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Sources and Generating Functionals

The previous page introduced the stress tensor and conserved currents as responses to background fields. This page turns that idea into a systematic tool.

A local operator is not just something we insert into a correlation function. It is something we can source. If Oi(x)\mathcal O_i(x) is a local operator, then a background function λi(x)\lambda^i(x) coupled to Oi(x)\mathcal O_i(x) lets us define a generating functional. Differentiating this generating functional with respect to λi(x)\lambda^i(x) creates insertions of Oi(x)\mathcal O_i(x).

That sounds like a formal trick. In AdS/CFT it becomes physical:

CFT sourceboundary value of a bulk field.\boxed{ \text{CFT source} \quad\longleftrightarrow\quad \text{boundary value of a bulk field}. }

The source formalism is therefore not optional background technology. It is the CFT half of the holographic dictionary.

We work mostly in Euclidean signature. Let Φ\Phi denote all microscopic fields of the theory. For scalar operator sources λi(x)\lambda^i(x), background gauge fields Aμa(x)A_\mu^a(x), and a background metric gμν(x)g_{\mu\nu}(x), define

Z[g,A,λ]=[DΦ]g,A,λeS[g,A,λ],\mathcal Z[g,A,\lambda] = \int [D\Phi]_{g,A,\lambda}\,e^{-S[g,A,\lambda]},

with

S[g,A,λ]=SCFT[Φ;g]+ddxgλi(x)Oi(x)+ddxgAμa(x)Jaμ(x)+.S[g,A,\lambda] = S_{\mathrm{CFT}}[\Phi;g] + \int d^d x\sqrt g\,\lambda^i(x)\mathcal O_i(x) + \int d^d x\sqrt g\,A_\mu^a(x)J^\mu_a(x) + \cdots.

The dots include possible higher-spin sources, fermionic sources in supersymmetric theories, and local counterterms needed to define the theory. The source AμaA_\mu^a is a background gauge field for a global symmetry; it is not integrated over in the CFT path integral.

We define the Euclidean connected generating functional by

W[g,A,λ]=logZ[g,A,λ].W[g,A,\lambda] = -\log \mathcal Z[g,A,\lambda].

This is the convention already used in the previous page. Many QFT texts instead define W=logZ\mathcal W=\log\mathcal Z. That convention is also fine, but every sign in the derivative formulas below changes. Here we use W=logZW=-\log\mathcal Z because it is the convention naturally matched to a Euclidean on-shell bulk action:

Zbulk[boundary data]exp[Srenos]WCFTSrenos.\mathcal Z_{\mathrm{bulk}}[\text{boundary data}] \simeq \exp\left[-S^{\mathrm{os}}_{\mathrm{ren}}\right] \quad\Rightarrow\quad W_{\mathrm{CFT}}\simeq S^{\mathrm{os}}_{\mathrm{ren}}.

The vacuum normalization is often irrelevant. One may use

Wnorm[g,A,λ]=W[g,A,λ]W[g,A,0]W_{\mathrm{norm}}[g,A,\lambda] = W[g,A,\lambda]-W[g,A,0]

when only connected correlators with operator insertions are desired.

The defining property of WW is that its first variation gives one-point functions in the presence of sources:

δW=12ddxgTμνδgμν+ddxgJaμδAμa+ddxgOiδλi.\delta W = \frac12\int d^d x\sqrt g\,\langle T^{\mu\nu}\rangle\delta g_{\mu\nu} + \int d^d x\sqrt g\,\langle J^\mu_a\rangle\delta A_\mu^a + \int d^d x\sqrt g\,\langle\mathcal O_i\rangle\delta\lambda^i.

Equivalently,

Tμν(x)=2gδWδgμν(x),\langle T^{\mu\nu}(x)\rangle = \frac{2}{\sqrt g}\frac{\delta W}{\delta g_{\mu\nu}(x)}, Jaμ(x)=1gδWδAμa(x),Oi(x)=1gδWδλi(x).\langle J^\mu_a(x)\rangle = \frac{1}{\sqrt g}\frac{\delta W}{\delta A_\mu^a(x)}, \qquad \langle\mathcal O_i(x)\rangle = \frac{1}{\sqrt g}\frac{\delta W}{\delta\lambda^i(x)}.

