Skip to content

Ward Identities and Chiral Symmetries

The previous pages used the renormalization group to show how a classically scale-free theory can generate a physical mass scale. We now pause before going further into current correlators and many-body examples, because the next layer of structure is controlled by symmetry. Symmetry does more than label states. In a local quantum field theory it becomes a system of identities among correlation functions.

Those identities are called Ward identities. They are the quantum version of current conservation, but with two important upgrades. First, local current conservation inside a time-ordered product includes contact terms when the current collides with another operator. Second, a symmetry of the classical action need not be a symmetry of the quantum measure and regulator. When this happens, the Ward identity has an anomalous term.

Massless fermions make these points vivid. A massless Dirac field has independent phase rotations of its left- and right-moving components. In two dimensions this becomes almost embarrassingly explicit: one chirality depends only on x+x^+ and the other only on xx^-. The same simplicity also exposes the axial anomaly. The vector current can be conserved as an operator identity in a background gauge field, but the axial current cannot be conserved at the same time.

Required background. Continuous symmetries, generators, and charges supplies the current and the local-parameter argument; localized transformations and Ward–Takahashi identities supplies the distributional contact-term logic used below. Helpful background. Vacuum polarization and gauge-invariant counterterms develops the same transversality condition in perturbative QED.

Light-cone and current conventions. Most formulas use the global QFT II conventions. In the two-dimensional parts of this page we use

x±=x0±x1,±=12(0±1),A±=A0±A1.x^\pm=x^0\pm x^1, \qquad \partial_\pm={1\over2}(\partial_0\pm\partial_1), \qquad A_\pm=A_0\pm A_1.

The metric is mostly minus, ημν=diag(+,)\eta_{\mu\nu}=\operatorname{diag}(+,-), and ϵ01=+1\epsilon^{01}=+1. We take

γ5=γ0γ1,P±=12(1±γ5),ψ±=P±ψ.\gamma^5=\gamma^0\gamma^1, \qquad P_\pm={1\over2}(1\pm\gamma^5), \qquad \psi_\pm=P_\pm\psi.

With these conventions one convenient identity is

γμγ5=ϵμνγν,j5μ=ψˉγμγ5ψ=ϵμνjν.\gamma^\mu\gamma^5=-\epsilon^{\mu\nu}\gamma_\nu, \qquad j_5^\mu=\bar\psi\gamma^\mu\gamma^5\psi =-\epsilon^{\mu\nu}j_\nu.

For Dirac slash notation we use the KaTeX-compatible form

p ⁣ ⁣ ⁣/γμpμ,q ⁣ ⁣ ⁣/γμqμ.p\!\!\!/\equiv\gamma^\mu p_\mu, \qquad q\!\!\!/\equiv\gamma^\mu q_\mu.

For a background gauge field we write

Dμ=μiAμ,ψe+iαψ,AμAμ+μα.D_\mu=\partial_\mu-iA_\mu, \qquad \psi\mapsto e^{+i\alpha}\psi, \qquad A_\mu\mapsto A_\mu+\partial_\mu\alpha.

The source term generated by ψˉiγμDμψ\bar\psi i\gamma^\mu D_\mu\psi is therefore +Aμjμ+A_\mu j^\mu. The displayed anomaly coefficient is for one massless Dirac fermion of positive unit charge.

Start with a field theory whose action is invariant under a continuous global transformation. For a Dirac field the simplest example is

ψ(x)e+iαψ(x),ψˉ(x)ψˉ(x)eiα.\psi(x)\mapsto e^{+i\alpha}\psi(x), \qquad \bar\psi(x)\mapsto \bar\psi(x)e^{-i\alpha}.

For the free massive Dirac Lagrangian

L=ψˉ(iγμμm)ψ,\mathcal L=\bar\psi(i\gamma^\mu\partial_\mu-m)\psi,

Noether’s theorem gives the vector current

jμ=ψˉγμψ\boxed{ j^\mu=\bar\psi\gamma^\mu\psi }

and the classical equation

μjμ=0.\partial_\mu j^\mu=0.

The quickest way to turn this into a Ward identity is to make the symmetry parameter local, αα(x)\alpha\to\alpha(x). The action is no longer invariant; instead,

δS=ddxμα(x)jμ(x)=+ddxα(x)μjμ(x),\delta S=-\int d^dx\,\partial_\mu\alpha(x)j^\mu(x) =+\int d^dx\,\alpha(x)\partial_\mu j^\mu(x),

up to boundary terms. In a path integral, an infinitesimal change of integration variables gives

0=DΦδ(eiSO).0=\int \mathcal D\Phi\,\delta\left(e^{iS}\mathcal O\right).

