
Advanced Quantum Mechanics course sequence · Interactive lesson
One-body operators: the sum of ⟨i|f|j⟩ c†ᵢ cⱼ
Kinetic energy, a potential, a dipole moment, a spin: everything you measured on one particle has to be rewritten before it can act on Fock space. Here the rewriting is done once and proved, then put to work on the density, on helium's singlet, and on which states a single photon can reach.
UAQM-10.03 · Lesson 3 of 9 in this unit. Position is not a completion score.Build the model
Every single-particle observable becomes one operator for every particle number.
The key idea
A one-body operator is the sum of one single-particle operator f over all the particles; in second quantisation it is F = Σᵢⱼ ⟨i|f|j⟩ c†ᵢ cⱼ, each term emptying orbital j and filling orbital i with amplitude ⟨i|f|j⟩.
Example. If ⟨2|f|1⟩ = 0.30 eV, the term (0.30 eV) c†₂ c₁ turns c†₁ c†₃|0⟩ into (0.30 eV) c†₂ c†₃|0⟩, moving the electron in orbital 1 to orbital 2 and leaving orbital 3 alone; on c†₂ c†₃|0⟩ it gives zero, orbital 1 being empty.
The complete physical model and assumptions
A one-body operator acts on particles one at a time: kinetic energy, an external potential, position and dipole moment, spin. In first quantisation it is Σₙ f(n), N copies of f acting on functions of N coordinates, so the kinetic energy of two electrons and of three are different operators on different spaces. Fock space needs one operator for all of them, and the answer is to promote the ket-bra |i⟩⟨j| to c†ᵢ cⱼ: F = Σᵢⱼ ⟨i|f|j⟩ c†ᵢ cⱼ. That is derived, not guessed. On a determinant, c†ᵢ cⱼ writes orbital i into the slot j held, its two ordering signs cancelling; Σₙ f(n) on a Slater determinant replaces one column at a time by f acting on that orbital, and expanding over the same basis gives the same determinants with the same coefficients. Determinants span every N-particle space, so the two are equal. What follows is bookkeeping with physics in it: a determinant's expectation value is a sum over occupied orbitals, ψ†fψ makes F basis-free, commutators of one-body operators stay one-body, and F cannot join determinants differing in two orbitals. The construction stops at anything acting on pairs, the Coulomb repulsion or S² itself, which needs c†c†cc and topic 10.04; a finite basis keeps only the part of f inside the orbitals it spans; and particle number is assumed fixed, as topic 10.01 arranged below the pair threshold.
1c†ᵢ cⱼ empties one orbital and fills another, in place
SI units throughout; x stands for position and spin together, and nothing here is relativistic, so Unit 9's (+, −, −, −) metric never enters. Order a set of orthonormal spin-orbitals once and for all, and write a determinant as an ordered product of creators on |0⟩, with topic 10.01's anticommutators quoted. Act with c†ᵢ cⱼ. If orbital j is empty, cⱼ reaches |0⟩ and gives zero. If j stands in slot k, cⱼ anticommutes past k − 1 creators, a sign (−1)(k−1), and removes c†ⱼ; c†ᵢ then needs k − 1 swaps to reach slot k, the same sign again. The signs cancel: c†ᵢ cⱼ writes i into j's slot and leaves every other orbital where it was. If i is another occupied orbital, c†ᵢ appears twice and the result vanishes, the Pauli principle; if i = j the state comes back, so c†ⱼ cⱼ = nⱼ counts. With three orbitals, c†₃ c₁ c†₁ c†₂|0⟩ = c†₃ c†₂|0⟩ = −c†₂ c†₃|0⟩: the minus sign appears only when the result is put back into the standard order.
2The first-quantised sum does the same, sign for sign
Now apply F⁽ᴺ⁾ = Σₙ f(n) to the Slater determinant of the same orbitals, (1/√N!) det[φ(xₙ)]. Each term of the determinant has one orbital per coordinate and f(n) acts on one factor, so F⁽ᴺ⁾ returns a sum of N determinants, the k-th with its column-k orbital φⱼ replaced by fφⱼ. Insert completeness, fφⱼ = Σᵢ φᵢ ⟨i|f|j⟩. A column equal to another occupied orbital kills its determinant; otherwise orbital i stands in j's slot with the rest untouched. That is, term for term and sign for sign, what Σᵢⱼ ⟨i|f|j⟩ c†ᵢ cⱼ produced. Determinants of a complete orthonormal set span every N-particle space, so equal action on all of them makes the operators equal: derived. Three checks. c†ᵢ cⱼ is dimensionless, so F has the unit of f. For N = 1, ⟨0|cₖ F c†ₗ|0⟩ = ⟨k|f|l⟩, the one-particle operator itself. And F|0⟩ = 0: an empty box has no kinetic energy. Nothing in F mentions N, so one operator serves every N and conserves it, each term holding one creator and one annihilator.