These expectation values are evaluated in the theory with the sources turned on. This matters. The symbol

Oi(x)g,A,λ\langle\mathcal O_i(x)\rangle_{g,A,\lambda}

means the one-point function in the deformed background, not necessarily the vacuum one-point function of the original flat-space CFT.

For most flat-space CFTs on Rd\mathbb R^d, one-point functions of non-identity primary operators vanish when all sources are set to zero:

Oi(x)λ=0=0.\langle\mathcal O_i(x)\rangle_{\lambda=0}=0.

But they need not vanish in a nontrivial state, on curved space, at finite temperature, in the presence of defects, or when sources are nonzero.

Sources, generating functional, responses, connected correlators, and the holographic on-shell action

Background sources define the Euclidean functional Z=eW\mathcal Z=e^{-W}. First derivatives of WW give one-point responses such as T\langle T\rangle, J\langle J\rangle, and O\langle\mathcal O\rangle. Higher derivatives give connected correlators, up to the sign (1)n1(-1)^{n-1} in the convention W=logZW=-\log\mathcal Z. In AdS/CFT, sources are boundary values of bulk fields and WCFTW_{\mathrm{CFT}} is computed by the renormalized on-shell bulk action in the classical limit.

Full correlators versus connected correlators

Section titled “Full correlators versus connected correlators”

The partition function Z\mathcal Z generates ordinary, not necessarily connected, correlation functions. The functional W=logZW=-\log\mathcal Z generates connected correlation functions.

To see the sign carefully, consider a single scalar source λ(x)\lambda(x) coupled as

S[λ]=S0+ddxgλ(x)O(x).S[\lambda] = S_0+ \int d^d x\sqrt g\,\lambda(x)\mathcal O(x).

Then

1gδWδλ(x)=O(x)λ.\frac{1}{\sqrt g}\frac{\delta W}{\delta\lambda(x)} = \langle\mathcal O(x)\rangle_\lambda.

The second derivative gives the linear response:

1g(x)g(y)δ2Wδλ(x)δλ(y)=O(x)O(y)c,λ+contact terms.\frac{1}{\sqrt{g(x)}\sqrt{g(y)}} \frac{\delta^2 W}{\delta\lambda(x)\delta\lambda(y)} = -\langle\mathcal O(x)\mathcal O(y)\rangle_{c,\lambda} +\text{contact terms}.

At separated points, and when the operator itself has no explicit source dependence,

O(x)O(y)c=1g(x)g(y)δ2Wδλ(x)δλ(y)λ=0.\boxed{ \langle\mathcal O(x)\mathcal O(y)\rangle_c = - \frac{1}{\sqrt{g(x)}\sqrt{g(y)}} \frac{\delta^2 W}{\delta\lambda(x)\delta\lambda(y)} \bigg|_{\lambda=0}. }

More generally,

O(x1)O(xn)c=(1)n11g1gnδnWδλ(x1)δλ(xn)λ=0\boxed{ \langle\mathcal O(x_1)\cdots\mathcal O(x_n)\rangle_c = (-1)^{n-1} \frac{1}{\sqrt{g_1}\cdots\sqrt{g_n}} \frac{\delta^n W}{\delta\lambda(x_1)\cdots\delta\lambda(x_n)} \bigg|_{\lambda=0} }

at separated points. Here gi=g(xi)g_i=g(x_i).

Equivalently, the expansion of WW around zero source is

W[λ]=W[0]+n=1(1)n+1n!ddx1g1ddxngnλ(x1)λ(xn)O(x1)O(xn)c.W[\lambda] = W[0] + \sum_{n=1}^{\infty} \frac{(-1)^{n+1}}{n!} \int d^d x_1\sqrt{g_1}\cdots d^d x_n\sqrt{g_n}\, \lambda(x_1)\cdots\lambda(x_n) \langle\mathcal O(x_1)\cdots\mathcal O(x_n)\rangle_c.

