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Derivation

Conserved Charge as Symmetry Generator

D-380 Home PU-402 Threads symmetry · fields Depends on Noether's First Theorem, Canonical Quantization of a Field
Statement

In a canonically quantized field theory, the conserved Noether charge \( Q=\int d^3x\, j^0 \) associated with a continuous internal symmetry acts on the fields as the generator of that symmetry: for an infinitesimal transformation \( \varphi\to\varphi+\delta\varphi \) (with the parameter \( \alpha \) scaled out, so \( \delta\varphi \) is the change per unit \( \alpha \)), the equal-time commutator satisfies \( [\,Q,\varphi(x)\,]=-\,i\,\delta\varphi(x) \). Equivalently, the finite unitary \( U(\alpha)=e^{\,i\alpha Q} \) implements the symmetry by conjugation, \( U\,\varphi\,U^{-1}=\varphi+\alpha\,\delta\varphi+\mathcal{O}(\alpha^2) \).

Why it matters

Noether's first theorem hands us a conserved number \( Q \) whenever the action is invariant, but says nothing about what \( Q \) does to states. Quantization turns \( Q \) into an operator, and this result identifies that operator with the geometric object it came from: \( Q \) is not merely conserved, it is the infinitesimal generator that rotates, shifts, or phases the fields. This is what makes "charge" and "symmetry" two views of one structure.

The relation underwrites almost everything downstream: Ward–Takahashi identities, the classification of states by charge sectors, the spontaneous-breaking criterion \( Q|0\rangle\neq 0 \), and the very statement that gauge redundancies are generated by (would-be) charges. It is the bridge from the classical Noether current to the quantum algebra of observables.

