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Stress Tensor, Primaries, and Conformal Transformations

The stress tensor turns the local singularities of a quantum field theory into symmetry transformations. In two dimensions, its two chiral components allow us to compute those transformations by contour integration. This page develops that connection: metric variation fixes the stress tensor, its OPE identifies primary fields, and contour deformation constrains their correlation functions.

Use the global conventions and the contractions, plane normal ordering, and zero-mode qualifications developed on the free-boson page. We work with the covariant matter fields XμX^\mu, before imposing the physical-state conditions. The classical metric constraint motivates those conditions; it does not set the quantum matter operator TXT_X to zero. Ghosts and the total stress tensor enter the later BRST treatment.

From metric variation to a holomorphic stress tensor

Section titled “From metric variation to a holomorphic stress tensor”

Vary the matter action with respect to the inverse Euclidean worldsheet metric. Writing the real coordinates as ξa\xi^a, the variation is

δSE=14πα′∫d2ξ h (∂aX⋅∂bX−12habhcd∂cX⋅∂dX)δhab.\delta S_E=\frac{1}{4\pi\alpha'}\int d^2\xi\,\sqrt h\, \left(\partial_aX\cdot\partial_bX -\frac12h_{ab}h^{cd}\partial_cX\cdot\partial_dX\right)\delta h^{ab}.

The definition of Tab\mathcal T_{ab} in the overview therefore gives

Tab=−12πα′(∂aX⋅∂bX−12habhcd∂cX⋅∂dX).\mathcal T_{ab}=-\frac{1}{2\pi\alpha'} \left(\partial_aX\cdot\partial_bX -\frac12h_{ab}h^{cd}\partial_cX\cdot\partial_dX\right).

Its classical trace vanishes in two dimensions: contracting the first term gives (∂X)2(\partial X)^2, while the trace of the second gives the same quantity. Diffeomorphism invariance gives ∇aTab=0\nabla^a\mathcal T_{ab}=0 on the field equation. These two statements have a particularly strong consequence in a flat complex coordinate patch. Since hzzˉ=hzˉz=2h^{z\bar z}=h^{\bar z z}=2,

Taa=4Tzzˉ=0,∂aTaz=2∂ˉTzz+2∂Tzˉz=0.\mathcal T^a{}_a=4\mathcal T_{z\bar z}=0, \qquad \partial^a\mathcal T_{az} =2\bar\partial\mathcal T_{zz}+2\partial\mathcal T_{\bar z z}=0.

Thus ∂ˉTzz=0\bar\partial\mathcal T_{zz}=0, and the conjugate equation gives ∂Tzˉzˉ=0\partial\mathcal T_{\bar z\bar z}=0. The CFT normalization is T=2πTzzT=2\pi\mathcal T_{zz}, so quantization with the plane subtraction yields

T(z)=−1α′:∂X⋅∂X:,Tˉ(zˉ)=−1α′:∂ˉX⋅∂ˉX:.T(z)=-\frac{1}{\alpha'}:\partial X\cdot\partial X:, \qquad \bar T(\bar z)=-\frac{1}{\alpha'}:\bar\partial X\cdot\bar\partial X:.

The contraction subtracted in defining the composite is proportional to the identity. In this plane vacuum prescription, ⟨T⟩=⟨Tˉ⟩=0\langle T\rangle=\langle\bar T\rangle=0. A change to the cylinder involves a finite vacuum term; it is not obtained by declaring the same subtraction in every coordinate system.

In the quantum theory, holomorphicity means that ∂ˉT=0\bar\partial T=0 inside correlation functions away from insertions. At an insertion there are contact terms, represented equivalently by poles and contour residues. On curved worldsheets there is also a trace anomaly. Neither qualification prevents the flat-patch calculation here, but neither should be discarded when using it elsewhere.

Consider an orientation-preserving change of coordinates

z′=f(z),zˉ′=fˉ(zˉ),f′(z)≠0z'=f(z),\qquad \bar z'=\bar f(\bar z),\qquad f'(z)\ne0

on a patch. For a real Euclidean coordinate change, the barred map is the complex conjugate of the unbarred one. Treating them as independent variables is a convenient complexification when differentiating or computing OPEs.

For the same metric expressed in the new coordinates,

ds2=e2ω(z,zˉ)dz dzˉ=e2ω(z,zˉ)∣f′(z)∣2 dz′ dzˉ′.ds^2=e^{2\omega(z,\bar z)}dz\,d\bar z =\frac{e^{2\omega(z,\bar z)}}{|f'(z)|^2}\,dz'\,d\bar z'.