The alternating sign is not physics. It is a bookkeeping consequence of the Euclidean convention S[λ]=S0+λOS[\lambda]=S_0+\int\lambda\mathcal O and W=logZW=-\log\mathcal Z.

If Oi\mathcal O_i is a scalar primary of scaling dimension Δi\Delta_i, then the source λi\lambda^i has engineering dimension

[λi]=dΔi.[\lambda^i]=d-\Delta_i.

This follows from the requirement that the deformation

ddxλiOi\int d^d x\,\lambda^i\mathcal O_i

be dimensionless. A constant source is therefore:

Operator dimensionSource typeInterpretation
Δi<d\Delta_i<drelevantdrives the CFT away from the fixed point in the IR
Δi=d\Delta_i=dmarginalmay preserve conformality if the beta function vanishes
Δi>d\Delta_i>dirrelevantgrows toward the UV and usually requires extra UV data

The source λi\lambda^i can also be position-dependent. A position-dependent source is not simply a coupling constant; it is a background field. If the source is varied in space, translation invariance is explicitly broken, and the stress tensor Ward identity notices this.

For example, with scalar sources turned on, the diffeomorphism Ward identity has the schematic form

μTμν=FνμaJaμ+Oiνλi+anomaly terms.\nabla_\mu\langle T^\mu{}_{\nu}\rangle = F^a_{\nu\mu}\langle J^\mu_a\rangle + \langle\mathcal O_i\rangle\nabla_\nu\lambda^i + \text{anomaly terms}.

This equation says exactly what it should say. A background gauge field can exert a force on the CFT, and a spatially varying scalar source can inject momentum.

Source transformations and Ward identities

Section titled “Source transformations and Ward identities”

The cleanest derivation of Ward identities is not to insert currents manually. It is to demand that W[g,A,λ]W[g,A,\lambda] be invariant under transformations of the background sources.

Suppose the CFT has a global symmetry group GG. We couple its current to a background gauge field AμaA_\mu^a. If the scalar sources λi\lambda^i transform in some representation of GG, then under an infinitesimal background gauge transformation,

δαAμa=Dμαa,\delta_\alpha A_\mu^a=D_\mu\alpha^a, δαλi=αa(ta)ijλj,\delta_\alpha\lambda^i =-\alpha^a(t_a)^i{}_j\lambda^j,

where the sign is a convention for the representation matrices tat_a. Gauge invariance of WW gives

0=δαW=ddxg(JaμDμαaOiαa(ta)ijλj)0=\delta_\alpha W = \int d^d x\sqrt g\, \left( \langle J^\mu_a\rangle D_\mu\alpha^a - \langle\mathcal O_i\rangle\alpha^a(t_a)^i{}_j\lambda^j \right)

when there is no anomaly. Integrating by parts gives

DμJaμ=Oi(ta)ijλj.D_\mu\langle J^\mu_a\rangle = - \langle\mathcal O_i\rangle(t_a)^i{}_j\lambda^j.

If the scalar sources vanish, this reduces to current conservation:

DμJaμ=0.D_\mu\langle J^\mu_a\rangle=0.

If there is an anomaly, the right-hand side receives an additional local functional of the background fields:

DμJaμ=Oi(ta)ijλj+Aa[A,g,λ].D_\mu\langle J^\mu_a\rangle = - \langle\mathcal O_i\rangle(t_a)^i{}_j\lambda^j + \mathcal A_a[A,g,\lambda].

An anomaly is not a failure of the method. It is exactly what the source formalism is designed to expose.

A CFT should also know how to respond to a Weyl rescaling of the background metric. Let

δσgμν=2σgμν.\delta_\sigma g_{\mu\nu}=2\sigma g_{\mu\nu}.

If Oi\mathcal O_i is a primary operator of dimension Δi\Delta_i, its source transforms as a spurion of dimension dΔid-\Delta_i:

δσλi=(dΔi)σλi.\delta_\sigma\lambda^i =-(d-\Delta_i)\sigma\lambda^i.

