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Number Operators and Conserved Quantities

The total number operator counts the particles or quanta represented by a chosen set of modes:

N^=∑iai†ai.\widehat N = \sum_i a_i^\dagger a_i.

Its many-body role is broader than counting. It generates a global U(1)U(1) transformation, decomposes Fock space into fixed-number sectors, supplies selection rules, and gives a one-line test for whether a Hamiltonian preserves particle number:

[H,N^]=0.[H,\widehat N] = 0.

The spectra and elementary ladder commutators are developed in Number Operators. This page is the many-body application guide: symmetry, charge counting, sector projectors, weighted conserved quantities, grand-canonical use, local versus global conservation, number-breaking mean field, fermion parity, and open-system sources.

Unless stated otherwise:

  • ai,ai†a_i,a_i^\dagger denote bosonic or fermionic mode operators;
  • ni=ai†ain_i=a_i^\dagger a_i is the occupation of complete mode ii;
  • N^=∑ini\widehat N=\sum_i n_i is the total number operator;
  • NN without a hat is an eigenvalue of N^\widehat N;
  • ΠN\Pi_N projects onto the fixed-NN sector HN\mathcal H_N;
  • HH acts on Fock space and is Hermitian;
  • Mp,qM_{p,q} is a monomial with pp creation and qq annihilation operators;
  • U(θ)=e−iθN^U(\theta)=e^{-i\theta\widehat N} is the chosen global U(1)U(1) convention.

With the opposite sign in the exponential, every phase below reverses. Conservation statements are unchanged.

This page owns the practical relation among:

  • number operators and global U(1)U(1) symmetry;
  • charge counting of many-body operator strings;
  • fixed-number blocks and selection rules;
  • exact, explicit, spontaneous, and effective number breaking;
  • exact reduced BCS pairing versus number-breaking BCS mean field;
  • total number, local number, and reservoir exchange;
  • numerical conservation checks.

Other pages retain their canonical roles:

Each mode number is

ni=ai†ai.n_i = a_i^\dagger a_i.

Its eigenvalue depends on statistics:

ni∈{{0,1,2,…},bosons,{0,1},fermions.n_i \in \begin{cases} \{0,1,2,\ldots\},&\text{bosons},\\ \{0,1\},&\text{fermions}. \end{cases}

The total operator is the sum over the complete one-particle mode basis:

N^=∑ini.\widehat N = \sum_i n_i.

Individual nin_i depend on the chosen modes. The total N^\widehat N does not change under a unitary rotation of the complete one-particle basis.

The identity on the one-particle Hilbert space lifts to total number:

N^=dΓ(IH1).\widehat N = d\Gamma(I_{\mathcal H_1}).

This explains several facts at once:

  • N^\widehat N is additive over particles;
  • it has eigenvalue NN on the NN-particle sector;
  • it is basis independent;
  • it is the natural generator of a common phase rotation of every mode.

The relation to general additive observables is developed in One-Body Operators.

Bosonic or fermionic Fock space decomposes as

F=⨁N∈SHN,\mathcal F = \bigoplus_{N\in\mathcal S} \mathcal H_N,

where S={0,1,2,…}\mathcal S=\{0,1,2,\ldots\} for an untruncated bosonic Fock space. For MM fermionic modes,

S={0,1,…,M}.\mathcal S = \{0,1,\ldots,M\}.

The spectral resolution of total number is

N^=∑N∈SNΠN,\widehat N = \sum_{N\in\mathcal S} N\Pi_N,

with

ΠNΠM=δNMΠN,∑NΠN=I.\Pi_N\Pi_M = \delta_{NM}\Pi_N, \qquad \sum_N\Pi_N = I.

A vector can have components in several sectors even though the sectors are mutually orthogonal.

Because number eigenvalues are integers, the projector onto HN\mathcal H_N has the Fourier representation

ΠN=12π∫02πdθ eiθ(N^−N).\Pi_N = \frac{1}{2\pi} \int_0^{2\pi} d\theta\, e^{i\theta(\widehat N-N)}.

Acting on a number eigenstate ∣M,α⟩\lvert M,\alpha\rangle gives

ΠN∣M,α⟩=δNM∣M,α⟩.\Pi_N \lvert M,\alpha\rangle = \delta_{NM} \lvert M,\alpha\rangle.

This group-averaging formula is useful for number projection of variational states and for deriving sector-resolved partition functions.

Define

U(θ)=e−iθN^.U(\theta) = e^{-i\theta\widehat N}.

Using

[N^,ai]=−ai,[N^,ai†]=ai†,[\widehat N,a_i] = -a_i, \qquad [\widehat N,a_i^\dagger] = a_i^\dagger,

one obtains

U(θ)aiU†(θ)=eiθai,U(θ)ai†U†(θ)=e−iθai†.\begin{aligned} U(\theta)a_iU^\dagger(\theta) &= e^{i\theta}a_i, \\ U(\theta)a_i^\dagger U^\dagger(\theta) &= e^{-i\theta}a_i^\dagger. \end{aligned}

All modes receive the same phase. This is a global internal transformation, not a position-dependent gauge transformation.