A Weyl rescaling can restore the chosen conformal-gauge representative. The reciprocal factor in this passive metric formula is consistent with the geometric statement that the map multiplies a tangent displacement by f′(z)f'(z): its absolute value rescales lengths, and its phase rotates all tangents through the same angle. A zero of f′f' invalidates the local coordinate change.

An explicit holomorphic map bends a coordinate grid while preserving the angle and equal scale of two local tangent vectors.

The map f(z)=z+z2/4f(z)=z+z^2/4 is regular on the displayed square. At z0=i/4z_0=i/4, multiplication by f′(z0)=1+i/8f'(z_0)=1+i/8 preserves the right angle and multiplies both tangent lengths by 65/8\sqrt{65}/8. The grids are actual mapped curves; the tangent arrows display the differential, rather than finite grid displacements.

A primary field has a simple local Jacobian law,

ϕ′(z′,zˉ′)=[f′(z)]−h[fˉ′(zˉ)]−hˉϕ(z,zˉ).\phi'(z',\bar z')=[f'(z)]^{-h}[\bar f'(\bar z)]^{-\bar h}\phi(z,\bar z).

The weights (h,hˉ)(h,\bar h) label its response to holomorphic and antiholomorphic changes of scale. Powers of the Jacobian are understood on a consistent local branch. Unlike the number of indices of an ordinary tensor, a quantum weight need not be an integer.

A real dilation z′=λzz'=\lambda z, with λ>0\lambda>0, multiplies the field at corresponding points by λ−Δ\lambda^{-\Delta}, where Δ=h+hˉ\Delta=h+\bar h. A rotation z′=eiθzz'=e^{i\theta}z multiplies it by e−isθe^{-is\theta}, where s=h−hˉs=h-\bar h. These statements explain dimension and spin. Primarity requires the full local transformation law, which is stronger than having definite dimension and spin.

Passive coordinates and an active field variation

Section titled “Passive coordinates and an active field variation”

To keep track of the sign, let z′=z+ϵ(z)z'=z+\epsilon(z). At the same numerical coordinate ww, the old coordinate is z=w−ϵ(w)z=w-\epsilon(w) to first order. Substituting this into the finite law gives

δpassϕ≡ϕ′(w,wˉ)−ϕ(w,wˉ)=−(ϵ∂+h∂ϵ+ϵˉ∂ˉ+hˉ∂ˉϵˉ)ϕ.\delta_{\mathrm{pass}}\phi \equiv\phi'(w,\bar w)-\phi(w,\bar w) =-\left(\epsilon\partial+h\partial\epsilon +\bar\epsilon\bar\partial+\bar h\bar\partial\bar\epsilon\right)\phi.

We will use the opposite, active action for contour generators:

δactϕ=(ϵ∂+h∂ϵ+ϵˉ∂ˉ+hˉ∂ˉϵˉ)ϕ=−δpassϕ.\delta_{\mathrm{act}}\phi =\left(\epsilon\partial+h\partial\epsilon +\bar\epsilon\bar\partial+\bar h\bar\partial\bar\epsilon\right)\phi =-\delta_{\mathrm{pass}}\phi.

Equivalently, the active finite operation at fixed coordinates sends ϕ(z,zˉ)\phi(z,\bar z) to [f′(z)]h[fˉ′(zˉ)]hˉϕ(f(z),fˉ(zˉ))[f'(z)]^h[\bar f'(\bar z)]^{\bar h}\phi(f(z),\bar f(\bar z)). This fixes which transformation the positive residues below generate. Tong’s §§4.2.2–4.2.3 present the Ward construction using the passive variation; comparing the named variations resolves the apparent sign difference.

How a charge becomes a contour around an operator

Section titled “How a charge becomes a contour around an operator”

On the cylinder, a conserved charge inserted just after an operator gives QϕQ\phi; inserted just before it gives ϕQ\phi Q. Their difference is [Q,ϕ][Q,\phi]. Under the cylinder-to-plane map, later Euclidean time becomes larger radius. The commutator is therefore represented by an outer contour minus an inner contour, both originally oriented counterclockwise. If no other insertion lies in the intervening annulus, this difference deforms to a small counterclockwise contour around ϕ\phi.