Assumptions
The symmetry is a continuous internal symmetry leaving the Lagrangian density strictly invariant, \( \delta\mathcal{L}=0 \).If \( \delta\mathcal{L}=\partial_\mu K^\mu\neq 0 \) the current acquires an extra piece \( -K^\mu \); the charge still generates the transformation but \( j^0 \) is no longer simply \( \pi\,\delta\varphi \), so every step below must carry the \( K^0 \) term.
The field variation \( \delta\varphi \) is an ultralocal function of the canonical coordinates \( \varphi \) alone (not of \( \pi \) or its gradients).If \( \delta\varphi \) depends on \( \pi \), it fails to commute with \( \pi(x) \) inside the integral and operator-ordering terms appear, spoiling the clean pull-through in the derivation.
Canonical quantization holds: equal-time commutators \( [\varphi(\mathbf{x}),\pi(\mathbf{y})]=i\,\delta^3(\mathbf{x}-\mathbf{y}) \) are well-defined after normal ordering / regularization.Without a well-defined equal-time algebra (e.g. in strongly-coupled or non-Lagrangian theories) the Dirac-delta manipulation is formal only and the identity must be re-derived from the operator symmetry action directly.
The charge is finite and time-independent, with fields decaying fast enough at spatial infinity that surface terms vanish.If \( Q \) diverges or surface contributions survive, \( Q \) is not a good operator on the Hilbert space (as in spontaneously broken symmetries), and \( [\,Q,\varphi\,] \) must be read as a formal/local statement.
Derivation
1
\[ Q=\int d^3x\, j^0(\mathbf{x},t),\qquad j^0=\frac{\partial\mathcal{L}}{\partial(\partial_0\varphi)}\,\delta\varphi=\pi(\mathbf{x})\,\delta\varphi(\mathbf{x}) \]
Import the Noether charge from the first theorem; for \( \delta\mathcal{L}=0 \) the time component of the current is the conjugate momentum \( \pi=\partial\mathcal{L}/\partial\dot\varphi \) times the field variation. A
2
\[ [\,\varphi(\mathbf{x},t),\pi(\mathbf{y},t)\,]=i\,\delta^3(\mathbf{x}-\mathbf{y}),\qquad [\,\varphi,\varphi\,]=[\,\pi,\pi\,]=0 \]
Import the equal-time canonical commutation relations from field quantization. All commutators below are taken at a common time \( t \). A
3
\[ [\,Q,\varphi(\mathbf{y},t)\,]=\int d^3x\,\big[\,\pi(\mathbf{x})\,\delta\varphi(\mathbf{x})\,,\,\varphi(\mathbf{y})\,\big] \]
Substitute \( Q \) and use linearity of the commutator to pull the spatial integral outside. A
4
\[ \big[\,\pi(\mathbf{x})\,\delta\varphi(\mathbf{x})\,,\,\varphi(\mathbf{y})\,\big]=\big[\,\pi(\mathbf{x}),\varphi(\mathbf{y})\,\big]\,\delta\varphi(\mathbf{x})+\pi(\mathbf{x})\,\big[\,\delta\varphi(\mathbf{x}),\varphi(\mathbf{y})\,\big] \]
Apply the Leibniz (derivation) rule \( [AB,C]=[A,C]B+A[B,C] \) for commutators. B
5
\[ \big[\,\delta\varphi(\mathbf{x}),\varphi(\mathbf{y})\,\big]=0\quad\Longrightarrow\quad \big[\,\pi(\mathbf{x})\,\delta\varphi(\mathbf{x}),\varphi(\mathbf{y})\,\big]=\big[\,\pi(\mathbf{x}),\varphi(\mathbf{y})\,\big]\,\delta\varphi(\mathbf{x}) \]
By the ultralocality assumption \( \delta\varphi \) is a function of \( \varphi \) only, and \( [\varphi,\varphi]=0 \), so the second term vanishes identically. This is exactly where the "\( \delta\varphi=\delta\varphi(\varphi) \)" hypothesis is used. C
6
\[ \big[\,\pi(\mathbf{x}),\varphi(\mathbf{y})\,\big]=-\,i\,\delta^3(\mathbf{x}-\mathbf{y}) \]
Antisymmetry of the commutator applied to Step 2: \( [\pi,\varphi]=-[\varphi,\pi]=-i\delta^3 \). A
7
\[ [\,Q,\varphi(\mathbf{y})\,]=\int d^3x\,\big(-\,i\,\delta^3(\mathbf{x}-\mathbf{y})\big)\,\delta\varphi(\mathbf{x})=-\,i\,\delta\varphi(\mathbf{y}) \]
Insert Step 6 into Step 3 and integrate the delta function, which sets \( \mathbf{x}=\mathbf{y} \). B
8
\[ U(\alpha)\,\varphi\,U^{-1}(\alpha)=e^{\,i\alpha Q}\,\varphi\,e^{-i\alpha Q}=\varphi+i\alpha[\,Q,\varphi\,]+\mathcal{O}(\alpha^2)=\varphi+\alpha\,\delta\varphi+\mathcal{O}(\alpha^2) \]
Exponentiate: the Hadamard/BCH expansion of conjugation shows that \( Q \) is the generator, since \( i\alpha(-i\,\delta\varphi)=\alpha\,\delta\varphi \) reproduces the classical transformation. Consistency fixes the sign in \( [Q,\varphi]=-i\,\delta\varphi \). C
Result
\[ \boxed{\;[\,Q,\varphi(x)\,]=-\,i\,\delta\varphi(x)\;,\qquad e^{\,i\alpha Q}\,\varphi\,e^{-i\alpha Q}=\varphi+\alpha\,\delta\varphi+\cdots\;} \]

Reading. The conserved charge does not merely commute with the Hamiltonian and sit inert; commuting it against a field returns (up to \( -i \)) exactly the infinitesimal symmetry variation of that field. In operator language \( Q \) is the Lie-algebra generator whose exponential is the unitary symmetry transformation on the Hilbert space. Conservation (\( \dot Q=0 \)) guarantees the same operator generates the symmetry at every instant.

Units check. In natural units (\( \hbar=1 \)) the commutator \( [Q,\varphi] \) carries the dimension of \( \varphi \), and so does \( \delta\varphi \), with \( -i \) dimensionless — balanced. Restoring \( \hbar \): the canonical relation is \( [\varphi,\pi]=i\hbar\,\delta^3 \) and the generator is \( U=e^{\,i\alpha Q/\hbar} \), giving \( [\,Q,\varphi\,]=-\,i\hbar\,\delta\varphi \). Both sides then carry \( [\varphi]\cdot[\hbar] \), consistent since \( Q \) has the dimension of \( \hbar \) per unit \( \alpha \) (an action-like generator).