Then the Weyl variation of WW gives

δσW=ddxgσ[Tμμi(dΔi)λiOi].\delta_\sigma W = \int d^d x\sqrt g\,\sigma \left[ \langle T^\mu{}_{\mu}\rangle - \sum_i(d-\Delta_i)\lambda^i\langle\mathcal O_i\rangle \right].

At a conformal fixed point with all scalar sources turned off, the right-hand side is zero in odd dimensions on a topologically trivial flat background, and equals the Weyl anomaly in even dimensions on curved backgrounds:

Tμμ=A[g,A].\langle T^\mu{}_{\mu}\rangle = \mathcal A[g,A].

In flat space with no anomaly and no sources,

Tμμ=0.\langle T^\mu{}_{\mu}\rangle=0.

This is the source-functional version of the stress-tensor tracelessness condition.

A common mistake is to think that contact terms are ignorable technicalities. They are not. Contact terms are exactly where background-field definitions, anomalies, and Ward identities live.

For example, the separated-point two-point function of scalar primaries is fixed by conformal symmetry:

Oi(x)Oj(0)=Gijx2Δiif Δi=Δj.\langle\mathcal O_i(x)\mathcal O_j(0)\rangle = \frac{G_{ij}}{|x|^{2\Delta_i}} \qquad \text{if }\Delta_i=\Delta_j.

But the full distribution may also contain terms supported at x=0x=0, such as derivatives of delta functions. These are contact terms. In the generating functional, they arise from local terms in WW:

Wct[λ]=ddxg(CijλiλjR+Dijμλiμλj+).W_{\mathrm{ct}}[\lambda] = \int d^d x\sqrt g\, \left( C_{ij}\lambda^i\lambda^j R + D_{ij}\nabla_\mu\lambda^i\nabla^\mu\lambda^j + \cdots \right).

Differentiating WctW_{\mathrm{ct}} gives contributions only when insertion points collide. Such terms are usually scheme-dependent, because one may add finite local counterterms. But not all contact terms are arbitrary. Anomalous contact terms can be protected and physically meaningful.

In AdS/CFT this distinction is mirrored by holographic renormalization. Divergent local terms must be subtracted by boundary counterterms. Finite local counterterms change scheme-dependent contact terms. The nonlocal part of the renormalized on-shell action gives separated-point CFT correlators.

A source is not the same thing as a state.

A source changes the action or background:

SS+λO.S\to S+\int\lambda\mathcal O.

A state specifies which expectation values are taken. In Lorentzian QFT, states are selected by initial conditions, density matrices, or operator insertions. In Euclidean QFT, states can be prepared by path integrals with specified boundary conditions or insertions.

This distinction becomes essential in holography. Near the AdS boundary, a scalar bulk field dual to an operator of dimension Δ\Delta behaves schematically as

ϕ(z,x)zdΔλ(x)+zΔA(x)+,z0.\phi(z,x) \sim z^{d-\Delta}\lambda(x) + z^{\Delta}A(x) + \cdots, \qquad z\to0.

The coefficient λ(x)\lambda(x) is the source. The coefficient A(x)A(x) is related to the expectation value O(x)\langle\mathcal O(x)\rangle, after holographic renormalization. The precise normalization depends on conventions, counterterms, and possible logarithmic terms, but the conceptual split is robust:

non-normalizable modesource,normalizable moderesponse/state data.\boxed{ \text{non-normalizable mode} \leftrightarrow \text{source}, \qquad \text{normalizable mode} \leftrightarrow \text{response/state data}. }

This is the standard quantization statement. In the Breitenlohner-Freedman window where alternate quantization is allowed, the two independent asymptotic coefficients can exchange roles after an appropriate Legendre transform. We will return to that refinement later.

This is one of the reasons generating functionals are the natural language of AdS/CFT.

Although the connected generating functional WW is the main object for AdS/CFT, it is useful to know the related effective action. Define the source-dependent one-point function

φi(x)=1gδWδλi(x)=Oi(x)λ.\varphi_i(x) = \frac{1}{\sqrt g}\frac{\delta W}{\delta\lambda^i(x)} = \langle\mathcal O_i(x)\rangle_\lambda.