For holomorphic ϵ\epsilon and antiholomorphic ϵˉ\bar\epsilon, the local conformal charge is

Q[ϵ,ϵˉ]=12πi∮γ[dz ϵ(z)T(z)−dzˉ ϵˉ(zˉ)Tˉ(zˉ)].Q[\epsilon,\bar\epsilon] =\frac{1}{2\pi i}\oint_\gamma \left[dz\,\epsilon(z)T(z)-d\bar z\,\bar\epsilon(\bar z)\bar T(\bar z)\right].

Here γ\gamma is one counterclockwise contour in the physical zz plane. To see why the minus sign matters, parameterize a small circle by z=w+reiθz=w+r e^{i\theta}, 0≤θ≤2π0\le\theta\le2\pi. Then

12πi∮γdzz−w=1,12πi∮γdzˉzˉ−wˉ=−1.\frac{1}{2\pi i}\oint_\gamma\frac{dz}{z-w}=1, \qquad \frac{1}{2\pi i}\oint_\gamma\frac{d\bar z}{\bar z-\bar w}=-1.

The conjugate coordinate goes clockwise. The minus sign in QQ compensates that reversal, so both chiral sectors give positive residues in the active transformation. One may instead orient a separate barred contour counterclockwise in the zˉ\bar z plane, but that is a different contour convention.

Outer minus inner radial contours reduce to a small contour around an insertion; the same physical loop has opposite holomorphic and antiholomorphic residues.

The outer and inner radial contours are both counterclockwise before subtraction. Their difference represents [Q,ϕ][Q,\phi]. A counterclockwise physical loop gives +1+1 for the normalized dz/(z−w)dz/(z-w) integral and −1-1 for its barred counterpart, explaining the charge one-form’s relative minus sign. The contours are schematic and exclude other insertions.

A charge associated with a vector field regular only on a patch should be used locally. A globally defined symmetry charge requires the vector field and integration domain to respect the global geometry and any boundaries.

The primary OPE follows from the charge action

Section titled “The primary OPE follows from the charge action”

Suppose the holomorphic singular part is

T(z)ϕ(w,wˉ)∼∑k≥1Ak(w,wˉ)(z−w)k.T(z)\phi(w,\bar w) \sim\sum_{k\ge1}\frac{A_k(w,\bar w)}{(z-w)^k}.

Taylor expanding ϵ(z)\epsilon(z) and performing the small contour gives

[Q[ϵ,0],ϕ]=∑k≥1∂k−1ϵ(w)(k−1)!Ak(w,wˉ).[Q[\epsilon,0],\phi] =\sum_{k\ge1}\frac{\partial^{k-1}\epsilon(w)}{(k-1)!}A_k(w,\bar w).

For a primary, the active law contains ϵ\epsilon and ∂ϵ\partial\epsilon, but no higher derivative of an arbitrary local ϵ\epsilon. Comparing their coefficients determines the OPE:

T(z)ϕ(w,wˉ)∼hϕ(w,wˉ)(z−w)2+∂ϕ(w,wˉ)z−w.T(z)\phi(w,\bar w) \sim\frac{h\phi(w,\bar w)}{(z-w)^2} +\frac{\partial\phi(w,\bar w)}{z-w}.

The barred formula replaces h,∂,z,wh,\partial,z,w by their barred counterparts. Conversely, these two OPEs reproduce the infinitesimal primary law. The simple pole moves the insertion; the double pole changes the field by its local Jacobian weight. Higher poles would generate additional derivatives of ϵ\epsilon and require a more general transformation law.

Free fields, descendants, and the special status of X

Section titled “Free fields, descendants, and the special status of X”

There are two possible contractions between the fields in TT and an external ∂Xμ\partial X^\mu. Wick’s theorem gives

T(z)∂Xμ(w)∼−2α′[−α′2(z−w)2]∂Xμ(z)=∂Xμ(z)(z−w)2.T(z)\partial X^\mu(w) \sim-\frac{2}{\alpha'} \left[-\frac{\alpha'}{2(z-w)^2}\right]\partial X^\mu(z) =\frac{\partial X^\mu(z)}{(z-w)^2}.

Expanding the uncontracted field at ww is essential: it produces the simple pole as well as the double pole,

T(z)∂Xμ(w)∼∂Xμ(w)(z−w)2+∂2Xμ(w)z−w.T(z)\partial X^\mu(w) \sim\frac{\partial X^\mu(w)}{(z-w)^2} +\frac{\partial^2X^\mu(w)}{z-w}.