Limiting cases
  • Free complex scalar, U(1): \( \delta\varphi=-i\varphi \) gives \( [Q,\varphi]=-\varphi \), so \( Q \) counts particle-minus-antiparticle number, \( Q|k\rangle=+|k\rangle \).
  • Spacetime translations: \( \delta\varphi=\partial_\mu\varphi \) promotes \( Q\to P_\mu \) and reproduces \( [P_\mu,\varphi]=-i\partial_\mu\varphi \), the Heisenberg equation for \( \mu=0 \).
  • Free real scalar, no continuous internal symmetry: \( \delta\varphi=0 \), the charge is trivial and \( [Q,\varphi]=0 \) — the theorem is empty but consistent.
  • Classical limit \( \hbar\to0 \): \( \tfrac{1}{i\hbar}[Q,\varphi]\to\{Q,\varphi\}_{\mathrm{PB}}=\delta\varphi \), recovering the Poisson-bracket generator of the classical symmetry.
Breaks when
  • Spontaneous symmetry breaking: when \( Q|0\rangle\neq0 \) the charge operator does not exist on the Hilbert space (its norm diverges, Fabri–Picasso). The local relation \( [Q,\varphi]=-i\delta\varphi \) still holds formally under the integral, but \( Q \) itself is ill-defined and cannot be exponentiated to a unitary — the symmetry is realized non-linearly through Goldstone modes.
  • Anomalous symmetries: a classically conserved current can fail to be conserved after quantization (\( \partial_\mu j^\mu\propto \) anomaly, e.g. the chiral/ABJ anomaly). Then \( Q \) is not time-independent, the naive charge does not generate a good symmetry, and the identity is corrected by anomaly terms.
  • Non-ultralocal or momentum-dependent \( \delta\varphi \): if the variation involves \( \pi \) (e.g. certain dualities or field-dependent gauge transformations), Step 5 fails and extra operator-ordering / Schwinger-term contributions appear.
  • Gauge (large vs. small) transformations: for local gauge symmetry the Gauss-law charge generates the transformation only on physical states; on the full field space the naive \( [Q,\varphi] \) mixes with constraints and gauge-fixing terms.
Failure modes
  • Sign flips: writing \( [Q,\varphi]=+i\delta\varphi \) by forgetting the antisymmetry \( [\pi,\varphi]=-[\varphi,\pi] \) in Step 6. The exponentiation in Step 8 is the sign check.
  • Dropping the \( i \): conflating the quantum commutator with the classical Poisson bracket \( \{Q,\varphi\}=\delta\varphi \); the factor \( i\hbar \) from \( [\;,\;]=i\hbar\{\;,\;\} \) is mandatory.
  • Using \( j^0=\pi\dot\varphi \) instead of \( \pi\,\delta\varphi \): confusing the Hamiltonian density (energy) with the Noether charge density; only \( \delta\varphi \) belongs here.
  • Forgetting the \( K^\mu \) term: for symmetries with \( \delta\mathcal{L}=\partial_\mu K^\mu \) (e.g. translations), omitting \( -K^0 \) gives the wrong charge and a wrong commutator.
  • Equal-time slip: commuting \( Q(t) \) with \( \varphi(t') \) at unequal times and still using the naive delta function; the canonical relation is equal-time only.
  • Ordering \( \pi\,\delta\varphi \) vs. \( \delta\varphi\,\pi \): assuming they are interchangeable when \( \delta\varphi \) is not ultralocal, silently discarding Schwinger terms.
Discussion

The content of this result is that quantization is a homomorphism from the classical symmetry algebra (Poisson brackets of charges) to the operator algebra (commutators). Noether's theorem gives us the map object \( Q \); canonical quantization gives us the bracket; and their marriage says \( \mathrm{ad}_Q\equiv[Q,\cdot] \) is precisely the infinitesimal symmetry action \( -i\,\delta \). Charges of a symmetry group therefore close into the same Lie algebra as the group generators — \( [Q_a,Q_b]=i f_{ab}{}^c Q_c \) — which is why isospin, flavour, and Poincaré charges obey the algebras they do.

Because \( Q \) generates the transformation, its eigenvalues label superselection sectors: states of definite charge, and matrix elements \( \langle\beta|\varphi|\alpha\rangle \) that vanish unless \( q_\beta-q_\alpha \) matches the charge \( \varphi \) carries. This is the operator origin of selection rules. It also makes the invariance of the vacuum, \( Q|0\rangle=0 \), the sharp criterion separating a linearly-realized (Wigner) symmetry from a spontaneously broken (Nambu–Goldstone) one.

