Φᵢᵃ⟩ = c†ₐcᵢ|Φ₀⟩. Contracting H between it and Φ₀ leaves hₐᵢ + Σⱼ ⟨aj||ij⟩ = ⟨a|f|i⟩, derived. Now rotate i towards a through an angle θ. A determinant is linear in each orbital, so Φ(θ) = cos θ Φ₀ + sin θ Φᵢᵃ exactly, and for real orbitals E(θ) = E₀ + Δ sin²θ + ⟨Φᵢᵃ|H|Φ₀⟩ sin 2θ with Δ = ⟨Φᵢᵃ|H|Φᵢᵃ⟩ − E₀. The slope at θ = 0 is 2⟨Φᵢᵃ|H|Φ₀⟩. Topic 10.06 made E stationary under every such rotation, so every single-excitation coupling vanishes: ⟨Φᵢᵃ|H|Φ₀⟩ = ⟨a|f|i⟩ = 0. Brillouin's theorem is not an extra fact about Hartree-Fock; it is Hartree-Fock, written as a statement about matrix elements. It needs stationarity only, not canonical orbitals, and it fails for any determinant short of convergence, where the slope 2⟨a|f|i⟩ tells the next iteration which way to rotate.

5Doubles carry the first correction

Expand the exact ground state in determinants built from the Hartree-Fock orbitals, Ψ = c₀Φ₀ + Σ cᵢᵃΦᵢᵃ + Σ cᵢⱼᵃᵇΦᵢⱼᵃᵇ + …, which is configuration interaction, named here. H is a two-body operator, so it links Φ₀ to nothing beyond doubles, and Brillouin removes the singles. The first-order wavefunction of Rayleigh-Schrödinger theory, quoted from Quantum Mechanics II, therefore contains doubles only, and the leading energy correction is a sum over them. With H₀ = Σ f(n), whose determinant energies are sums of εᵢ, it is Møller-Plesset second order, E⁽²⁾ = −Σ |⟨ab||ij⟩|²/(εₐ + εb − εᵢ − εⱼ), quoted and not pursued. Every term is negative, and one electron has no pairs, so E⁽²⁾ = 0 and Hartree-Fock is exact there, as it must be. Singles are not absent from Ψ: they enter at second order through their coupling to the doubles. What Brillouin forbids is the direct step. The orbital energies also earn a second job here: their differences are the denominators.

6Relaxation and correlation pull in opposite directions

Koopmans' ion is not stationary. Its own Fock operator lacks the departed electron, f − Jₖ + Kₖ, so its Brillouin element for j → a is −⟨ak||jk⟩, not zero: the hole pulls the remaining orbitals inward, and letting them rotate lowers the ion. Relaxation therefore always makes −εₖ too large. Correlation pushes the other way, because the N-electron atom has more pairs to correlate than its ion and is lowered more. For helium, quoted from topic 10.08: −ε = 24.98 eV, relaxation 1.53 eV, correlation 1.14 eV, leaving Koopmans 0.39 eV above the measured 24.587 eV. Neon's 2p gives −ε = 23.14 eV against the measured 21.56 eV. A core hole relaxes far more: neon's −ε₁ₛ = 891.8 eV overshoots the measured 870.2 eV by 21.6 eV, as eight outer electrons contract onto a hole that acts on them like an extra nuclear charge. In a large system a delocalised hole spreads over N sites and the relaxation falls away as N grows, which is why band theory may read Hartree-Fock bands as removal energies. For affinities both errors raise the true value, so −εₐ fails worst.

2

Key equations

Read the units, assumptions and limits before substituting.

Koopmans' theorem

E(N − 1k) − EHF = −εₖ, so IEₖ ≈ −εₖ

Removing k takes out hₖₖ and k's whole repulsion with the others, which is εₖ. Exact for one electron: hydrogen's −ε is 13.6 eV.

εₖ = ⟨k|f|k⟩ for occupied canonical orbital k; energies in eV, with Eₕ = 27.211 eV; other orbitals frozen; derived

Total energy is not the sum of the εᵢ

EHF = Σᵢ εᵢ − ½ Σᵢⱼ (Jᵢⱼ − Kᵢⱼ)

Each εᵢ holds electron i's repulsion with all the others, so Σεᵢ counts every pair twice. Helium: EHF = 2ε − J = −77.87 eV, not 2ε = −49.96 eV.

sums over occupied spin-orbitals; Jᵢⱼ, Kᵢⱼ the direct and exchange integrals of topic 10.05, in eV; derived

Why canonical orbitals

IE(u) = −⟨u|f|u⟩ for u = Σₖ Uₖ φₖ, stationary only when f u = ε u

EHF is unchanged by any unitary mixing of occupied orbitals; removal energies are not. A localised bond orbital gives an average of bands, not a band.

U a normalised vector of occupied amplitudes; φₖ occupied orbitals; ⟨u|f|u⟩ in eV; derived

Brillouin's theorem

⟨Φᵢᵃ|H|Φ₀⟩ = ⟨a|f|i⟩ = 0

The contraction leaves the occupied-virtual element of f, and Hartree-Fock stationarity sets that whole block to zero, canonical orbitals or not.

Φᵢᵃ = c†ₐcᵢΦ₀ puts occupied i into virtual a; f the Fock operator; matrix elements in eV; derived

One orbital rotated into a virtual

E(θ) = E₀ + Δ sin²θ + ⟨Φᵢᵃ|H|Φ₀⟩ sin 2θ

The slope at θ = 0 is 2⟨Φᵢᵃ|H|Φ₀⟩, so a stationary determinant is one with no single-excitation coupling: Brillouin and Hartree-Fock are one condition.