The Hamiltonian is invariant under this global U(1)U(1) family when

U(θ)HU†(θ)=HU(\theta)HU^\dagger(\theta) = H

for every θ\theta. Differentiating at θ=0\theta=0 gives

[N^,H]=0.[\widehat N,H] = 0.

Conversely, a vanishing commutator makes HH invariant under the generated unitary group. Thus, under the usual domain assumptions,

global U(1) invariance⟺[H,N^]=0.\text{global }U(1)\text{ invariance} \quad\Longleftrightarrow\quad [H,\widehat N]=0.

On a fixed-NN state, U(θ)U(\theta) produces only the ray phase e−iNθe^{-iN\theta}. Across several number sectors it changes relative phases, and it acts nontrivially on charged operators.

Let

Mp,q=ai1†⋯aip†ajq⋯aj1.M_{p,q} = a_{i_1}^\dagger\cdots a_{i_p}^\dagger a_{j_q}\cdots a_{j_1}.

Repeated use of the commutator product rule gives

[N^,Mp,q]=(p−q)Mp,q.[\widehat N,M_{p,q}] = (p-q)M_{p,q}.

The integer

r=p−qr = p-q

is the number charge of the monomial: it maps the NN sector into the N+rN+r sector.

Equal numbers of creation and annihilation operators imply r=0r=0. This term-by-term test is often faster and less error prone than constructing the full commutator matrix.

Charge counting routes equal creation and annihilation numbers to global U(1) symmetry and fixed-number blocks, while pair terms mix number sectors but preserve parity

The difference r=p−qr=p-q between creation and annihilation counts is the number charge of a monomial. Neutral terms preserve every fixed-NN sector and the full global U(1)U(1) symmetry. Terms with r=±2r=\pm2 mix number sectors but still preserve number parity.

TermNumber chargeConsequence
ai†aja_i^\dagger a_j00transfers one particle; preserves total number
ai†aj†alaka_i^\dagger a_j^\dagger a_l a_k00pair scattering; preserves total number
ai†a_i^\dagger+1+1creates one particle
aia_i−1-1annihilates one particle
ai†aj†a_i^\dagger a_j^\dagger+2+2creates a pair
ajaia_j a_i−2-2annihilates a pair
ai†ajaka_i^\dagger a_j a_k−1-1one creation and two annihilations

A Hermitian number-breaking Hamiltonian contains charge-changing terms in conjugate pairs. Hermiticity does not restore number conservation.

Many conserved quantities are weighted mode occupations:

Q^=∑iqini.\widehat Q = \sum_i q_i n_i.

Then

[Q^,ai†]=qiai†,[Q^,ai]=−qiai.[\widehat Q,a_i^\dagger] = q_i a_i^\dagger, \qquad [\widehat Q,a_i] = -q_i a_i.

For a monomial,

[Q^,Mp,q]=(∑α=1pqiα−∑β=1qqjβ)Mp,q.\begin{aligned} [\widehat Q,M_{p,q}] ={}& \left( \sum_{\alpha=1}^{p}q_{i_\alpha} - \sum_{\beta=1}^{q}q_{j_\beta} \right) M_{p,q}. \end{aligned}

This tests electric charge, species number, spin projection in an appropriate basis, or any Abelian additive quantum number. A process can violate the unweighted excitation count while conserving a physically weighted charge.

A standard Hamiltonian with one- and two-body terms is

H=∑i,jhijai†aj+12∑i,j,k,lVij;klai†aj†alak.\begin{aligned} H ={}& \sum_{i,j} h_{ij}a_i^\dagger a_j \\ &+ \frac12 \sum_{i,j,k,l} V_{ij;kl} a_i^\dagger a_j^\dagger a_l a_k. \end{aligned}

Every monomial is neutral, so

[H,N^]=0.[H,\widehat N] = 0.

The Hamiltonian may strongly mix mode occupations and generate correlations. Conservation of total number does not imply conservation of each nin_i or independent-particle dynamics.

Explicit time dependence of H(t)H(t) does not by itself break particle-number conservation. If

[H(t),N^]=0[H(t),\widehat N] = 0

for every time, then

dN^Hdt=iℏ[HH(t),N^H]=0.\frac{d\widehat N_H}{dt} = \frac{i}{\hbar} [H_H(t),\widehat N_H] = 0.

A time-dependent hopping amplitude, trap, or interaction can preserve number. A coherent source or pair drive can break it. Energy conservation and number conservation are separate questions.

Insert fixed-number projectors around the commutator:

ΠN[N^,H]ΠM=(N−M)ΠNHΠM.\Pi_N [\widehat N,H] \Pi_M = (N-M) \Pi_N H\Pi_M.

If [N^,H]=0[\widehat N,H]=0, then

ΠNHΠM=0N≠M.\Pi_N H\Pi_M = 0 \qquad N\neq M.

Therefore

H=⨁NHN,HN=ΠNHΠN.H = \bigoplus_N H_N, \qquad H_N = \Pi_N H\Pi_N.

Time evolution is block diagonal as well:

U(t,t0)=⨁NUN(t,t0).U(t,t_0) = \bigoplus_N U_N(t,t_0).