3Kinetic energy, external potential and density
Substituting ψ(x) = Σᵢ φᵢ(x) cᵢ from topic 10.02 folds the double sum into F = ∫ dx ψ†(x) f ψ(x); since ⟨i|f|j⟩ and c†ᵢ cⱼ change by inverse unitary matrices, F is the same in every basis. Kinetic energy is T = ∫ dx ψ†(−ħ²∇²/2m)ψ, diagonal in plane waves: T = Σ (ħ²k²/2m) c†(k, σ) c(k, σ). A potential U(r) gives V = ∫ d³r U(r) n(r), where n(r) = Σσ ψ†σ(r) ψσ(r) is the second-quantised Σₙ δ³(r − rₙ), in m⁻³. In a box of volume Ω, V = (1/Ω) Σ Ũ(q) c†(k + q, σ) c(k, σ), with Ũ the Fourier transform of U: the potential scatters one electron by q at a time. On a determinant only diagonal terms survive, so ⟨Φ|F|Φ⟩ = Σ over occupied i of ⟨i|f|i⟩. Helium's effective-charge determinant, Zeff = 27/16, has ⟨T⟩ = 2(27/16)² × 13.606 eV = 77.5 eV. The virial theorem, quoted, turns the measured total energy, −79.0 eV, into ⟨T⟩ = 79.0 eV: this determinant misses 1.5 eV of kinetic energy.
4Total spin, and the singlet check
Spin is one-body too. A spin-orbital is a spatial orbital times ↑ or ↓, with single-particle elements ⟨a↑|sz|a↑⟩ = ħ/2, ⟨a↓|sz|a↓⟩ = −ħ/2 and ⟨a↑|s₊|a′↓⟩ = ħ⟨a|a′⟩, so Sz = (ħ/2) Σₐ (nₐ↑ − nₐ↓) and S₊ = ħ Σₐ c†ₐ↑ cₐ↓, derived. Put two electrons in one spatial orbital, Φ = c†ₐ↑ c†ₐ↓|0⟩. Only the a term of S₊ acts: cₐ↓ anticommutes past c†ₐ↑ and removes c†ₐ↓, leaving −c†ₐ↑ c†ₐ↑|0⟩ = 0. So S₊Φ = 0 and SzΦ = 0, and S² = S₋S₊ + Sz² + ħSz gives S²Φ = 0: a singlet, which written out is Quantum Mechanics II's φ(r₁)φ(r₂)(↑↓ − ↓↑)/√2, recovered as a check. The same cancellation makes every closed shell a singlet. Experiment agrees: helium's 1s² ground state is ¹S₀ with no triplet partner, and its lowest triplet level, 1s2s ³S₁, lies 19.82 eV higher. Different orbitals behave differently: S₊ c†ᵤ↑ c†ᵥ↓|0⟩ = ħ c†ᵤ↑ c†ᵥ↑|0⟩, whose squared norm ħ²(1 − |⟨u|v⟩|²) vanishes only when v is u itself, up to a phase.
5One electron at a time: which determinants F can join
Every term of F moves at most one electron, so its matrix elements between determinants of one orthonormal set take one of three forms, fixed by how many spin-orbitals differ, derived. None: ⟨Φ|F|Φ⟩ = Σ over occupied i of ⟨i|f|i⟩. One, a replaced by r in a's slot: ⟨r|f|a⟩. Two or more: zero, however large the single-particle elements are. The electric-dipole operator D = −e Σₙ rₙ is one-body and blind to spin, so between single determinants a photon moves one electron, keeps its spin, and needs a non-zero one-electron element. Helium bears this out. Its strongest absorption line from the ground state is at 58.4 nm, 21.22 eV: 1s² → 1s2p ¹P, one orbital changed. A one-photon jump to 2s2p changes two orbitals and has no amplitude between determinants, yet Madden and Codling found it in 1963, a resonance near 60.1 eV in helium's synchrotron absorption, because neither state is really a single determinant. Any intensity in a two-electron jump measures correlation, the part of the wavefunction one determinant leaves out.