At the level of correlation functions the same identity, inserted inside a path integral, becomes the Ward–Takahashi identity: \( \partial_\mu\langle j^\mu(x)\,\varphi(y_1)\cdots\rangle=-i\sum_k\delta(x-y_k)\langle\varphi(y_1)\cdots\delta\varphi(y_k)\cdots\rangle \). The contact terms on the right are nothing but the equal-time \( [Q,\varphi]=-i\delta\varphi \) commutator re-expressed as delta-function singularities when the divergence of the current hits an operator insertion. Anomalies are precisely the statement that this identity picks up an extra, non-classical term from the measure.

Common misconceptions. "Conserved" and "generator" are not the same claim: a quantity can be conserved (commute with \( H \)) yet be a c-number that generates nothing. The theorem's force is that the Noether charge is simultaneously conserved and the generator, and that these two facts have the same origin (invariance of the action). Also, the relation is exact, not a leading-order approximation: it holds to all orders in \( \alpha \) through the finite conjugation \( e^{i\alpha Q}\varphi e^{-i\alpha Q} \).

Worked examples
1
\[ \textbf{U(1) charge of a complex scalar.}\quad \mathcal{L}=\partial_\mu\varphi^\dagger\partial^\mu\varphi-m^2\varphi^\dagger\varphi,\quad \varphi\to e^{-i\alpha}\varphi \]
Internal phase symmetry; identify \( \delta\varphi=-i\varphi \), \( \delta\varphi^\dagger=+i\varphi^\dagger \) (per unit \( \alpha \)). A
2
\[ \pi=\frac{\partial\mathcal{L}}{\partial\dot\varphi}=\dot\varphi^\dagger,\quad \pi^\dagger=\dot\varphi;\qquad j^0=\pi\,\delta\varphi+\pi^\dagger\,\delta\varphi^\dagger=-i\big(\pi\varphi-\pi^\dagger\varphi^\dagger\big) \]
Conjugate momenta from the Lagrangian; assemble the charge density from both fields. B
3
\[ Q=-\,i\int d^3x\,\big(\pi\varphi-\pi^\dagger\varphi^\dagger\big),\qquad [\varphi(\mathbf{x}),\pi(\mathbf{y})]=i\delta^3(\mathbf{x}-\mathbf{y}) \]
Integrate; use the complex-field canonical algebra (\( \varphi \) pairs with \( \pi \), \( \varphi^\dagger \) with \( \pi^\dagger \)). A
4
\[ [Q,\varphi(\mathbf{y})]=-\,i\int d^3x\,[\pi(\mathbf{x}),\varphi(\mathbf{y})]\,\varphi(\mathbf{x})=-\,i\int d^3x\,(-i\delta^3)\,\varphi=-\varphi(\mathbf{y}) \]
Only the \( \pi\varphi \) term contributes (\( \varphi \) commutes with \( \varphi^\dagger,\pi^\dagger \)); evaluate the delta. B
\[ [\,Q,\varphi\,]=-\varphi=-i\,\delta\varphi\quad(\delta\varphi=-i\varphi)\;\checkmark \]

Reading. \( e^{i\alpha Q}\varphi e^{-i\alpha Q}=\varphi+i\alpha(-\varphi)+\cdots=e^{-i\alpha}\varphi \), reproducing the phase rotation exactly. Acting on a one-particle state, \( Q \) returns charge \( +1 \); on an antiparticle, \( -1 \). Units: \( Q \) is dimensionless (a pure number of quanta), matching \( [\varphi] \) on both sides.