This is the algebraic reason fixed-number exact diagonalization is valid for a number-conserving Hamiltonian.

For a state ρ\rho, define

PN=Tr⁡(ρΠN).P_N = \operatorname{Tr}(\rho\Pi_N).

When [H,N^]=0[H,\widehat N]=0, every PNP_N is constant under closed-system time evolution. Consequently, all moments

⟨N^m⟩=∑NNmPN\langle\widehat N^m\rangle = \sum_N N^m P_N

are conserved.

This is stronger than conservation of the mean alone. A state can have constant ⟨N^⟩\langle\widehat N\rangle while its full number distribution changes under a specially engineered nonconserving process. Exact U(1)U(1) symmetry freezes the entire distribution.

A number-conserving Hamiltonian does not force every state to have definite number. An initial state may contain several sectors:

∣Ψ(0)⟩=∑NcN∣ψN⟩.\lvert\Psi(0)\rangle = \sum_N c_N\lvert\psi_N\rangle.

Each sector evolves independently:

∣Ψ(t)⟩=∑NcNUN(t)∣ψN⟩.\lvert\Psi(t)\rangle = \sum_N c_N U_N(t)\lvert\psi_N\rangle.

The probabilities ∣cN∣2|c_N|^2 are fixed, while relative sector phases and the internal states can evolve. Thus:

  • conservation does not imply a sharp value;
  • a sharp value does not by itself imply a superselection rule;
  • an indefinite-number state does not by itself imply number-breaking dynamics.

Suppose an operator OrO_r satisfies

[N^,Or]=rOr.[\widehat N,O_r] = rO_r.

Between number eigenstates,

⟨N′,α′∣[N^,Or]∣N,α⟩=(N′−N)×⟨N′,α′∣Or∣N,α⟩.\begin{aligned} \langle N',\alpha'\vert [\widehat N,O_r] \vert N,\alpha\rangle ={}& (N'-N) \\ &\times \langle N',\alpha'\vert O_r \vert N,\alpha\rangle. \end{aligned}

Therefore a nonzero matrix element requires

N′=N+r.N' = N+r.

In a fixed-number state, the expectation of every charged operator vanishes:

⟨Or⟩=0r≠0.\langle O_r\rangle = 0 \qquad r\neq0.

This is why ⟨ai⟩\langle a_i\rangle and ⟨aiaj⟩\langle a_i a_j\rangle vanish in an exact number eigenstate even when one-body or pair coherence is physically strong.

Let

bα=∑iUiα∗aib_\alpha = \sum_i U_{i\alpha}^*a_i

for unitary UU. Then

∑αbα†bα=∑i,j,αUiαUjα∗ai†aj=∑iai†ai.\begin{aligned} \sum_\alpha b_\alpha^\dagger b_\alpha ={}& \sum_{i,j,\alpha} U_{i\alpha} U_{j\alpha}^* a_i^\dagger a_j \\ ={}& \sum_i a_i^\dagger a_i. \end{aligned}

Individual occupations transform into off-diagonal bilinears, but their complete sum remains N^\widehat N. A truncated or nonunitary change of one-particle space need not preserve this identity without a carefully transformed operator.

For several species or internal components,

N^s=∑iais†ais,N^=∑sN^s.\widehat N_s = \sum_i a_{is}^\dagger a_{is}, \qquad \widehat N = \sum_s \widehat N_s.

A Hamiltonian can conserve more than one number. Spin-conserving Hubbard hopping preserves N↑N_\uparrow and N↓N_\downarrow separately. A spin-flip term such as

Hsf=Ω∑i(ci↑†ci↓+ci↓†ci↑)H_{\mathrm{sf}} = \Omega \sum_i \left( c_{i\uparrow}^\dagger c_{i\downarrow} + c_{i\downarrow}^\dagger c_{i\uparrow} \right)

preserves N↑+N↓N_\uparrow+N_\downarrow but not the two component numbers separately.

The physically conserved combinations follow from all conversion terms, not from the labels chosen before writing the Hamiltonian.

Quasiparticle Number Is a Different Charge

Section titled “Quasiparticle Number Is a Different Charge”

Phonons, magnons, Bogoliubov modes, polaritons, and other quasiparticles have their own occupation operators. Their total occupation need not equal a microscopic particle number and is often not conserved.

A Hamiltonian diagonal in quasiparticle operators,

Hqp=E0+∑αEαβα†βα,H_{\mathrm{qp}} = E_0 + \sum_\alpha E_\alpha \beta_\alpha^\dagger\beta_\alpha,

conserves ∑αβα†βα\sum_\alpha\beta_\alpha^\dagger\beta_\alpha only within that quadratic effective model. Interactions among quasiparticles can create and annihilate them while preserving an underlying atomic, electric, or spin charge.

Always name the counted degrees of freedom. Bogoliubov Quasiparticles works this distinction through explicitly for bosonic and fermionic transformations, including expected microscopic number, exact parity, and number-conserving formulations.