If the measure is invariant, this becomes a relation between the divergence of the current and the variation of the inserted operator O\mathcal O. Let QkQ_k be the charge of Ok\mathcal O_k, so δαOk=+iαQkOk\delta_\alpha\mathcal O_k=+i\alpha Q_k\mathcal O_k. With the time-ordered Green-function normalization used here, the Minkowski-space identity is

μTjμ(x)=1nO(x)=k=1nQkδ(d)(xxk)T=1nO(x).\boxed{ \begin{aligned} &\partial_\mu\left\langle Tj^\mu(x)\prod_{\ell=1}^n\mathcal O_\ell(x_\ell) \right\rangle \\ &\qquad=-\sum_{k=1}^nQ_k\delta^{(d)}(x-x_k) \left\langle T\prod_{\ell=1}^n\mathcal O_\ell(x_\ell)\right\rangle. \end{aligned} }

The right-hand side is the contact-term part of the Ward identity. Away from all other insertions, the current is conserved. At coincident points, the current generates the symmetry transformation of the operator it hits. In canonical language this is the same statement as

[Q,O(x)]=QOO(x),δαO(x)=iα[Q,O(x)]=+iαQOO(x),Q=dd1xj0,[Q,\mathcal O(x)]=-Q_{\mathcal O}\mathcal O(x), \qquad \delta_\alpha\mathcal O(x)=-i\alpha[Q,\mathcal O(x)] =+i\alpha Q_{\mathcal O}\mathcal O(x), \qquad Q=\int d^{d-1}x\,j^0,

where the transformation is implemented by U(α)=eiαQU(\alpha)=e^{-i\alpha Q} and QOQ_{\mathcal O} is the charge appearing in the phase e+iαQOe^{+i\alpha Q_{\mathcal O}}. The path-integral contact terms are the spacetime version of this equal-time commutator.

This is why Ward identities are identities of distributions, not merely identities of ordinary functions at separated points. Dropping the contact terms gives a statement that is too weak to determine counterterms and too weak to protect gauge invariance.

For the Dirac two-point function, the vector Ward identity reads

μxTjμ(x)ψ(y)ψˉ(z)=δ(d)(xy)Tψ(y)ψˉ(z)+δ(d)(xz)Tψ(y)ψˉ(z).\partial_\mu^x\left\langle Tj^\mu(x)\psi(y)\bar\psi(z)\right\rangle =-\delta^{(d)}(x-y)\langle T\psi(y)\bar\psi(z)\rangle +\delta^{(d)}(x-z)\langle T\psi(y)\bar\psi(z)\rangle.

The signs simply say that ψ\psi and ψˉ\bar\psi carry opposite U(1)U(1) charges. In momentum space, the same statement becomes the Ward–Takahashi identity

qμΓμ(p+q,p)=S1(p+q)S1(p),\boxed{ q_\mu\Gamma^\mu(p+q,p)=S^{-1}(p+q)-S^{-1}(p), }

where S(p)S(p) is the full fermion propagator and Γμ\Gamma^\mu is the full current vertex.

A current insertion on a fermion line gives the Ward identity relating the vertex to inverse propagators

The Ward–Takahashi identity says that contracting a current insertion with its momentum is equivalent to subtracting the inverse propagator on the two sides of the insertion. This is the diagrammatic form of charge conservation inside correlation functions.

This identity is much stronger than the classical equation μjμ=0\partial_\mu j^\mu=0. It constrains loop corrections. In QED it implies, after renormalization, the equality of the vertex and fermion wavefunction renormalization constants in a gauge-invariant scheme. More generally, it is the algebraic reason why gauge invariance organizes counterterms.

Background sources and transverse polarization

Section titled “Background sources and transverse polarization”

A clean way to package Ward identities is to couple a source to the current. Write

Z[A]=eiW[A]=DΦexp(iS0+iddxAμjμ).Z[A]=e^{iW[A]} =\int \mathcal D\Phi\, \exp\left(iS_0+i\int d^dx\,A_\mu j^\mu\right).

The current expectation value in the background AA is

jμ(x)A=+δW[A]δAμ(x).\langle j^\mu(x)\rangle_A=+{\delta W[A]\over\delta A_\mu(x)}.

If the source AμA_\mu is interpreted as a background gauge field, then the local transformation

ψ(x)e+iα(x)ψ(x),Aμ(x)Aμ(x)+μα(x)\psi(x)\mapsto e^{+i\alpha(x)}\psi(x), \qquad A_\mu(x)\mapsto A_\mu(x)+\partial_\mu\alpha(x)

leaves the source-coupled theory invariant. Therefore

W[A+α]=W[A].W[A+\partial\alpha]=W[A].

Expanding to first order in α\alpha gives

0=ddxμα(x)δWδAμ(x)=ddxα(x)μδWδAμ(x).0=\int d^dx\,\partial_\mu\alpha(x){\delta W\over\delta A_\mu(x)} =-\int d^dx\,\alpha(x)\partial_\mu{\delta W\over\delta A_\mu(x)}.