A Legendre transform exchanges the source λi\lambda^i for the response φi\varphi_i. With our sign convention, a natural definition is

Γ[φ]=W[λ]ddxgλiφi,\Gamma[\varphi] = W[\lambda] - \int d^d x\sqrt g\,\lambda^i\varphi_i,

where λ\lambda is eliminated in favor of φ\varphi. Then

1gδΓδφi(x)=λi(x).\frac{1}{\sqrt g}\frac{\delta\Gamma}{\delta\varphi_i(x)} = -\lambda^i(x).

This object is useful when discussing spontaneous symmetry breaking, effective potentials, double-trace deformations, and alternative quantization in AdS. But for the basic holographic dictionary, W[λ]W[\lambda] is primary: the boundary value of the bulk field is the source, and differentiating WW gives the response.

The source formalism also makes multi-trace deformations almost automatic. Suppose a large-NN CFT contains a single-trace scalar operator O\mathcal O. A double-trace deformation has the form

Sf=SCFT+f2ddxO(x)2.S_f = S_{\mathrm{CFT}} + \frac{f}{2}\int d^d x\,\mathcal O(x)^2.

This is not a linear source, but it can be studied by introducing an auxiliary field σ(x)\sigma(x):

exp[f2O2][Dσ]exp[(12fσ2+iσO)],\exp\left[-\frac{f}{2}\int\mathcal O^2\right] \propto \int[D\sigma]\, \exp\left[ -\int\left( \frac{1}{2f}\sigma^2+i\sigma\mathcal O \right) \right],

up to contour and sign conventions. The double-trace deformation is thereby converted into a source problem for O\mathcal O. In AdS/CFT, double-trace deformations correspond to mixed boundary conditions for the dual bulk field. This will become important later, especially in large-NN CFT.

The source formalism is the sharpest way to state the AdS/CFT dictionary:

ZCFT[gμν,Aμa,λi]=Zbulk[GMNgμν,AMaAμa,ϕiλi].\boxed{ \mathcal Z_{\mathrm{CFT}}[g_{\mu\nu},A_\mu^a,\lambda^i] = \mathcal Z_{\mathrm{bulk}}[G_{MN}\to g_{\mu\nu},\,\mathcal A_M^a\to A_\mu^a,\,\phi^i\to\lambda^i]. }

In the classical bulk limit,

WCFT[g,A,λ]=logZCFTSrenos[g,A,λ].W_{\mathrm{CFT}}[g,A,\lambda] = -\log\mathcal Z_{\mathrm{CFT}} \simeq S^{\mathrm{os}}_{\mathrm{ren}}[g,A,\lambda].

Therefore,

Oi(x)=1gδSrenosδλi(x),\langle\mathcal O_i(x)\rangle = \frac{1}{\sqrt g}\frac{\delta S^{\mathrm{os}}_{\mathrm{ren}}}{\delta\lambda^i(x)}, Jaμ(x)=1gδSrenosδAμa(x),\langle J^\mu_a(x)\rangle = \frac{1}{\sqrt g}\frac{\delta S^{\mathrm{os}}_{\mathrm{ren}}}{\delta A_\mu^a(x)}, Tμν(x)=2gδSrenosδgμν(x),\langle T^{\mu\nu}(x)\rangle = \frac{2}{\sqrt g}\frac{\delta S^{\mathrm{os}}_{\mathrm{ren}}}{\delta g_{\mu\nu}(x)},

in the convention of this course. Higher functional derivatives of SrenosS^{\mathrm{os}}_{\mathrm{ren}} give connected CFT correlators at leading order in the bulk saddle expansion.

This is why so much of practical AdS/CFT consists of the following steps:

  1. Choose boundary sources.
  2. Solve bulk equations with those boundary conditions.
  3. Renormalize the on-shell action.
  4. Differentiate with respect to the sources.

All four steps are just the source-response logic of QFT written geometrically.

The partition function Z\mathcal Z generates full correlators. The functional W=logZW=-\log\mathcal Z generates connected correlators, with the sign (1)n1(-1)^{n-1} in the convention used here.