Thus ∂Xμ\partial X^\mu is primary of weights (1,0)(1,0), and ∂ˉXμ\bar\partial X^\mu is primary of weights (0,1)(0,1). For the free mixed composite

Oμν=:∂Xμ∂ˉXν:,\mathcal O^{\mu\nu}=:\partial X^\mu\bar\partial X^\nu:,

the two OPE calculations act on the two factors separately, giving (h,hˉ)=(1,1)(h,\bar h)=(1,1). The definition includes the local contact subtraction discussed on the preceding page. There is no mixed pole at separated points. This argument applies to this free composite; arbitrary coincident products do not inherit primary transformation laws merely by adding weights.

For XX itself, contraction instead gives

T(z)Xμ(w,wˉ)∼∂Xμ(w)z−w.T(z)X^\mu(w,\bar w)\sim\frac{\partial X^\mu(w)}{z-w}.

This is the local scalar transformation law. It does not make the unregulated noncompact XX an ordinary weight-zero primary in a conformally invariant vacuum. Its logarithmic contraction changes by an additive constant under dilation, and its unsuppressed target zero mode prevents an unqualified vacuum two-point function. Derivatives remove the additive ambiguity. Properly defined exponentials have their own quantum weights, derived on the next page. The infrared and higher-derivative qualifications are explicit in Tong’s §4.3.3.

The qualification about chirality also matters for target-space Lorentz transformations. For example, the antisymmetric currents

Izμν=:Xμ∂Xν−Xν∂Xμ:,Izˉμν=:Xμ∂ˉXν−Xν∂ˉXμ:I_z^{\mu\nu}=:X^\mu\partial X^\nu-X^\nu\partial X^\mu:, \qquad I_{\bar z}^{\mu\nu}=:X^\mu\bar\partial X^\nu-X^\nu\bar\partial X^\mu:

obey ∂ˉIzμν+∂Izˉμν=0\bar\partial I_z^{\mu\nu}+\partial I_{\bar z}^{\mu\nu}=0 on the free equation away from insertions: differentiating each component gives mixed derivative products which cancel in the sum. A single component need not be holomorphic, because it contains the full field XX. Conservation of a two-dimensional current is a weaker statement than separate conservation of two chiral currents.

Now differentiate the primary OPE with respect to ww. The derivative acts on both fields and denominators, yielding

T(z)∂ϕ(w,wˉ)∼2hϕ(z−w)3+(h+1)∂ϕ(z−w)2+∂2ϕz−w.T(z)\partial\phi(w,\bar w) \sim\frac{2h\phi}{(z-w)^3} +\frac{(h+1)\partial\phi}{(z-w)^2} +\frac{\partial^2\phi}{z-w}.

The derivative has weights (h+1,hˉ)(h+1,\bar h) under dilation and rotation, but for h≠0h\ne0 its third-order pole prevents primarity. For example, ∂2X\partial^2X has weight two and a third-order pole with coefficient 2∂X2\partial X. A field obtained by differentiating a primary is a descendant. The exceptional case h=0h=0 removes this particular third-order obstruction; it does not repair the zero-mode problem of XX.

A primary has only double and simple stress-tensor poles, while its derivative generically has an additional third-order pole.

Differentiation raises the holomorphic weight by one but also produces the pole 2hϕ/(z−w)32h\phi/(z-w)^3. Its contour residue is hϵ′′ϕh\epsilon''\phi. For a nonzero primary with h≠0h\ne0, this extra term distinguishes the descendant from a primary of weight h+1h+1; the barred weight is unchanged.

Let G=⟨∏i=1nϕi(zi,zˉi)⟩G=\langle\prod_{i=1}^n\phi_i(z_i,\bar z_i)\rangle for mutually separated primary insertions. Work in the conformally invariant plane vacuum, or equivalently on the sphere with the vacuum at infinity, without additional boundaries or sources. Subtract from the stress insertion the poles predicted by each local OPE:

F(z)=⟨T(z)∏iϕi⟩−∑i[hi(z−zi)2+1z−zi∂zi]G.F(z)=\left\langle T(z)\prod_i\phi_i\right\rangle -\sum_i\left[\frac{h_i}{(z-z_i)^2} +\frac{1}{z-z_i}\partial_{z_i}\right]G.