Since α(x)\alpha(x) is arbitrary,

μδW[A]δAμ(x)=0.\boxed{ \partial_\mu{\delta W[A]\over\delta A_\mu(x)}=0. }

Differentiating this identity once more with respect to AνA_\nu and then setting A=0A=0 gives transversality of the current-current correlator,

μxΠμν(xy)=0,\partial_\mu^x\Pi^{\mu\nu}(x-y)=0,

where

Πμν(xy)=iTjμ(x)jν(y)conn+possible local contact terms.\Pi^{\mu\nu}(x-y) =i\langle Tj^\mu(x)j^\nu(y)\rangle_{\rm conn} +\text{possible local contact terms}.

In momentum space,

qμΠμν(q)=0.\boxed{ q_\mu\Pi^{\mu\nu}(q)=0. }

Lorentz invariance then fixes the nonlocal parity-even part of the two-point function to have the form

Πμν(q)=(qμqνq2ημν)Π(q2)+local transverse terms.\boxed{ \Pi^{\mu\nu}(q) =\left(q^\mu q^\nu-q^2\eta^{\mu\nu}\right)\Pi(q^2) +\text{local transverse terms}. }

This formula is familiar from vacuum polarization, but here the lesson is more general: a conserved current can only generate a transverse response. In gauge theory, this is why a photon mass term AμAμA_\mu A^\mu is forbidden by gauge invariance, while a correction to FμνFμνF_{\mu\nu}F^{\mu\nu} is allowed.

There is one subtlety that will matter below. The correlator Tjμjν\langle Tj^\mu j^\nu\rangle by itself is not always the whole Πμν\Pi^{\mu\nu}. Local contact terms can be added by local counterterms in W[A]W[A]. They do not affect separated-point current conservation, but they do affect the precise Ward identity at coincident points. Gauge invariance often fixes those local terms.

In even spacetime dimensions, the massless Dirac Lagrangian has an additional classical symmetry. Define γ5\gamma^5 so that it anticommutes with every γμ\gamma^\mu,

{γ5,γμ}=0.\{\gamma^5,\gamma^\mu\}=0.

For m=0m=0,

L0=ψˉiγμμψ\mathcal L_0=\bar\psi i\gamma^\mu\partial_\mu\psi

is invariant under the axial rotation

ψeiβγ5ψ,ψˉψˉeiβγ5.\psi\mapsto e^{i\beta\gamma^5}\psi, \qquad \bar\psi\mapsto \bar\psi e^{i\beta\gamma^5}.

The corresponding axial current is

j5μ=ψˉγμγ5ψ.\boxed{ j_5^\mu=\bar\psi\gamma^\mu\gamma^5\psi. }

Classically,

μj5μ=0(m=0).\partial_\mu j_5^\mu=0 \qquad (m=0).

If the mass is nonzero, the axial symmetry is explicitly broken. A direct variation gives

μj5μ=2imψˉγ5ψ\boxed{ \partial_\mu j_5^\mu=2im\bar\psi\gamma^5\psi }

in Minkowski signature. The vector current remains conserved because the mass term preserves ordinary phase rotations.

The chiral projectors

P±=12(1±γ5)P_\pm={1\over2}(1\pm\gamma^5)

split the fermion into two components,

ψ=ψ++ψ.\psi=\psi_++\psi_-.

The vector and axial rotations are equivalently independent phase rotations of these two components. With the vector convention above and the axial rotation ψeiβγ5ψ\psi\mapsto e^{i\beta\gamma^5}\psi,

ψ+e+iα+iβψ+,ψe+iαiβψ.\psi_+\mapsto e^{+i\alpha+i\beta}\psi_+, \qquad \psi_-\mapsto e^{+i\alpha-i\beta}\psi_-.

The mass term mixes the two chiralities. Schematically,

mψˉψ=m(ψˉ+ψ+ψˉψ+),m\bar\psi\psi =m\left(\bar\psi_+\psi_-+\bar\psi_-\psi_+\right),

so it is invariant under the vector phase but not under the axial phase. This is the simplest way to remember why a massless fermion has more symmetry than a massive fermion.

For NN massless Dirac fermions, the symmetry is enlarged. In four dimensions, ignoring anomalies and gauge interactions for the moment, one has independent flavor rotations of left- and right-handed fermions,

U(N)L×U(N)R.U(N)_L\times U(N)_R.

Mass terms reduce this to the diagonal vector subgroup unless the mass matrix has degeneracies. This chiral flavor symmetry is one of the organizing principles of low-energy QCD, where quark masses are small compared with the strong scale.

Two dimensions are special because a massless Dirac equation separates into two one-dimensional propagation equations. With the light-cone conventions in the note above, the free massless action can be written as

The labels ++ and - are convention labels, not universal names for “right” and “left.” What matters physically is the equation of motion: one component propagates along constant xx^- and the other along constant x+x^+. When comparing references, translate the light-cone convention before comparing signs in the axial current.