6Commutators stay one-body; products do not
From the anticommutators, [c†ᵢ cⱼ, c†ₖ cₗ] = δⱼₖ c†ᵢ cₗ − δᵢₗ c†ₖ cⱼ, derived in two lines: the rule |i⟩⟨j| obeys. So the commutator of two one-body operators is the one-body operator of [f, g], and second quantisation preserves commutators. The components of S obey [Sₓ, Sy] = iħSz for every N with no further work, and [T, X] for X = Σₙ xₙ is the one-body operator of [p²/2m, x] = −iħp/m. Products differ. In FG, writing cⱼ c†ₖ = δⱼₖ − c†ₖ cⱼ splits Σ fᵢⱼ gₖₗ c†ᵢ cⱼ c†ₖ cₗ into a one-body piece with matrix fg and a remainder Σ fᵢⱼ gₖₗ c†ᵢ c†ₖ cₗ cⱼ that moves two electrons at once, the second-quantised sum of f(n)g(m) over n ≠ m. S² = S⋅S is the case that matters: its pair part, 2 Σ sₙ⋅sₘ over n < m, is two-body, which is why a determinant can be an eigenstate of Sz and not of S². Operators acting on pairs are topic 10.04's.
Key equations
Read the units, assumptions and limits before substituting.
One-body operator on Fock space
F = Σᵢⱼ ⟨i|f|j⟩ c†ᵢ cⱼ
One operator in place of a separate Σₙ f(n) for each N: it gives F|0⟩ = 0 on the vacuum and ⟨0|cₖ F c†ₗ|0⟩ = ⟨k|f|l⟩ for one particle.
f: single-particle operator; ⟨i|f|j⟩ in f's unit, J for an energy; c†ᵢ cⱼ is dimensionless; i, j run over spin-orbitals. Derived.One electron moved, in place
c†ᵢ cⱼ |… j …⟩ = |… i …⟩
The same replacement, sign included, that Σₙ f(n) makes on one column of a Slater determinant: that match is the whole proof that the two forms agree.
i takes j's slot in the ordered product, so the two ordering signs cancel; zero if j is empty or i ≠ j is filled. Derived.Basis-free form with field operators
F = ∫ dx ψ†(x) f ψ(x)
Kinetic energy is ∫ dx ψ†(−ħ²∇²/2m)ψ. A basis rotation of topic 10.02 changes ⟨i|f|j⟩ and c†ᵢ cⱼ by inverse matrices, so F is the same in every basis.
x = (r, σ), and ∫ dx sums over σ and integrates over r; ψ carries m⁻³⁄², so ψ†ψ is in m⁻³. Derived from ψ = Σᵢ φᵢ cᵢ.Density operator
n(r) = Σσ ψ†σ(r) ψσ(r) ↔ Σₙ δ³(r − rₙ)
A local potential then reads V = ∫ d³r U(r) n(r), and the number operator is N̂ = ∫ d³r n(r) = Σᵢ c†ᵢ cᵢ.
n in m⁻³. For a determinant Φ, ⟨Φ|n(r)|Φ⟩ = Σ over occupied i of |φᵢ(r)|². Derived.Total spin raising operator
S₊ = ħ Σₐ c†ₐ↑ cₐ↓
On c†ₐ↑ c†ₐ↓|0⟩ it produces c†ₐ↑ twice, which is zero, so with Sz = 0 a doubly occupied orbital is a singlet: Quantum Mechanics II's paired state.
a runs over spatial orbitals; ħ in J s; alongside it Sz = (ħ/2) Σₐ (nₐ↑ − nₐ↓). Derived from ⟨↑|s₊|↓⟩ = ħ.Matrix elements between determinants
⟨Φ′|F|Φ⟩ = 0 if Φ′ and Φ differ in two or more spin-orbitals
One-photon dipole absorption, with D = −e Σₙ rₙ, therefore moves one electron between determinants; any two-electron jump needs correlation.
One difference, a replaced by r in a's slot: ⟨r|f|a⟩. No difference: Σ over occupied i of ⟨i|f|i⟩. Both built from one orthonormal set. Derived.Interactive lab
Predict first. Explore the model. Compare the result.
Explore the model
Try this. Start at θ = 0: both electrons share u, the curves coincide, S₊ annihilates Φ and the state is a pure singlet. Raise θ to 90° and the triplet weight climbs to one half. Then change k at fixed θ: the densities reshape but the bars stay put, because S₊ sees only the overlap.