For a spatial region Ω\Omega,

N^Ω=∫Ωddr n(r).\widehat N_\Omega = \int_\Omega d^dr\, n(\mathbf r).

Even when total number is conserved, N^Ω\widehat N_\Omega generally is not. Particles can cross the boundary:

dN^Ωdt=−∫∂ΩdS⋅jN+S^Ω.\frac{d\widehat N_\Omega}{dt} = - \int_{\partial\Omega} d\mathbf S\cdot \mathbf j_N + \widehat S_\Omega.

The source S^Ω\widehat S_\Omega vanishes for a locally number-conserving closed model. Taking Ω\Omega to be the complete closed system removes boundary flux and recovers global conservation.

The global commutator [H,N^]=0[H,\widehat N]=0 does not by itself identify a unique local current. Locality and the density decomposition are additional inputs.

Chemical Potential and the Grand Hamiltonian

Section titled “Chemical Potential and the Grand Hamiltonian”

When particle number is conserved, define

K=H−μN^.K = H-\mu\widehat N.

Then

[K,N^]=0.[K,\widehat N] = 0.

On one fixed-NN sector,

KN=HN−μNIN.K_N = H_N-\mu N I_N.

The chemical-potential term is a constant energy shift inside that sector. It does not change fixed-NN eigenvectors or closed-system expectation values. Its thermodynamic role is to change the relative weights assigned to different number sectors.

An equilibrium chemical potential normally couples to a conserved charge. If the proposed charge is not conserved by the microscopic isolated dynamics, the interpretation of its multiplier requires additional justification.

Grand-Canonical Mixtures Are Not Coherent Superpositions

Section titled “Grand-Canonical Mixtures Are Not Coherent Superpositions”

For [H,N^]=0[H,\widehat N]=0, the grand-canonical density operator is block diagonal:

ρβ,μ=⨁NPNρN,β.\rho_{\beta,\mu} = \bigoplus_N P_N\rho_{N,\beta}.

It is a statistical mixture over number sectors, not a coherent vector with an observable phase between sectors. Number fluctuations in this ensemble therefore do not by themselves violate a particle-number superselection restriction.

Three statements must remain distinct:

  1. [H,N^]=0[H,\widehat N]=0: the chosen closed-system dynamics preserves number sectors;
  2. ρ=∑NΠNρΠN\rho=\sum_N\Pi_N\rho\Pi_N: the state has no inter-sector coherences;
  3. [A,N^]=0[A,\widehat N]=0 for every allowed observable AA: accessible operations cannot compare number-sector phases.

Only the third is an operational superselection restriction. A direct-sum decomposition or one commuting Hamiltonian is not enough to establish it. Reference frames, reservoirs, and enlarged descriptions can change which operations are available.

Define fermion parity spectrally by

PF=(−1)N^=eiπN^.P_F = (-1)^{\widehat N} = e^{i\pi\widehat N}.

It acts as

PFaiPF†=−ai,PFai†PF†=−ai†.P_Fa_iP_F^\dagger = -a_i, \qquad P_Fa_i^\dagger P_F^\dagger = -a_i^\dagger.

An operator with even total ladder degree preserves fermion parity. In particular, pair creation and annihilation change NN by two, so they break continuous U(1)U(1) number symmetry but preserve the discrete Z2\mathbb Z_2 parity symmetry.

Bosonic models can also possess number parity when every process changes NN by an even integer. That model symmetry should not be conflated with the broader role of fermion parity in fermionic observable algebras.

Define the pair operators

bk†=ck↑†c−k↓†,bk=c−k↓ck↑.b_{\mathbf k}^\dagger = c_{\mathbf k\uparrow}^\dagger c_{-\mathbf k\downarrow}^\dagger, \qquad b_{\mathbf k} = c_{-\mathbf k\downarrow} c_{\mathbf k\uparrow}.

A reduced BCS grand Hamiltonian is

Kred=∑k,σξkckσ†ckσ−g∑k,k′bk†bk′,\begin{aligned} K_{\mathrm{red}} ={}& \sum_{\mathbf k,\sigma} \xi_{\mathbf k} c_{\mathbf k\sigma}^\dagger c_{\mathbf k\sigma} \\ &- g \sum_{\mathbf k,\mathbf k'} b_{\mathbf k}^\dagger b_{\mathbf k'}, \end{aligned}

where g>0g>0 denotes attraction in this convention. Since

[N^,bk†]=2bk†,[N^,bk]=−2bk,[\widehat N,b_{\mathbf k}^\dagger] = 2b_{\mathbf k}^\dagger, \qquad [\widehat N,b_{\mathbf k}] = -2b_{\mathbf k},

the pair-scattering product is neutral:

[N^,bk†bk′]=0.[\widehat N,b_{\mathbf k}^\dagger b_{\mathbf k'}] = 0.

Therefore

[Kred,N^]=0.[K_{\mathrm{red}},\widehat N] = 0.

The exact reduced pairing Hamiltonian scatters pairs; it does not create particles from nothing.

BCS Mean-Field Theory owns the full reduced-model, Cooper-instability, gap-equation, and quasiparticle derivation. The comparison here remains focused on number charge.