1
\[ \textbf{Momentum generates translations.}\quad x^\mu\to x^\mu+a^\mu,\qquad \delta\varphi=\partial_i\varphi\ \ (\text{per unit }a^i) \]
Spatial translation of a real scalar; the field variation is its gradient. This symmetry has \( \delta\mathcal{L}=\partial_\mu K^\mu \), so the charge is the momentum \( P_i=\int d^3x\,T^{0}{}_{i} \). B
2
\[ T^{0}{}_{i}=\pi\,\partial_i\varphi,\qquad P_i=\int d^3x\,\pi(\mathbf{x})\,\partial_i\varphi(\mathbf{x}),\qquad \pi=\dot\varphi \]
The momentum density is \( \pi\,\partial_i\varphi \) (the \( K^0 \) piece cancels the would-be \( \delta^i_i\mathcal{L} \) for the spatial components). B
3
\[ [P_i,\varphi(\mathbf{y})]=\int d^3x\,[\pi(\mathbf{x}),\varphi(\mathbf{y})]\,\partial_i\varphi(\mathbf{x})=\int d^3x\,(-i\delta^3)\,\partial_i\varphi(\mathbf{x}) \]
Use \( [\pi,\varphi]=-i\delta^3 \); \( \partial_i\varphi \) commutes with \( \varphi(\mathbf{y}) \) at equal time. B
4
\[ [P_i,\varphi(\mathbf{y})]=-\,i\,\partial_i\varphi(\mathbf{y}) \]
Integrate the delta, differentiating the gradient at \( \mathbf{x}=\mathbf{y} \). A
\[ [\,P_i,\varphi\,]=-\,i\,\partial_i\varphi=-i\,\delta\varphi\;\checkmark \]

Reading. Momentum is the generator of spatial translations: \( e^{i\mathbf{a}\cdot\mathbf{P}}\varphi(\mathbf{x})e^{-i\mathbf{a}\cdot\mathbf{P}}=\varphi(\mathbf{x}+\mathbf{a}) \). The time component gives the Heisenberg equation \( [H,\varphi]=-i\dot\varphi \). Units: \( [P_i]= \) momentum, \( [\partial_i\varphi]=[\varphi]/\text{length} \); with \( \hbar=1 \), momentum \( = 1/\text{length} \), so both sides share dimension \( [\varphi]/\text{length} \).