S0=d2x(iψ+ψ++iψ+ψ).S_0=\int d^2x\, \left(i\psi_+^\dagger\partial_-\psi_+ +i\psi_-^\dagger\partial_+\psi_-\right).

The equations of motion are

ψ+=0,+ψ=0.\boxed{ \partial_-\psi_+=0, \qquad \partial_+\psi_-=0. }

Therefore

ψ+=ψ+(x+),ψ=ψ(x)\psi_+=\psi_+(x^+), \qquad \psi_-=\psi_-(x^-)

on shell. The two chiral densities are

J+=ψ+ψ+,J=ψψ.J_+=\psi_+^\dagger\psi_+, \qquad J_-=\psi_-^\dagger\psi_-.

They obey

J+=0,+J=0\partial_-J_+=0, \qquad \partial_+J_-=0

classically. The vector and axial currents are the sum and difference of the chiral currents. In the convention j5μ=ϵμνjνj_5^\mu=-\epsilon^{\mu\nu}j_\nu, the axial current is not an independent object in two dimensions; it is the Hodge dual of the vector current.

Vector and axial rotations of chiral fermions and the Dirac mass coupling

The two chiral components are independent when m=0m=0. The vector rotation acts with the same phase on both components, while the axial rotation acts with opposite phases. A Dirac mass couples the two chiralities and breaks the axial symmetry.

The free propagator of a chiral component has a characteristic distributional form. Up to a conventional normalization,

Tψ+(x)ψ+(0)1x+i0sgn(x).\langle T\psi_+(x)\psi_+^\dagger(0)\rangle \propto {1\over x^+-i0\operatorname{sgn}(x^-)}.

The pole prescription remembers time ordering. It also hides a contact term. The useful identity is

1x+i0sgn(x)=P1x++iπsgn(x)δ(x+),{1\over x^+-i0\operatorname{sgn}(x^-)} =\mathcal P{1\over x^+}+i\pi\operatorname{sgn}(x^-)\delta(x^+),

so

1x+i0sgn(x)=2πiδ(x+)δ(x).\partial_-{1\over x^+-i0\operatorname{sgn}(x^-)} =2\pi i\,\delta(x^+)\delta(x^-).

This is the Lorentzian cousin of

zˉ1z=πδ(2)(z).\partial_{\bar z}{1\over z}=\pi\delta^{(2)}(z).

The lesson is small but important: a chiral propagator looks holomorphic away from coincident points, but its derivative is not zero as a distribution. Contact terms are precisely what make Ward identities true.

The Thirring interaction as an auxiliary gauge field

Section titled “The Thirring interaction as an auxiliary gauge field”

The massless Thirring model is the two-dimensional current-current theory

LTh=ψˉiγμμψg2jμjμ,jμ=ψˉγμψ.\mathcal L_{\rm Th} =\bar\psi i\gamma^\mu\partial_\mu\psi -{g\over2}j_\mu j^\mu, \qquad j^\mu=\bar\psi\gamma^\mu\psi.

In light-cone variables this is, up to harmless factors of two,

LTh=iψ+ψ++iψ+ψgJ+J.\mathcal L_{\rm Th} =i\psi_+^\dagger\partial_-\psi_+ +i\psi_-^\dagger\partial_+\psi_- -gJ_+J_-.

The interaction couples the two chiral densities, but it does not mix the fields ψ+\psi_+ and ψ\psi_- the way a mass term would. It preserves the vector and axial U(1)U(1) symmetries. Power counting makes gg dimensionless, so this is a marginal current-current deformation rather than a relevant mass perturbation. Symmetry and power counting alone do not prove gaplessness; the exact solution, equivalently bosonization to a free compact scalar with a coupling-dependent radius, shows that the massless one-flavor Thirring model lies on a gapless line of fixed points. Bosonization and sine-Gordon/Thirring duality develops that equivalence later in the course.

This conclusion is specific to the Abelian one-flavor interaction written above. With several flavors there are inequivalent ways to contract flavor and chiral indices. Non-Abelian current-current or Gross–Neveu interactions can have nonzero beta functions and dynamically generate a scale. The number of flavors by itself is therefore not enough information: the operator and its symmetry representation must also be specified.

A useful rewriting introduces an auxiliary vector field AμA_\mu with no kinetic term:

L=ψˉiγμμψ+Aμjμ+12gAμAμ.\mathcal L =\bar\psi i\gamma^\mu\partial_\mu\psi +A_\mu j^\mu+{1\over2g}A_\mu A^\mu.

The equation of motion for AμA_\mu is algebraic,

Aμ=gjμ.A^\mu=-g j^\mu.