If one defines W=logZ\mathcal W=\log\mathcal Z and couples sources as e+JOe^{+\int J\mathcal O}, connected correlators are derivatives of W\mathcal W without the alternating signs above. Both conventions are common. Mixing them is the real danger.

Pitfall 3: treating all contact terms as meaningless

Section titled “Pitfall 3: treating all contact terms as meaningless”

Many contact terms are scheme-dependent. Some are anomaly-related and physical. The source functional is the right place to tell the difference.

Pitfall 4: mistaking a source for a dynamical field

Section titled “Pitfall 4: mistaking a source for a dynamical field”

In the CFT, gμνg_{\mu\nu}, AμaA_\mu^a, and λi\lambda^i are background sources. They are not integrated over. In the bulk dual, the fields whose boundary values equal these sources are dynamical in the interior, but their boundary values are fixed when computing Zbulk\mathcal Z_{\mathrm{bulk}}.

The source is boundary data. The vev is the response. In AdS language, the source and response are usually the two independent asymptotic coefficients of a bulk field.

Sources turn local operators into functional derivatives:

Oi(x)=1gδWδλi(x).\langle\mathcal O_i(x)\rangle = \frac{1}{\sqrt g}\frac{\delta W}{\delta\lambda^i(x)}.

The connected generating functional in this course is

W=logZ.W=-\log\mathcal Z.

Therefore separated-point connected correlators obey

O(x1)O(xn)c=(1)n11g1gnδnWδλ(x1)δλ(xn)λ=0.\langle\mathcal O(x_1)\cdots\mathcal O(x_n)\rangle_c = (-1)^{n-1} \frac{1}{\sqrt{g_1}\cdots\sqrt{g_n}} \frac{\delta^n W}{\delta\lambda(x_1)\cdots\delta\lambda(x_n)} \bigg|_{\lambda=0}.

Background gauge invariance, diffeomorphism invariance, and Weyl covariance of WW generate the current, stress-tensor, and trace Ward identities. Contact terms are controlled by local terms in WW.

In AdS/CFT,

WCFT[sources]Srenos[bulk fields with fixed boundary values],W_{\mathrm{CFT}}[\text{sources}] \simeq S_{\mathrm{ren}}^{\mathrm{os}}[\text{bulk fields with fixed boundary values}],

so the QFT source-response formalism becomes the practical prescription for computing holographic one-point functions and correlators.

Exercise 1 — The sign of the connected two-point function

Section titled “Exercise 1 — The sign of the connected two-point function”

Let

Z[λ]=[DΦ]eS0ddxλ(x)O(x),W[λ]=logZ[λ].\mathcal Z[\lambda] = \int[D\Phi]e^{-S_0-\int d^d x\,\lambda(x)\mathcal O(x)}, \qquad W[\lambda]=-\log\mathcal Z[\lambda].

Assume O\mathcal O has no explicit dependence on λ\lambda. Show that

δ2Wδλ(x)δλ(y)=O(x)O(y)c.\frac{\delta^2 W}{\delta\lambda(x)\delta\lambda(y)} = -\langle\mathcal O(x)\mathcal O(y)\rangle_c.
Solution

First,

δWδλ(x)=1ZδZδλ(x).\frac{\delta W}{\delta\lambda(x)} = -\frac{1}{\mathcal Z}\frac{\delta\mathcal Z}{\delta\lambda(x)}.

Since

δZδλ(x)=ZO(x),\frac{\delta\mathcal Z}{\delta\lambda(x)} = -\mathcal Z\langle\mathcal O(x)\rangle,

we get

δWδλ(x)=O(x).\frac{\delta W}{\delta\lambda(x)} = \langle\mathcal O(x)\rangle.

Now differentiate once more:

δδλ(y)O(x)=δδλ(y)(1Z[DΦ]O(x)eS0λO).\frac{\delta}{\delta\lambda(y)}\langle\mathcal O(x)\rangle = \frac{\delta}{\delta\lambda(y)} \left( \frac{1}{\mathcal Z}\int[D\Phi]\,\mathcal O(x)e^{-S_0-\int\lambda\mathcal O} \right).