Introduce

Δ=g∑k⟨bk⟩.\Delta = g \sum_{\mathbf k} \langle b_{\mathbf k}\rangle.

The usual unprojected mean-field grand Hamiltonian has the form

KMF=∑k,σξkckσ†ckσ−∑k(Δbk†+Δ∗bk)+∣Δ∣2g.\begin{aligned} K_{\mathrm{MF}} ={}& \sum_{\mathbf k,\sigma} \xi_{\mathbf k} c_{\mathbf k\sigma}^\dagger c_{\mathbf k\sigma} \\ &- \sum_{\mathbf k} \left( \Delta b_{\mathbf k}^\dagger + \Delta^*b_{\mathbf k} \right) + \frac{|\Delta|^2}{g}. \end{aligned}

Holding the chosen c-number Δ\Delta fixed,

[N^,KMF]=−2∑kΔbk†+2∑kΔ∗bk,\begin{aligned} [\widehat N,K_{\mathrm{MF}}] ={}& -2\sum_{\mathbf k} \Delta b_{\mathbf k}^\dagger \\ &+ 2\sum_{\mathbf k} \Delta^*b_{\mathbf k}, \end{aligned}

which is generally nonzero. The approximation mixes sectors whose particle numbers differ by two while preserving fermion parity.

This does not mean the underlying reduced BCS model violates particle-number conservation. The number breaking belongs to the symmetry-breaking mean-field representation. Reduced BCS Model develops the exact fixed-number sectors, blocking, and Richardson solution.

The thermodynamic saddle, coherence factors, and number-projected interpretation are developed in BCS Mean-Field Theory.

Under the convention U(θ)=e−iθN^U(\theta)=e^{-i\theta\widehat N},

bk⟼e2iθbk,Δ⟼e2iθΔ.b_{\mathbf k} \longmapsto e^{2i\theta}b_{\mathbf k}, \qquad \Delta \longmapsto e^{2i\theta}\Delta.

The family of mean-field Hamiltonians is covariant if Δ\Delta transforms with the anomalous average. Choosing one fixed phase for Δ\Delta selects a representative from that family.

In a finite exact number eigenstate,

⟨bk⟩=0\langle b_{\mathbf k}\rangle = 0

by the number selection rule. Pairing can instead appear in neutral quantities such as ⟨bk†bk′⟩\langle b_{\mathbf k}^\dagger b_{\mathbf k'}\rangle. A source, phase reference, thermodynamic-limit construction, or number-projected state is needed to relate the exact and symmetry-breaking languages carefully.

Explicit, Spontaneous, and Effective Breaking

Section titled “Explicit, Spontaneous, and Effective Breaking”

These phrases describe different physics.

The Hamiltonian itself does not commute with N^\widehat N. A coherent source is

Hsrc=∑i(fiai†+fi∗ai).H_{\mathrm{src}} = \sum_i \left( f_i a_i^\dagger + f_i^*a_i \right).

It changes subsystem number by one and fixes a phase reference.

The microscopic Hamiltonian preserves U(1)U(1), but a thermodynamic-limit state or variational ansatz selects a phase. Finite-size exact eigenstates can remain number eigenstates even when neutral correlation functions reveal incipient order.

The modeled subsystem exchanges particles with an omitted condensate, reservoir, drive, or reaction channel. The subsystem Hamiltonian or master equation need not conserve its number even when an enlarged closed description conserves a total charge.

Using the word “broken” without identifying which of these mechanisms is intended obscures the approximation.

Bosonic effective models commonly contain a linear source or a pairing drive:

Hpair=12∑i,j(Δijai†aj†+Δij∗ajai).H_{\mathrm{pair}} = \frac12 \sum_{i,j} \left( \Delta_{ij}a_i^\dagger a_j^\dagger + \Delta_{ij}^*a_j a_i \right).

The source changes NN by one. The pair drive changes NN by two and can preserve bosonic number parity. Stability of a bosonic pairing Hamiltonian is a separate condition; a formal parity symmetry does not guarantee a spectrum bounded below.

A mean-field replacement ai→ϕia_i\to\phi_i is an approximation involving a phase reference or symmetry-breaking limit. It is not an identity in a finite fixed-number Hilbert space.

An expectation such as

⟨aiaj⟩\langle a_i a_j\rangle

has number charge −2-2 in the commutator convention:

[N^,aiaj]=−2aiaj.[\widehat N,a_i a_j] = -2a_i a_j.

It vanishes in a number eigenstate and in any U(1)U(1)-invariant density operator. A nonzero anomalous expectation therefore presupposes a number-breaking state description, a phase reference, or an enlarged relational interpretation.

Neutral pair correlations such as

⟨ai†aj†alak⟩\langle a_i^\dagger a_j^\dagger a_l a_k \rangle

can be nonzero without breaking number symmetry.