Substituting back gives

+Aμjμ+12gAμAμ=g2jμjμ.+A_\mu j^\mu+{1\over2g}A_\mu A^\mu =-{g\over2}j_\mu j^\mu.

Thus the current-current interaction is equivalent to the exchange of an auxiliary vector field.

The Thirring current-current interaction can be rewritten using an auxiliary vector field

The Thirring interaction may be decoupled by a Hubbard–Stratonovich field AμA_\mu. Because AμA_\mu has no bare kinetic term, integrating it out is exact and returns the four-fermion current-current interaction; the overall sign is a convention for gg and for the auxiliary-field quadratic term.

This rewriting is not just cosmetic. Once fermions are integrated out, the effective action for AμA_\mu is a determinant,

eiW[A]=DψDψˉexp(id2xψˉiγμ(μiAμ)ψ),e^{iW[A]}=\int \mathcal D\psi\mathcal D\bar\psi\, \exp\left(i\int d^2x\,\bar\psi i\gamma^\mu(\partial_\mu-iA_\mu)\psi\right),

or formally

W[A]=iTrlog(iγμ(μiAμ)).W[A]=-i\operatorname{Tr}\log\left(i\gamma^\mu(\partial_\mu-iA_\mu)\right).

Expanding W[A]W[A] in powers of AA generates current correlators. Gauge invariance of W[A]W[A] is exactly the vector Ward identity. The next page computes this quadratic term carefully; here we only need the conceptual point: local counterterms in W[A]W[A] decide which Ward identities are preserved.

This last sentence is the practical bridge to anomalies. The separated-point determinant may look symmetric under several classical transformations, but the local terms required to define it can privilege one symmetry over another. For a dynamical gauge field, preserving the gauge symmetry is not optional.

Vector Ward identity versus axial Ward identity

Section titled “Vector Ward identity versus axial Ward identity”

For a massless two-dimensional Dirac fermion, the vector and axial currents are related by

j5μ=ϵμρjρ.j_5^\mu=-\epsilon^{\mu\rho}j_\rho.

Define the vector two-point function

Πμν(q)=id2xeiqxTjμ(x)jν(0)conn+contact terms.\Pi^{\mu\nu}(q)=i\int d^2x\,e^{iq\cdot x} \langle Tj^\mu(x)j^\nu(0)\rangle_{\rm conn} +\text{contact terms}.

If vector gauge invariance is imposed, then

qμΠμν(q)=0.q_\mu\Pi^{\mu\nu}(q)=0.

In two dimensions, the one-loop result has the nonlocal structure

Πμν(q)=1π(ημνqμqνq2)\Pi^{\mu\nu}(q) ={1\over\pi}\left(\eta^{\mu\nu}-{q^\mu q^\nu\over q^2}\right)

for one unit-charge Dirac fermion, up to convention-dependent local signs from the definition of W[A]W[A]. This tensor is transverse:

qμΠμν(q)=0.q_\mu\Pi^{\mu\nu}(q)=0.

Now form the mixed axial-vector correlator

Π5μν(q)=id2xeiqxTj5μ(x)jν(0)conn.\Pi_5^{\mu\nu}(q) =i\int d^2x\,e^{iq\cdot x} \langle Tj_5^\mu(x)j^\nu(0)\rangle_{\rm conn}.

Using j5μ=ϵμρjρj_5^\mu=-\epsilon^{\mu\rho}j_\rho gives

Π5μν(q)=ϵμρΠρν(q).\Pi_5^{\mu\nu}(q)=-\epsilon^{\mu\rho}\Pi_\rho{}^\nu(q).

Therefore

qμΠ5μν(q)=qμϵμρ1π(δρνqρqνq2).q_\mu\Pi_5^{\mu\nu}(q) =-q_\mu\epsilon^{\mu\rho}{1\over\pi} \left(\delta_\rho{}^\nu-{q_\rho q^\nu\over q^2}\right).

The second term vanishes because qμϵμρqρ=0q_\mu\epsilon^{\mu\rho}q_\rho=0. Hence

qμΠ5μν(q)=1πϵνρqρ.\boxed{ q_\mu\Pi_5^{\mu\nu}(q) ={1\over\pi}\epsilon^{\nu\rho}q_\rho. }

Because the vector source enters as +Aνjν+A_\nu j^\nu, linear response gives j5μA=+Π5μνAν+O(A2)\langle j_5^\mu\rangle_A=+\Pi_5^{\mu\nu}A_\nu+O(A^2). Thus, suppressing the Fourier factor of ii,

qμj5μA=+1πϵνρqρAν=1πϵρνqρAν.q_\mu\langle j_5^\mu\rangle_A =+{1\over\pi}\epsilon^{\nu\rho}q_\rho A_\nu =-{1\over\pi}\epsilon^{\rho\nu}q_\rho A_\nu.