Live results
- OVERLAP ⟨u|v⟩
- 0.64
- ⟨S²⟩ = ‖S₊Φ‖²
- 0.59 ħ²
- TRIPLET WEIGHT
- 0.29
- SINGLET WEIGHT
- 0.71
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. Mixing angle θ: 50 °; Admixed box level k: 2
This experiment is kept only while this page is open. It does not change saved course progress.
Catch the common trap
The tempting step is from S = Σₙ sₙ being one-body to S² being one-body too, and from there to every Slater determinant with Sz = 0 having a definite total spin, or even being a singlet. Both are wrong. Squaring a sum of one-particle terms gives S² = Σₙ sₙ² + 2 Σ sₙ⋅sₘ over pairs n < m, and the pair sum is a two-body operator, quartic in c and c†. A determinant is guaranteed to be an eigenstate only of one-body operators diagonal in its own orbitals, such as N̂ and Sz, and S² is neither. Work instead from one-body pieces, S² = S₋S₊ + Sz² + ħSz. With two electrons of opposite spin in orthogonal orbitals the norm of S₊Φ is ħ, so ⟨S²⟩ = ħ², halfway between a singlet's 0 and a triplet's 2ħ²: the determinant is an equal mixture. Only a doubly occupied orbital, where S₊ meets c†ₐ↑ twice, is a singlet.
Practice & worked examples
3 authored examples. Make an attempt, then reveal the reasoning one step at a time.
EasyExample 1
Electrons sit in a one-dimensional box of length L = 0.80 nm. Write the kinetic energy in second quantisation on the box orbitals, then apply the same operator to the vacuum, to one electron in c†₂↑|0⟩, and to four electrons in c†₁↑ c†₁↓ c†₂↑ c†₂↓|0⟩.
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.
- The box orbitals diagonalise t = p²/2m, with ⟨n|t|n′⟩ = n²E₁ when n′ = n and 0 otherwise, so T = Σ over n and σ of n²E₁ c†ₙσ cₙσ: a weighted count of occupations.
- E₁ = h²/(8mL²) = (6.626 × 10⁻³⁴ J s)² / (8 × 9.109 × 10⁻³¹ kg × (0.80 × 10⁻⁹ m)²) = 9.41 × 10⁻²⁰ J = 0.588 eV.
- Vacuum: every occupation is 0, so T|0⟩ = 0. One electron: only orbital 2↑ is filled, so T c†₂↑|0⟩ = 4E₁ c†₂↑|0⟩ with 4E₁ = 2.35 eV, Quantum Mechanics I's n = 2 box level: the one-particle limit.
- Four electrons: the filled spin-orbitals are 1↑, 1↓, 2↑ and 2↓, so the eigenvalue is (1 + 1 + 4 + 4)E₁ = 10E₁ = 5.88 eV. No new operator was needed, only a different state.
- Checks: the occupations are pure numbers, so T carries E₁'s unit, an energy. The closed shell is also a singlet, S₊Φ = 0: the terms of S₊ with a = 1 and 2 meet an ↑ place already full, and every higher term finds no ↓ electron to move.
Answer. T|0⟩ = 0; T gives 2.35 eV on c†₂↑|0⟩ and 5.88 eV on the four-electron closed shell, all from one operator, Σ n²E₁ c†ₙσ cₙσ with E₁ = 0.588 eV.
MediumExample 2
Excited helium is described by the determinant Φ = c†₁ₛ↑ c†₂ₛ↓|0⟩. Use S₊ = ħ Σₐ c†ₐ↑ cₐ↓ to find ⟨S²⟩ and the singlet and triplet weights. Then, with the measured 1s2s levels, ³S₁ at 19.820 eV and ¹S₀ at 20.616 eV above the ground state, find ⟨H⟩ and how long Φ takes to become c†₁ₛ↓ c†₂ₛ↑|0⟩.
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.
- Only the 2s term of S₊ finds a ↓ electron. c₂ₛ↓ anticommutes past c†₁ₛ↑, a factor −1, and removes c†₂ₛ↓; then c†₂ₛ↑ c†₁ₛ↑ = −c†₁ₛ↑ c†₂ₛ↑. So S₊Φ = ħ c†₁ₛ↑ c†₂ₛ↑|0⟩, the M = 1 triplet, with norm ħ because 1s and 2s are orthogonal.
- SzΦ = 0, so ⟨S²⟩ = ‖S₊Φ‖² + ⟨Sz²⟩ + ħ⟨Sz⟩ = ħ². Two electrons can only have S² = 0 or 2ħ², so the triplet weight is ħ²/(2ħ²) = 1/2 and the singlet weight is the other 1/2.