For a Lindblad–GKSL equation

ρ˙=−iℏ[H,ρ]+∑μκμD[Lμ]ρ,\dot\rho = -\frac{i}{\hbar}[H,\rho] + \sum_\mu \kappa_\mu \mathcal D[L_\mu]\rho,

with

D[L]ρ=LρL†−12{L†L,ρ},\mathcal D[L]\rho = L\rho L^\dagger - \frac12 \{L^\dagger L,\rho\},

the number expectation obeys

ddt⟨N^⟩=iℏ⟨[H,N^]⟩+∑μκμ⟨Lμ†N^Lμ−12{Lμ†Lμ,N^}⟩.\begin{aligned} \frac{d}{dt} \langle\widehat N\rangle ={}& \frac{i}{\hbar} \langle[H,\widehat N]\rangle \\ &+ \sum_\mu \kappa_\mu \left\langle L_\mu^\dagger\widehat N L_\mu - \frac12 \{L_\mu^\dagger L_\mu,\widehat N\} \right\rangle. \end{aligned}

If

[N^,Lμ]=−rμLμ[\widehat N,L_\mu] = -r_\mu L_\mu

and Lμ†LμL_\mu^\dagger L_\mu commutes with N^\widehat N, that channel contributes

−rμκμ⟨Lμ†Lμ⟩.-r_\mu\kappa_\mu \langle L_\mu^\dagger L_\mu\rangle.

Single-particle loss has rμ=1r_\mu=1, pair loss has rμ=2r_\mu=2, and number dephasing with Lμ=niL_\mu=n_i has rμ=0r_\mu=0.

For a finite matrix representation, useful diagnostics are:

  1. compute C=[H,N^]C=[H,\widehat N] and compare ∥C∥\lVert C\rVert with a scale such as ∥H∥∥N^∥\lVert H\rVert\lVert\widehat N\rVert;
  2. inspect ΠNHΠM\Pi_NH\Pi_M for N≠MN\neq M;
  3. propagate states from one sector and monitor leakage;
  4. monitor the full distribution PNP_N, not only ⟨N^⟩\langle\widehat N\rangle;
  5. test every weighted charge claimed by the model;
  6. distinguish physical symmetry breaking from truncation or floating-point residuals;
  7. verify that a basis transformation also transforms the charge operator;
  8. test exact and mean-field Hamiltonians separately.

A numerical commutator should be judged relative to matrix scales and precision. Reporting only an absolute residual can be misleading.

When [H,N^]=0[H,\widehat N]=0, constructing only the required NN sector reduces memory and runtime. For MM modes,

dim⁡HN(F)=(MN)\dim\mathcal H_N^{(F)} = \binom MN

for fermions, while for bosons

dim⁡HN(B)=(N+M−1N).\dim\mathcal H_N^{(B)} = \binom{N+M-1}{N}.

Additional commuting charges can split the sector further. One must not impose a symmetry block that the actual Hamiltonian breaks; doing so silently removes physical matrix elements.

  • Calling every mode occupation a conserved quantity.
  • Assuming a time-dependent Hamiltonian necessarily breaks particle-number conservation.
  • Checking only ⟨N^⟩\langle\widehat N\rangle instead of [H,N^][H,\widehat N] or the full distribution.
  • Confusing a fixed-number state with a number-conserving Hamiltonian.
  • Treating number conservation as an automatic superselection rule.
  • Forgetting that N^\widehat N is basis independent only under a complete unitary mode transformation.
  • Claiming that exact reduced BCS pair scattering violates number conservation.
  • Claiming that BCS mean field conserves NN because it preserves parity.
  • Treating a nonzero anomalous average as compatible with an exact finite number eigenstate without a reference or projection argument.
  • Confusing quasiparticle number with microscopic particle number.
  • Adding −μN^-\mu\widehat N to a fixed-NN problem and expecting eigenvectors to change.
  • Inferring a local current from the global commutator alone.
  • Interpreting subsystem loss as a fundamental violation when an omitted reservoir carries the compensating charge.
  • Enforcing a symmetry sector numerically after adding a term that breaks it.
QuestionDiagnostic
Does a monomial conserve total number?count r=p−qr=p-q
Does the Hamiltonian have global U(1)U(1) symmetry?verify [H,N^]=0[H,\widehat N]=0
Which sectors can OrO_r connect?only N→N+rN\to N+r
Is the Hamiltonian block diagonal?check ΠNHΠM=0\Pi_NH\Pi_M=0 for N≠MN\neq M
Does pair creation preserve anything?it breaks U(1)U(1) but preserves number parity
Does a chemical potential alter fixed-NN eigenvectors?no; −μN-\mu N is constant in that sector
Does a grand-canonical state require number coherence?no; it is block diagonal when [H,N^]=0[H,\widehat N]=0
Does conservation imply superselection?no; allowed operations must also be restricted
Is local number conserved?derive its continuity equation and boundary flux
Does an open-system jump remove rr particles?check [N^,L]=−rL[\widehat N,L]=-rL
  • Total number is dΓ(IH1)d\Gamma(I_{\mathcal H_1}) and is invariant under complete one-particle basis rotations.
  • N^\widehat N generates a global U(1)U(1) transformation of the ladder operators.
  • A monomial with pp creations and qq annihilations carries number charge p−qp-q.
  • [H,N^]=0[H,\widehat N]=0 makes the Hamiltonian and time evolution block diagonal in fixed-NN sectors.
  • Number conservation preserves the full sector probability distribution, not merely its mean.
  • Charged operators obey N→N+rN\to N+r selection rules and have zero expectation in fixed-number states.
  • Separate species numbers survive only when conversion terms preserve them individually.
  • Total conservation does not imply local conservation without a continuity equation.
  • Exact reduced BCS pair scattering conserves NN; unprojected BCS mean field breaks U(1)U(1) but preserves fermion parity.
  • Conservation, superselection, explicit breaking, spontaneous breaking, and open-system exchange are distinct statements.