In position space this is the axial anomaly in a background gauge field:

μj5μA=1πϵμνμAν=12πϵμνFμν.\boxed{ \partial_\mu\langle j_5^\mu\rangle_A =-{1\over\pi}\epsilon^{\mu\nu}\partial_\mu A_\nu =-{1\over2\pi}\epsilon^{\mu\nu}F_{\mu\nu}. }

Thus the vector current can be conserved, or the axial current can be conserved, but not both in a gauge-invariant quantum theory with a background vector field. For a dynamical gauge field, preserving vector gauge invariance is mandatory; the axial symmetry becomes anomalous.

The vector Ward identity and the axial Ward identity cannot both be imposed after regularization

The same current-current loop tests both vector and axial Ward identities in two dimensions. A gauge-invariant choice of local counterterms preserves qμΠμν=0q_\mu\Pi^{\mu\nu}=0 and leaves a finite contact term in the epsilon-rotated axial identity.

There is a useful diagrammatic way to see why a contradiction can occur. Contracting the vacuum polarization graph with qμq_\mu gives

qμΠμν(q)ddp(2π)dtr[γνS(p+q)q ⁣ ⁣ ⁣/S(p)].q_\mu\Pi^{\mu\nu}(q) \sim \int {d^dp\over(2\pi)^d}\, \operatorname{tr}\left[ \gamma^\nu S(p+q)q\!\!\!/ S(p) \right].

Since

q ⁣ ⁣ ⁣/=S1(p+q)S1(p),q\!\!\!/=S^{-1}(p+q)-S^{-1}(p),

one is tempted to write

qμΠμν(q)ddp(2π)dtrγν[S(p)S(p+q)]=0q_\mu\Pi^{\mu\nu}(q) \sim \int {d^dp\over(2\pi)^d}\, \operatorname{tr}\,\gamma^\nu\left[S(p)-S(p+q)\right] =0

by shifting the integration variable. This argument is legitimate only if the integral is sufficiently convergent or if the regulator respects the shift. In anomalous diagrams, the formal shift changes the boundary of the regulated integration region. A finite surface term can survive.

A one-dimensional caricature is

ΛΛdp[f(p+q)f(p)]qΛΛdpf(p)=q[f(Λ)f(Λ)].\int_{-\Lambda}^{\Lambda}dp\,[f(p+q)-f(p)] \simeq q\int_{-\Lambda}^{\Lambda}dp\,f'(p) =q[f(\Lambda)-f(-\Lambda)].

If the boundary term remains finite as Λ\Lambda\to\infty, the naive shift fails. The anomaly is a regulated version of precisely this phenomenon.

A continuous symmetry gives a current. In a quantum field theory, the corresponding conservation law becomes a Ward identity: the divergence of the current inside a correlation function is zero away from insertions, but has contact terms at coincident points. In momentum space, the vector Ward identity for a fermion current is

qμΓμ(p+q,p)=S1(p+q)S1(p).q_\mu\Gamma^\mu(p+q,p)=S^{-1}(p+q)-S^{-1}(p).

Coupling the current to a background field turns the same statement into gauge invariance of W[A]W[A]. Differentiating gauge invariance gives transversality of current correlators,

qμΠμν(q)=0.q_\mu\Pi^{\mu\nu}(q)=0.

Massless fermions have chiral symmetries. In two dimensions, the massless Dirac fermion splits into independent chiral components ψ+(x+)\psi_+(x^+) and ψ(x)\psi_-(x^-). The Thirring interaction couples their densities but does not create a mass term, so it preserves the vector and axial U(1)U(1) symmetries. Its exact solution is a gapless line; this conclusion is stronger than the symmetry and power-counting argument alone.

The quantum theory adds the crucial caveat: not every classical symmetry survives regularization. In two dimensions, preserving vector gauge invariance forces the axial current to satisfy

μj5μ=12πϵμνFμν\partial_\mu j_5^\mu=-{1\over2\pi}\epsilon^{\mu\nu}F_{\mu\nu}

for one unit-charge massless Dirac fermion. This is the first anomaly in the course. Notice the logic: the anomaly is not a failure of algebra at separated points; it is a statement about the regulated contact terms of composite currents. The next page studies those current-current correlators and local counterterms more explicitly.

Replacing a Ward identity by μjμ=0\partial_\mu j^\mu=0. Inside time-ordered products, contact terms are part of the statement and generate the symmetry action on coincident insertions.

Demanding both vector and axial conservation after regularization. The two currents can coexist classically, but a regulator may not preserve both. In a gauge theory, vector gauge invariance is the identity that must be preserved.

Treating j5μ=ϵμνjνj_5^\mu=-\epsilon^{\mu\nu}j_\nu as equality of Ward identities. The identity means that the same correlator is tested in two different tensor directions. A transverse vector correlator generally has an anomalous axial divergence.