The derivative of the numerator gives

O(x)O(y).-\langle\mathcal O(x)\mathcal O(y)\rangle.

The derivative of 1/Z1/\mathcal Z gives

+O(x)O(y).+\langle\mathcal O(x)\rangle\langle\mathcal O(y)\rangle.

Therefore

δ2Wδλ(x)δλ(y)=O(x)O(y)+O(x)O(y)=O(x)O(y)c.\frac{\delta^2 W}{\delta\lambda(x)\delta\lambda(y)} = -\langle\mathcal O(x)\mathcal O(y)\rangle + \langle\mathcal O(x)\rangle\langle\mathcal O(y)\rangle = -\langle\mathcal O(x)\mathcal O(y)\rangle_c.

Let O\mathcal O be a scalar primary of dimension Δ\Delta in a dd-dimensional CFT. Show that the source λ\lambda in

ddxλO\int d^d x\,\lambda\mathcal O

has dimension dΔd-\Delta. Then classify the deformation as relevant, marginal, or irrelevant.

Solution

The action is dimensionless. Since

[ddx]=d,[O]=Δ,[d^d x]=-d, \qquad [\mathcal O]=\Delta,

we need

[ddx]+[λ]+[O]=0.[d^d x]+[\lambda]+[\mathcal O]=0.

Thus

d+[λ]+Δ=0,-d+[\lambda]+\Delta=0,

so

[λ]=dΔ.[\lambda]=d-\Delta.

If Δ<d\Delta<d, then [λ]>0[\lambda]>0 and the deformation is relevant. If Δ=d\Delta=d, it is marginal. If Δ>d\Delta>d, it is irrelevant.

Exercise 3 — Gauge Ward identity with charged sources

Section titled “Exercise 3 — Gauge Ward identity with charged sources”

Assume

δW=ddxg(JaμδAμa+Oiδλi).\delta W = \int d^d x\sqrt g\, \left( \langle J^\mu_a\rangle\delta A_\mu^a + \langle\mathcal O_i\rangle\delta\lambda^i \right).

Under a background gauge transformation,

δαAμa=Dμαa,δαλi=αa(ta)ijλj.\delta_\alpha A_\mu^a=D_\mu\alpha^a, \qquad \delta_\alpha\lambda^i=-\alpha^a(t_a)^i{}_j\lambda^j.

Derive the Ward identity for DμJaμD_\mu\langle J^\mu_a\rangle assuming no anomaly.

Solution

Gauge invariance says δαW=0\delta_\alpha W=0. Therefore

0=ddxg(JaμDμαaOiαa(ta)ijλj).0= \int d^d x\sqrt g\, \left( \langle J^\mu_a\rangle D_\mu\alpha^a - \langle\mathcal O_i\rangle\alpha^a(t_a)^i{}_j\lambda^j \right).

Integrate the first term by parts:

ddxgJaμDμαa=ddxgαaDμJaμ,\int d^d x\sqrt g\,\langle J^\mu_a\rangle D_\mu\alpha^a = - \int d^d x\sqrt g\,\alpha^aD_\mu\langle J^\mu_a\rangle,

assuming the boundary term vanishes. Then

0=ddxgαa(DμJaμ+Oi(ta)ijλj).0= -\int d^d x\sqrt g\,\alpha^a \left( D_\mu\langle J^\mu_a\rangle + \langle\mathcal O_i\rangle(t_a)^i{}_j\lambda^j \right).

Since αa(x)\alpha^a(x) is arbitrary,

DμJaμ=Oi(ta)ijλj.D_\mu\langle J^\mu_a\rangle = - \langle\mathcal O_i\rangle(t_a)^i{}_j\lambda^j.

When λi=0\lambda^i=0, this reduces to current conservation.

Exercise 4 — Weyl Ward identity with scalar sources

Section titled “Exercise 4 — Weyl Ward identity with scalar sources”

Assume

δW=12ddxgTμνδgμν+ddxgOiδλi.\delta W = \frac12\int d^d x\sqrt g\,\langle T^{\mu\nu}\rangle\delta g_{\mu\nu} + \int d^d x\sqrt g\,\langle\mathcal O_i\rangle\delta\lambda^i.