- Written out, Φ = (|T₀⟩ + |S⟩)/√2, with T₀ and S the M = 0 triplet and the singlet built from 1s and 2s. Treating the measured levels as their energies, ⟨H⟩ = (19.820 + 20.616)/2 eV = 20.218 eV above the ground state, with spread (20.616 − 19.820)/2 eV = 0.398 eV.
- The two parts dephase at ΔE = 0.796 eV. After h/(2ΔE) = (4.136 × 10⁻¹⁵ eV s)/(2 × 0.796 eV) = 2.60 fs their relative sign has flipped, giving (|T₀⟩ − |S⟩)/√2 = c†₁ₛ↓ c†₂ₛ↑|0⟩: the spins have exchanged orbitals.
- Checks: h/ΔE has the unit of time, and in the limit 2s → 1s the determinant becomes the closed shell, where S₊Φ = 0, ⟨S²⟩ = 0 and nothing oscillates. The mixing belongs to the open shell.
Answer. ⟨S²⟩ = ħ², so the weights are 1/2 singlet and 1/2 triplet; ⟨H⟩ = 20.22 eV above the ground state with spread 0.40 eV, and the spins exchange orbitals after 2.60 fs.
HardExample 3
Three electrons in a one-dimensional box of length L = 1.00 nm occupy Φ = c†₁↑ c†₁↓ c†₂↑|0⟩, with spin-orbitals ordered 1↑, 1↓, 2↑, 2↓, 3↑, 3↓. Given ⟨i|x|j⟩ = −8ijL/(π²(i² − j²)²) for i + j odd and 0 for i + j even (i ≠ j), find every excited determinant within orbitals 1 to 3 that X = Σₙ xₙ connects to Φ, with its signed element, ΔE and f = (2mΔE/ħ²)|⟨Φ′|X|Φ⟩|².
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.
- Second quantise: X = Σ over i, j and σ of ⟨i|x|j⟩ c†ᵢσ cⱼσ. No term changes σ and each term moves one electron, so only single replacements out of Φ appear; a determinant differing from Φ in two orbitals, such as c†₁↑ c†₂↓ c†₃↑|0⟩, gets zero.
- Screen the single moves. 1↑ → 2↑ and 2↑ → 1↑ land on filled places, so Pauli blocks them. 1↑ → 3↑ and 1↓ → 3↓ have i + j even, so ⟨3|x|1⟩ = 0. Moves that flip a spin are absent from X. Two survive: 1↓ → 2↓ and 2↑ → 3↑.
- Signs. c₁↓ passes c†₁↑, a factor −1, and c†₂↓ joins after c†₂↑: c†₂↓ c₁↓ Φ = −c†₁↑ c†₂↑ c†₂↓|0⟩, so that element is −⟨2|x|1⟩ = +16L/(9π²) = +0.180 L. c†₃↑ takes 2↑'s slot: c†₃↑ c₂↑ Φ = +c†₁↑ c†₁↓ c†₃↑|0⟩, element ⟨3|x|2⟩ = −48L/(25π²) = −0.195 L. First quantisation agrees: φ₂↓ in column 2 of det(φ₁↑, φ₁↓, φ₂↑) needs one swap to reach standard order.
- Energies, with E₁ = h²/(8mL²) = 0.376 eV: ΔE = (4 − 1)E₁ = 1.13 eV and (9 − 4)E₁ = 1.88 eV. Since 2mE₁/ħ² = π²/L², f = (ΔE/E₁)π²(element/L)², which is dimensionless as it must be: 3π²(0.1801)² = 0.961 and 5π²(0.1945)² = 1.87.
- Check: the Thomas-Reiche-Kuhn sum rule, quoted, makes f summed over all final determinants equal N = 3. These two carry 2.83 and moves into orbitals 4 and above carry the remaining 0.17. The Pauli-blocked pair would have carried +0.961 and −0.961, so blocking them costs the sum nothing.
Answer. c†₁↑ c†₂↑ c†₂↓|0⟩: element +0.180 L, ΔE = 1.13 eV, f = 0.961. c†₁↑ c†₁↓ c†₃↑|0⟩: element −0.195 L, ΔE = 1.88 eV, f = 1.87. Every other excited determinant within orbitals 1 to 3 gives zero.
Quick check
Select an answer and explain it before checking.
Review & continue
A one-body operator is the sum of one single-particle operator f over all the particles; in second quantisation it is F = Σᵢⱼ ⟨i|f|j⟩ c†ᵢ cⱼ, each term emptying orbital j and filling orbital i with amplitude ⟨i|f|j⟩.
- 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.