Calling a current-current interaction a mass term. The Thirring coupling is marginal in two dimensions; the mass term ψˉψ\bar\psi\psi is a relevant perturbation that mixes chiralities and breaks axial symmetry. Gaplessness follows from the exact solution, not from this distinction by itself.

Exercise 1: Derive the contact-term Ward identity

Section titled “Exercise 1: Derive the contact-term Ward identity”

Let a field Φk\Phi_k have charge QkQ_k under the global U(1)U(1) convention used on this page, so that

δΦk=iαQkΦk.\delta\Phi_k=-i\alpha Q_k\Phi_k.

Use a local parameter α(x)\alpha(x) to derive the Ward identity for

Tjμ(x)Φ1(x1)Φn(xn).\left\langle Tj^\mu(x)\Phi_1(x_1)\cdots\Phi_n(x_n)\right\rangle.
Solution

Under a local transformation, the action changes by

δS=ddxμα(x)jμ(x)=ddxα(x)μjμ(x).\delta S=\int d^dx\,\partial_\mu\alpha(x)j^\mu(x) =-\int d^dx\,\alpha(x)\partial_\mu j^\mu(x).

The path integral is invariant under a change of variables:

0=iδSTΦ1Φn+Tδ(Φ1Φn).0=\left\langle i\delta S\,T\Phi_1\cdots\Phi_n\right\rangle +\left\langle T\delta(\Phi_1\cdots\Phi_n)\right\rangle.

The operator variation is

δ(Φ1Φn)=ik=1nα(xk)QkΦ1ΦkΦn.\delta(\Phi_1\cdots\Phi_n) =-i\sum_{k=1}^n\alpha(x_k)Q_k\Phi_1\cdots\Phi_k\cdots\Phi_n.

Writing α(xk)=ddxα(x)δ(d)(xxk)\alpha(x_k)=\int d^dx\,\alpha(x)\delta^{(d)}(x-x_k) and using the arbitrariness of α(x)\alpha(x) gives

μxTjμ(x)=1nΦ(x)=k=1nQkδ(d)(xxk)T=1nΦ(x).\boxed{ \begin{aligned} &\partial_\mu^x\left\langle Tj^\mu(x)\prod_{\ell=1}^n\Phi_\ell(x_\ell) \right\rangle \\ &\qquad=-\sum_{k=1}^n Q_k\delta^{(d)}(x-x_k) \left\langle T\prod_{\ell=1}^n\Phi_\ell(x_\ell)\right\rangle \end{aligned} }.

The divergence of the current is supported only at operator insertions and generates their charge transformations. Alternative definitions that attach factors of ii to Green functions move corresponding factors between the two sides without changing this content.

Exercise 2: Construct the transverse current tensor

Section titled “Exercise 2: Construct the transverse current tensor”

Assume Lorentz invariance and current conservation in a parity-even theory. Show that a two-point function of conserved currents in momentum space has the form

Πμν(q)=(qμqνq2ημν)Π(q2)\Pi^{\mu\nu}(q)=\left(q^\mu q^\nu-q^2\eta^{\mu\nu}\right)\Pi(q^2)

up to local transverse terms.

Solution

The most general parity-even rank-two tensor built from qμq^\mu and ημν\eta^{\mu\nu} is

Πμν(q)=A(q2)ημν+B(q2)qμqν.\Pi^{\mu\nu}(q)=A(q^2)\eta^{\mu\nu}+B(q^2)q^\mu q^\nu.

Current conservation gives

0=qμΠμν(q)=A(q2)qν+B(q2)q2qν.0=q_\mu\Pi^{\mu\nu}(q) =A(q^2)q^\nu+B(q^2)q^2q^\nu.

For generic qq, this requires

A(q2)=q2B(q2).A(q^2)=-q^2B(q^2).

Therefore

Πμν(q)=B(q2)(qμqνq2ημν).\Pi^{\mu\nu}(q)=B(q^2)\left(q^\mu q^\nu-q^2\eta^{\mu\nu}\right).

Renaming B(q2)=Π(q2)B(q^2)=\Pi(q^2) gives the stated form. Polynomial transverse pieces correspond to local gauge-invariant counterterms.

Exercise 3: Derive the axial anomaly from vector response

Section titled “Exercise 3: Derive the axial anomaly from vector response”

In two dimensions, suppose the vector current correlator of one massless Dirac fermion is

Πμν(q)=1π(ημνqμqνq2).\Pi^{\mu\nu}(q)={1\over\pi} \left(\eta^{\mu\nu}-{q^\mu q^\nu\over q^2}\right).

Using j5μ=ϵμρjρj_5^\mu=-\epsilon^{\mu\rho}j_\rho, compute qμΠ5μν(q)q_\mu\Pi_5^{\mu\nu}(q).

Solution

The mixed axial-vector correlator is

Π5μν(q)=ϵμρΠρν(q).\Pi_5^{\mu\nu}(q)=-\epsilon^{\mu\rho}\Pi_\rho{}^\nu(q).