Under a Weyl transformation,

δσgμν=2σgμν,δσλi=(dΔi)σλi.\delta_\sigma g_{\mu\nu}=2\sigma g_{\mu\nu}, \qquad \delta_\sigma\lambda^i=-(d-\Delta_i)\sigma\lambda^i.

Show that the Weyl variation of WW is

δσW=ddxgσ[Tμμi(dΔi)λiOi].\delta_\sigma W = \int d^d x\sqrt g\,\sigma \left[ \langle T^\mu{}_{\mu}\rangle - \sum_i(d-\Delta_i)\lambda^i\langle\mathcal O_i\rangle \right].
Solution

Insert the Weyl variations into the first-variation formula. The metric term gives

12ddxgTμν(2σgμν)=ddxgσTμμ.\frac12\int d^d x\sqrt g\,\langle T^{\mu\nu}\rangle(2\sigma g_{\mu\nu}) = \int d^d x\sqrt g\,\sigma\langle T^\mu{}_{\mu}\rangle.

The scalar-source term gives

ddxgOi[(dΔi)σλi]=ddxgσi(dΔi)λiOi.\int d^d x\sqrt g\,\langle\mathcal O_i\rangle \left[-(d-\Delta_i)\sigma\lambda^i\right] = - \int d^d x\sqrt g\,\sigma \sum_i(d-\Delta_i)\lambda^i\langle\mathcal O_i\rangle.

Adding both terms yields

δσW=ddxgσ[Tμμi(dΔi)λiOi].\delta_\sigma W = \int d^d x\sqrt g\,\sigma \left[ \langle T^\mu{}_{\mu}\rangle - \sum_i(d-\Delta_i)\lambda^i\langle\mathcal O_i\rangle \right].

If the theory is Weyl invariant and has no anomaly, the bracket must vanish.

Exercise 5 — Holographic one-point function from an on-shell action

Section titled “Exercise 5 — Holographic one-point function from an on-shell action”

Suppose the renormalized Euclidean bulk on-shell action for a scalar source has the quadratic form

Srenos[λ]=12ddxddyλ(x)K(x,y)λ(y),S_{\mathrm{ren}}^{\mathrm{os}}[\lambda] = \frac12\int d^d x\,d^d y\,\lambda(x)K(x,y)\lambda(y),

with K(x,y)=K(y,x)K(x,y)=K(y,x). In the convention WCFTSrenosW_{\mathrm{CFT}}\simeq S_{\mathrm{ren}}^{\mathrm{os}}, compute O(x)λ\langle\mathcal O(x)\rangle_\lambda and the connected two-point function.

Solution

The one-point function is the first functional derivative:

O(x)λ=δWδλ(x)=δSrenosδλ(x).\langle\mathcal O(x)\rangle_\lambda = \frac{\delta W}{\delta\lambda(x)} = \frac{\delta S_{\mathrm{ren}}^{\mathrm{os}}}{\delta\lambda(x)}.

Using the symmetry of KK,

δSrenosδλ(x)=ddyK(x,y)λ(y).\frac{\delta S_{\mathrm{ren}}^{\mathrm{os}}}{\delta\lambda(x)} = \int d^d y\,K(x,y)\lambda(y).

Thus

O(x)λ=ddyK(x,y)λ(y).\langle\mathcal O(x)\rangle_\lambda = \int d^d y\,K(x,y)\lambda(y).

The second derivative of WW is

δ2Wδλ(x)δλ(y)=K(x,y).\frac{\delta^2 W}{\delta\lambda(x)\delta\lambda(y)}=K(x,y).

But with the convention W=logZW=-\log\mathcal Z and S=S0+λOS=S_0+\int\lambda\mathcal O, the connected two-point function is minus the second derivative of WW:

O(x)O(y)c=K(x,y).\langle\mathcal O(x)\mathcal O(y)\rangle_c = - K(x,y).

In other sign conventions, the final sign may be absorbed into the definition of the source coupling or of the generating functional. The invariant statement is that the kernel of the quadratic on-shell action determines the two-point function.