θ the rotation angle; Δ = ⟨Φᵢᵃ|H|Φᵢᵃ⟩ − E₀ in eV; real orbitals; exact, since Φ(θ) = cos θ Φ₀ + sin θ Φᵢᵃ

First correction: doubles only

E⁽²⁾ = −Σ |⟨ab||ij⟩|² / (εₐ + εb − εᵢ − εⱼ)

Brillouin removes singles and the two-body H removes triples and beyond. Every term is negative, and with one electron there are no pairs, so E⁽²⁾ = 0.

each occupied pair ij and virtual pair ab once; ⟨ab||ij⟩ = ⟨ab|v|ij⟩ − ⟨ab|v|ji⟩ in eV; Møller-Plesset, quoted
3

Interactive lab

Predict first. Explore the model. Compare the result.

Explore the model

0.0 eV
−8 to 8 eV; steps of 0.5.
8.4 eV
0 to 10 eV; steps of 0.2.
44 eV
16 to 50 eV; steps of 2.

Try this. Start at b = 0: the left minimum sits at θ = 0, which is Brillouin's theorem. Move b and it slides off, the mark of an unconverged determinant. The default, v = 8.4 eV across Δ = 44 eV, relaxes by 1.55 eV, close to helium's 1.53 eV; raise v and ER grows, near v²/Δ while v is small against Δ.

Live results

NEUTRAL GAIN ON ROTATING
0.000 eV
ION RELAXATION ER
1.55 eV
SECOND ORDER v²/Δ
1.60 eV
ION ROTATION ANGLE
-10.4 °

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

Interactive Advanced Quantum Mechanics modelEnergy against the angle θ through which one occupied orbital turns into a virtual, both with gap Δ = 44 eV. Left, the N-electron determinant: slope 2b = 0.0 eV at θ = 0, zero for converged Hartree-Fock orbitals. Right, Koopmans' frozen ion: the hole's pull v = 8.4 eV tilts it, and relaxing lowers it by 1.55 eV, relaxation's share of −εₖ's overshoot.N electrons: E(θ) − E₀N − 1: E(θ) − (E₀ − εₖ)slope at 0: 2b = 0.0 eVion relaxes by 1.55 eVrelaxed ionθ = −45°+45°θ = −45°+45°
Energy against the angle θ through which one occupied orbital turns into a virtual, both with gap Δ = 44 eV. Left, the N-electron determinant: slope 2b = 0.0 eV at θ = 0, zero for converged Hartree-Fock orbitals. Right, Koopmans' frozen ion: the hole's pull v = 8.4 eV tilts it, and relaxing lowers it by 1.55 eV, relaxation's share of −εₖ's overshoot.

Predict → change one variable → check

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

Saved baseline. Neutral coupling b = ⟨Φᵢᵃ|H|Φ₀⟩: 0.0 eV; Hole's pull v on the frozen ion: 8.4 eV; Rotation gap Δ (both panels): 44 eV

Baseline 0.0; choose −8 to 8, in steps of 0.5.
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 tempting reading is that an orbital energy is the energy one electron has, so the atom's energy must be the sum of its orbital energies. It is wrong by the whole electron repulsion. εᵢ is the cost of removing electron i from the field of all the others, so the repulsion of each pair is counted once in εᵢ and again in εⱼ, and EHF = Σεᵢ − ½Σᵢⱼ (Jᵢⱼ − Kᵢⱼ). For helium the error is J = 27.9 eV, over a third of the binding energy. The same slip appears when −ε of every occupied orbital is added and called the total binding energy: helium's two orbital energies give 49.96 eV, while its two measured ionisation energies add to 79.0 eV, because the second electron is removed from He⁺, whose orbital has already contracted. Orbital energies describe one-electron removals from a fixed atom, never shares of its total energy.

5

Practice & worked examples

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

EasyExample 1

A converged restricted Hartree-Fock calculation on the two-electron ion Li⁺ (1s²) returns EHF = −7.2364 Eₕ and ε₁ₛ = −2.7924 Eₕ, with Eₕ = 27.211 eV. Estimate the energy to ionise Li⁺ to Li²⁺ by Koopmans' theorem and compare it with the measured 75.640 eV. Then use the two numbers alone to find the 1s-1s Coulomb integral J and the one-electron energy h.

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.

MediumExample 2

In a converged closed-shell molecule the highest occupied orbital k has −εₖ = 15.80 eV. In the frozen ion with k emptied, keep one relaxation channel, occupied j into virtual a, with ⟨a|f|j⟩ = 0 in the neutral, ⟨ak||jk⟩ = 1.50 eV, and the rotated ion lying Δ = 9.00 eV above the frozen one. Find the ion's single-excitation coupling, its relaxation energy and rotation angle, and the corrected ionisation energy, and compare with second order.

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

A tetrahedral molecule's four doubly occupied valence orbitals are rewritten as equivalent localised bond orbitals λ₁ … λ₄. In that basis the occupied block of the Fock matrix has every diagonal element α = −0.640 Eₕ and every off-diagonal element β = −0.100 Eₕ. Find the canonical orbital energies and Koopmans' ionisation energies, decide whether removal from λ₁ has a stationary energy, and check that EHF is the same in both descriptions.

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.

6

Quick check

Select an answer and explain it before checking.

Expand the exact ground state of a closed-shell atom in determinants built from its converged Hartree-Fock orbitals: Ψ = c₀Φ₀ + Σ cᵢᵃΦᵢᵃ + Σ cᵢⱼᵃᵇΦᵢⱼᵃᵇ + …. Which statement about the singly excited determinants Φᵢᵃ is right?
7

Review & continue

Koopmans' theorem: with every other orbital frozen, removing an electron from canonical Hartree-Fock orbital k costs −εₖ. Brillouin's theorem: H has no matrix element between the converged determinant and any singly excited one.

  • 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.