Thus

qμΠ5μν(q)=1πqμϵμρ(δρνqρqνq2).q_\mu\Pi_5^{\mu\nu}(q) =-{1\over\pi}q_\mu\epsilon^{\mu\rho} \left(\delta_\rho{}^\nu-{q_\rho q^\nu\over q^2}\right).

The second term vanishes because

qμϵμρqρ=0.q_\mu\epsilon^{\mu\rho}q_\rho=0.

Therefore

qμΠ5μν(q)=1πqμϵμν.q_\mu\Pi_5^{\mu\nu}(q) =-{1\over\pi}q_\mu\epsilon^{\mu\nu}.

Since qμϵμν=ϵνρqρq_\mu\epsilon^{\mu\nu}=-\epsilon^{\nu\rho}q_\rho, we find

qμΠ5μν(q)=1πϵνρqρ.\boxed{ q_\mu\Pi_5^{\mu\nu}(q)={1\over\pi}\epsilon^{\nu\rho}q_\rho. }

This is the momentum-space axial anomaly in the convention used on this page.

Exercise 4: Integrate out the Thirring auxiliary field

Section titled “Exercise 4: Integrate out the Thirring auxiliary field”

Show that integrating out the auxiliary field in

LA=ψˉiγμμψ+Aμjμ+12gAμAμ\mathcal L_A=\bar\psi i\gamma^\mu\partial_\mu\psi +A_\mu j^\mu+{1\over2g}A_\mu A^\mu

reproduces the Thirring interaction (g/2)jμjμ-(g/2)j_\mu j^\mu.

Solution

The AμA_\mu equation of motion is

+jμ+1gAμ=0,+j^\mu+{1\over g}A^\mu=0,

so

Aμ=gjμ.A^\mu=-gj^\mu.

Substitute this into the AA-dependent part of the Lagrangian:

+Aμjμ+12gAμAμ=gjμjμ+12gg2jμjμ.+A_\mu j^\mu+{1\over2g}A_\mu A^\mu =-g j_\mu j^\mu+{1\over2g}g^2j_\mu j^\mu.

Hence

+Aμjμ+12gAμAμ=g2jμjμ.+A_\mu j^\mu+{1\over2g}A_\mu A^\mu =-{g\over2}j_\mu j^\mu.

The auxiliary-field path integral gives the same result, up to an irrelevant Gaussian normalization.

Exercise 5: Expose the chiral propagator contact term

Section titled “Exercise 5: Expose the chiral propagator contact term”

For the massless two-dimensional chiral propagator

G+(x)=1x+i0sgn(x),G_+(x)={1\over x^+-i0\operatorname{sgn}(x^-)},

use

1x+i0sgn(x)=P1x++iπsgn(x)δ(x+){1\over x^+-i0\operatorname{sgn}(x^-)} =\mathcal P{1\over x^+}+i\pi\operatorname{sgn}(x^-)\delta(x^+)

to show that G+(x)\partial_-G_+(x) is a contact term.

Solution

The principal-value term has no xx^- dependence, so

P1x+=0.\partial_-\mathcal P{1\over x^+}=0.

The second term gives

(iπsgn(x)δ(x+))=iπ(2δ(x))δ(x+).\partial_-\left(i\pi\operatorname{sgn}(x^-)\delta(x^+)\right) =i\pi\left(2\delta(x^-)\right)\delta(x^+).

Therefore

G+(x)=2πiδ(x+)δ(x).\boxed{ \partial_-G_+(x)=2\pi i\,\delta(x^+)\delta(x^-). }

Thus the chiral propagator is annihilated by \partial_- away from the origin, but not as a distribution. This is exactly the kind of contact term that appears in Ward identities.

  • S. Coleman, Lectures of Sidney Coleman on Quantum Field Theory, B. Gin-ge Chen, D. Derbes, D. Griffiths, B. Hill, R. Sohn, and Y.-S. Ting (eds.), World Scientific (2019), especially the lectures on symmetries, Ward identities, and two-dimensional fermions.
  • A. M. Polyakov, Gauge Fields and Strings, Harwood Academic Publishers (1987), especially the discussions of two-dimensional field theory and anomalies.
  • M. D. Schwartz, Quantum Field Theory and the Standard Model, Cambridge University Press (2014), chs. 14 and 30.
  • M. Srednicki, Quantum Field Theory, Cambridge University Press (2007), sections on continuous symmetries, Ward identities, and anomalies.
  • S. Weinberg, The Quantum Theory of Fields, Vols. I–II, Cambridge University Press (1995–1996), chapters on symmetries, current algebra, and anomalies.
  • A. Zee, Quantum Field Theory in a Nutshell, 2nd ed., Princeton University Press (2010), discussions of chiral symmetry, bosonization, and anomalies.