Problems
  1. Show that for the U(1) complex scalar, \( [Q,\varphi^\dagger]=+\varphi^\dagger \), and hence that \( \varphi^\dagger \) creates a quantum of charge \( +1 \) while \( \varphi \) lowers charge by one.
    Solution \( [Q,\varphi^\dagger(\mathbf{y})]=-i\int d^3x\,[-\pi^\dagger\varphi^\dagger,\varphi^\dagger(\mathbf{y})] \). Only the \( \pi^\dagger \) term contributes: \( =+i\int d^3x\,[\pi^\dagger(\mathbf{x}),\varphi^\dagger(\mathbf{y})]\varphi^\dagger(\mathbf{x})=+i\int d^3x\,(-i\delta^3)\varphi^\dagger=+\varphi^\dagger(\mathbf{y}) \). This equals \( -i\,\delta\varphi^\dagger \) with \( \delta\varphi^\dagger=+i\varphi^\dagger \). Since \( Q(\varphi^\dagger|q\rangle)=(q+1)\varphi^\dagger|q\rangle \) follows from \( [Q,\varphi^\dagger]=+\varphi^\dagger \), \( \varphi^\dagger \) raises charge by one.
  2. Two commuting charges \( Q_1,Q_2 \) generate variations \( \delta_1\varphi,\delta_2\varphi \). Use the Jacobi identity to show that \( [\,[Q_1,Q_2],\varphi\,]=-i\big(\delta_1(\delta_2\varphi)-\delta_2(\delta_1\varphi)\big) \), and interpret when \( [Q_1,Q_2]=0 \).
    Solution Jacobi: \( [[Q_1,Q_2],\varphi]=[Q_1,[Q_2,\varphi]]-[Q_2,[Q_1,\varphi]] \). Insert \( [Q_a,\varphi]=-i\delta_a\varphi \): \( =[Q_1,-i\delta_2\varphi]-[Q_2,-i\delta_1\varphi]=-i\big(-i\delta_1\delta_2\varphi\big)+i\big(-i\delta_2\delta_1\varphi\big) \). Wait, track carefully: \( [Q_1,-i\delta_2\varphi]=-i\,[Q_1,\delta_2\varphi]=-i(-i\,\delta_1(\delta_2\varphi))=-\delta_1\delta_2\varphi \), and similarly the second term gives \( +\delta_2\delta_1\varphi \). So \( [[Q_1,Q_2],\varphi]=-\delta_1\delta_2\varphi+\delta_2\delta_1\varphi=-\big(\delta_1\delta_2-\delta_2\delta_1\big)\varphi \). Writing this as \( -i\,\delta_{[1,2]}\varphi \) shows the charge commutator generates the commutator of transformations. If the two transformations commute (abelian), \( [Q_1,Q_2]=0 \) and the charges are simultaneously diagonalizable.
  3. A free real scalar of mass \( m \) has Hamiltonian \( H=\int d^3x\,\tfrac12(\pi^2+(\nabla\varphi)^2+m^2\varphi^2) \). Verify by direct commutation that \( [H,\varphi(\mathbf{y})]=-i\pi(\mathbf{y})=-i\dot\varphi(\mathbf{y}) \), consistent with time translation being generated by \( H \).
    Solution Only the \( \tfrac12\pi^2 \) term has a nonzero commutator with \( \varphi \): \( [H,\varphi(\mathbf{y})]=\int d^3x\,\tfrac12[\pi(\mathbf{x})^2,\varphi(\mathbf{y})] \). Use \( [\pi^2,\varphi]=\pi[\pi,\varphi]+[\pi,\varphi]\pi=2\pi(-i\delta^3) \). So \( [H,\varphi(\mathbf{y})]=\int d^3x\,\tfrac12\cdot 2\pi(\mathbf{x})(-i\delta^3(\mathbf{x}-\mathbf{y}))=-i\pi(\mathbf{y}) \). Since the Heisenberg equation gives \( \dot\varphi=i[H,\varphi]=\pi \), we confirm \( [H,\varphi]=-i\dot\varphi \), i.e. \( \delta\varphi=\dot\varphi \) for time translation.
  4. For SU(2) isospin acting on a doublet \( \varphi_a\ (a=1,2) \) as \( \delta\varphi_a=-i\,(T^A)_{ab}\varphi_b \) with \( T^A=\tfrac12\sigma^A \), write the charges \( Q^A \) and show \( [Q^A,\varphi_a]=-(T^A)_{ab}\varphi_b \). Confirm the charges satisfy \( [Q^A,Q^B]=i\epsilon^{ABC}Q^C \).
    Solution \( Q^A=\int d^3x\,\pi_a\,\delta\varphi_a/(\text{per }\alpha^A)=-i\int d^3x\,\pi_a(T^A)_{ab}\varphi_b \). Then \( [Q^A,\varphi_c(\mathbf{y})]=-i\int d^3x\,(T^A)_{ab}[\pi_a(\mathbf{x}),\varphi_c(\mathbf{y})]\varphi_b(\mathbf{x})=-i\int d^3x\,(T^A)_{ab}(-i\delta_{ac}\delta^3)\varphi_b=-(T^A)_{cb}\varphi_b(\mathbf{y}) \), matching \( -i\delta\varphi_c \). For the algebra, apply the previous problem's result: \( \delta^A\delta^B-\delta^B\delta^A \) acting on \( \varphi \) equals \( -[T^A,T^B]\varphi=-i\epsilon^{ABC}T^C\varphi \), i.e. \( \delta_{[A,B]}=\epsilon^{ABC}\delta^C \), which forces \( [Q^A,Q^B]=i\epsilon^{ABC}Q^C \) — the su(2) algebra.
  5. Estimate the "size" of a symmetry rotation: for a coherent-like field configuration with \( \varphi\sim v \) (a VEV) under U(1), how does \( e^{i\alpha Q} \) act, and why does the charge fail to exist when \( v\neq0 \)? Give the Fabri–Picasso argument schematically.
    Solution Formally \( e^{i\alpha Q}\varphi e^{-i\alpha Q}=e^{-i\alpha}\varphi \), rotating the phase of the VEV. Compute the norm of \( Q|0\rangle \): \( \langle0|Q^2|0\rangle=\int d^3x\,d^3y\,\langle0|j^0(x)j^0(y)|0\rangle \). By translation invariance the integrand depends only on \( \mathbf{x}-\mathbf{y} \), so one integral gives an overall volume factor \( V\to\infty \) times a nonzero constant (nonzero precisely because \( \langle0|j^0|0\rangle \) probes the broken order parameter \( v\neq0 \)). Hence \( \|Q|0\rangle\|^2\propto V\to\infty \): \( Q|0\rangle \) is non-normalizable, so \( Q \) does not exist as an operator on the Hilbert space and cannot be exponentiated to a unitary — the symmetry is spontaneously broken, realized non-linearly by massless Goldstone bosons. The local relation \( [Q,\varphi]=-i\delta\varphi \) survives only as a statement about the current.