Symmetry Sectors in Many-Body Numerics develops the computational use of fixed-NN and number-parity blocks, including dimension, closure, and sector-changing-observable checks.

Prove that a normally ordered monomial Mp,qM_{p,q} satisfies

[N^,Mp,q]=(p−q)Mp,q.[\widehat N,M_{p,q}] = (p-q)M_{p,q}.
Solution

Use

[N^,ai†]=ai†,[N^,ai]=−ai[\widehat N,a_i^\dagger] = a_i^\dagger, \qquad [\widehat N,a_i] = -a_i

and the product rule

[A,BC]=[A,B]C+B[A,C].[A,BC] = [A,B]C+B[A,C].

Each of the pp creation operators contributes +Mp,q+M_{p,q} to the commutator, while each of the qq annihilation operators contributes −Mp,q-M_{p,q}. Summing the contributions gives

[N^,Mp,q]=(p−q)Mp,q.[\widehat N,M_{p,q}] = (p-q)M_{p,q}.

The result is the same for bosons and fermions because it uses ordinary commutators with the even operator N^\widehat N.

Let [N^,Or]=rOr[\widehat N,O_r]=rO_r. Show that

⟨N′,α′∣Or∣N,α⟩\langle N',\alpha'\vert O_r \vert N,\alpha\rangle

vanishes unless N′=N+rN'=N+r.

Solution

Take the matrix element of the commutator:

⟨N′,α′∣[N^,Or]∣N,α⟩=(N′−N)×⟨N′,α′∣Or∣N,α⟩.\begin{aligned} \langle N',\alpha'\vert [\widehat N,O_r] \vert N,\alpha\rangle ={}& (N'-N) \\ &\times \langle N',\alpha'\vert O_r \vert N,\alpha\rangle. \end{aligned}

The defining relation gives the same left side as

r⟨N′,α′∣Or∣N,α⟩.r \langle N',\alpha'\vert O_r \vert N,\alpha\rangle.

Therefore

(N′−N−r)⟨N′,α′∣Or∣N,α⟩=0.(N'-N-r) \langle N',\alpha'\vert O_r \vert N,\alpha\rangle = 0.

A nonzero matrix element requires N′=N+rN'=N+r.

For

bα=∑iUiα∗ai,b_\alpha = \sum_i U_{i\alpha}^*a_i,

with unitary UU, prove

∑αbα†bα=∑iai†ai.\sum_\alpha b_\alpha^\dagger b_\alpha = \sum_i a_i^\dagger a_i.
Solution

Substitute the mode transformation:

∑αbα†bα=∑i,j,αUiαUjα∗ai†aj=∑i,jδijai†aj=∑iai†ai.\begin{aligned} \sum_\alpha b_\alpha^\dagger b_\alpha ={}& \sum_{i,j,\alpha} U_{i\alpha} U_{j\alpha}^* a_i^\dagger a_j \\ ={}& \sum_{i,j} \delta_{ij} a_i^\dagger a_j \\ ={}& \sum_i a_i^\dagger a_i. \end{aligned}

Unitarity supplied

∑αUiαUjα∗=δij.\sum_\alpha U_{i\alpha}U_{j\alpha}^* = \delta_{ij}.

The total is invariant, although each new bα†bαb_\alpha^\dagger b_\alpha is a linear combination of old diagonal and off-diagonal bilinears.

Exercise 4: Number blocks and sector probabilities

Section titled “Exercise 4: Number blocks and sector probabilities”

Assume [H,N^]=0[H,\widehat N]=0.

  1. Show that ΠNHΠM=0\Pi_NH\Pi_M=0 for N≠MN\neq M.
  2. Show that PN(t)=Tr⁡[ρ(t)ΠN]P_N(t)=\operatorname{Tr}[\rho(t)\Pi_N] is constant under unitary evolution.
Solution

For the first part,

ΠN[N^,H]ΠM=(N−M)ΠNHΠM.\Pi_N [\widehat N,H] \Pi_M = (N-M) \Pi_NH\Pi_M.

The left side vanishes. If N≠MN\neq M, division by N−MN-M gives

ΠNHΠM=0.\Pi_NH\Pi_M = 0.

Thus HH commutes with every spectral projector ΠN\Pi_N. For the second part,

dPNdt=−iℏTr⁡([H,ρ]ΠN)=−iℏTr⁡(ρ[ΠN,H])=0.\begin{aligned} \frac{dP_N}{dt} &= -\frac{i}{\hbar} \operatorname{Tr} \left( [H,\rho]\Pi_N \right) \\ &= -\frac{i}{\hbar} \operatorname{Tr} \left( \rho[\Pi_N,H] \right) = 0. \end{aligned}

Every sector probability is conserved.

Exercise 5: Conversion between two species

Section titled “Exercise 5: Conversion between two species”

Let

Hg=g(a†b+b†a).H_g = g \left( a^\dagger b + b^\dagger a \right).

Determine which of Na=a†aN_a=a^\dagger a, Nb=b†bN_b=b^\dagger b, and Ntot=Na+NbN_{\mathrm{tot}}=N_a+N_b are conserved.

Solution

The commutators are

[Na,Hg]=g(a†b−b†a),[Nb,Hg]=−g(a†b−b†a).\begin{aligned} [N_a,H_g] &= g \left( a^\dagger b - b^\dagger a \right), \\ [N_b,H_g] &= -g \left( a^\dagger b - b^\dagger a \right). \end{aligned}

Neither component number is conserved. Adding them gives

[Ntot,Hg]=0.[N_{\mathrm{tot}},H_g] = 0.

The coupling converts one species into the other while preserving the total occupation.

Exercise 6: Exact and mean-field BCS number symmetry

Section titled “Exercise 6: Exact and mean-field BCS number symmetry”

Let [N^,bk†]=2bk†[\widehat N,b_{\mathbf k}^\dagger]=2b_{\mathbf k}^\dagger and [N^,bk]=−2bk[\widehat N,b_{\mathbf k}]=-2b_{\mathbf k}.

  1. Show that bk†bk′b_{\mathbf k}^\dagger b_{\mathbf k'} conserves number.
  2. Show that Δbk†+Δ∗bk\Delta b_{\mathbf k}^\dagger+\Delta^*b_{\mathbf k} does not conserve number for fixed nonzero Δ\Delta.
  3. State which discrete symmetry remains.
Solution

For pair scattering,

[N^,bk†bk′]=2bk†bk′−2bk†bk′=0.\begin{aligned} [\widehat N, b_{\mathbf k}^\dagger b_{\mathbf k'}] ={}& 2b_{\mathbf k}^\dagger b_{\mathbf k'} - 2b_{\mathbf k}^\dagger b_{\mathbf k'} \\ ={}&0. \end{aligned}

For the mean-field pair source,

[N^,Δbk†+Δ∗bk]=2Δbk†−2Δ∗bk,\begin{aligned} [\widehat N, \Delta b_{\mathbf k}^\dagger + \Delta^*b_{\mathbf k}] ={}& 2\Delta b_{\mathbf k}^\dagger \\ &- 2\Delta^*b_{\mathbf k}, \end{aligned}

which is generally nonzero. Both terms change particle number by an even integer, so fermion parity (−1)N^(-1)^{\widehat N} remains conserved.

Exercise 7: Chemical potential in a fixed-number sector

Section titled “Exercise 7: Chemical potential in a fixed-number sector”

Let K=H−μN^K=H-\mu\widehat N with [H,N^]=0[H,\widehat N]=0. Show that on HN\mathcal H_N, evolution under KK differs from evolution under HH only by a global phase.

Solution

On the fixed-NN sector,

KN=HN−μNIN.K_N = H_N-\mu N I_N.

Because the second term is proportional to the identity,

e−iKNt/ℏ=e−i(HN−μNIN)t/ℏ=eiμNt/ℏe−iHNt/ℏ.\begin{aligned} e^{-iK_Nt/\hbar} &= e^{-i(H_N-\mu NI_N)t/\hbar} \\ &= e^{i\mu Nt/\hbar} e^{-iH_Nt/\hbar}. \end{aligned}

The prefactor is a global phase on HN\mathcal H_N, so every expectation value within that sector is unchanged. The chemical potential matters when comparing or statistically weighting different NN sectors.

For one bosonic mode with number-conserving HH and master equation

ρ˙=−iℏ[H,ρ]+κD[a]ρ,\dot\rho = -\frac{i}{\hbar}[H,\rho] + \kappa\mathcal D[a]\rho,

derive the equation for ⟨n⟩\langle n\rangle.

Solution

The Hamiltonian contribution vanishes because [H,n]=0[H,n]=0. For the dissipator, use

[n,a]=−a,[n,a] = -a,

so the jump removes one quantum. The adjoint dissipator gives

ddt⟨n⟩=κ⟨a†na−12{a†a,n}⟩=−κ⟨a†a⟩.\begin{aligned} \frac{d}{dt}\langle n\rangle ={}& \kappa \left\langle a^\dagger n a - \frac12 \{a^\dagger a,n\} \right\rangle \\ ={}& -\kappa \langle a^\dagger a\rangle. \end{aligned}

Therefore

ddt⟨n⟩=−κ⟨n⟩,\frac{d}{dt} \langle n\rangle = -\kappa\langle n\rangle,

with solution ⟨n(t)⟩=e−κt⟨n(0)⟩\langle n(t)\rangle=e^{-\kappa t}\langle n(0)\rangle. Number is not conserved in the subsystem because the environment receives the lost quanta.

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