This difference has no singularity at any finite insertion and is holomorphic elsewhere. The vacuum condition at infinity makes the first term decay as z−4z^{-4}; the explicit pole sum is at worst O(z−1)O(z^{-1}). Thus FF is an entire function tending to zero at infinity. By Liouville’s theorem, F=0F=0:

⟨T(z)∏iϕi⟩=∑i[hi(z−zi)2+1z−zi∂zi]G.\left\langle T(z)\prod_i\phi_i\right\rangle =\sum_i\left[\frac{h_i}{(z-z_i)^2} +\frac{1}{z-z_i}\partial_{z_i}\right]G.

There is a conjugate Ward identity for Tˉ\bar T. This is an equality of separated-point correlators; its distributional completion includes contact terms at the ziz_i.

Why the z−4z^{-4} condition? In the coordinate u=1/zu=1/z, no operator has been inserted at u=0u=0. The stress tensor is regular there and transforms as a quadratic differential under this Möbius change, giving T(z)=z−4T(u)T(z)=z^{-4}T(u). For free bosons, covariance of the plane subtraction under inversion follows directly from

u′(z)u′(w)[u(z)−u(w)]2=1(z−w)2.\frac{u'(z)u'(w)}{[u(z)-u(w)]^2}=\frac{1}{(z-w)^2}.

For a general local map the subtraction has a finite mismatch: the stress tensor is not itself primary. The associated central term is studied next. Inversion has no such mismatch. We have also specified a vacuum state; a different state or topology can leave a holomorphic contribution that local poles alone do not fix.

Global Ward equations and two-point functions

Section titled “Global Ward equations and two-point functions”

Expanding the pole sum at large zz and setting its z−1z^{-1}, z−2z^{-2}, and z−3z^{-3} coefficients to zero gives

∑i∂ziG=0,∑i(zi∂zi+hi)G=0,∑i(zi2∂zi+2hizi)G=0.\sum_i\partial_{z_i}G=0, \qquad \sum_i(z_i\partial_{z_i}+h_i)G=0, \qquad \sum_i(z_i^2\partial_{z_i}+2h_i z_i)G=0.

These are the translation, dilation/rotation, and special-conformal Ward equations. The barred equations supply the other chiral components. They can also be obtained by integrating TT against 1,z,z21,z,z^2 and moving the contour to infinity. See Ginsparg’s §§2.1 and 2.4 for the relation between these constraints and correlation functions.

For two insertions, translations give G=G(z12,zˉ12)G=G(z_{12},\bar z_{12}), where z12=z1−z2z_{12}=z_1-z_2. The second equation gives

(z12∂z12+h1+h2)G=0,G=C12 z12−h1−h2zˉ12−hˉ1−hˉ2.(z_{12}\partial_{z_{12}}+h_1+h_2)G=0, \qquad G=C_{12}\,z_{12}^{-h_1-h_2}\bar z_{12}^{-\bar h_1-\bar h_2}.

Using this result in the third equation leaves (h1−h2)z12G=0(h_1-h_2)z_{12}G=0. For a nonzero separated correlator, h1=h2=hh_1=h_2=h, and the barred equation similarly requires hˉ1=hˉ2=hˉ\bar h_1=\bar h_2=\bar h. Therefore

⟨ϕ1(z1,zˉ1)ϕ2(z2,zˉ2)⟩=C12z122hzˉ122hˉ.\langle\phi_1(z_1,\bar z_1)\phi_2(z_2,\bar z_2)\rangle =\frac{C_{12}}{z_{12}^{2h}\bar z_{12}^{2\bar h}}.

The constant C12C_{12} is theory- and normalization-dependent; symmetry does not set it to one or make it positive. In particular, the covariant matter theory includes the timelike coordinate. Its two-point bilinear should not be confused with a positive inner product on physical string states.

Why only Möbius maps act globally on the sphere

Section titled “Why only Möbius maps act globally on the sphere”

A local vector field ϵ(z)∂z\epsilon(z)\partial_z must be regular in every chart to generate a global symmetry. Under u=1/zu=1/z its component is

ϵu(u)=dudzϵ(z)=−u2ϵ(1/u).\epsilon_u(u)=\frac{du}{dz}\epsilon(z)=-u^2\epsilon(1/u).

Regularity at finite zz rules out finite poles; regularity at u=0u=0 then restricts the entire function ϵ\epsilon to a polynomial of degree at most two. Hence

ϵ(z)=a0+a1z+a2z2.\epsilon(z)=a_0+a_1z+a_2z^2.

The resulting finite, globally invertible holomorphic maps of the sphere are

f(z)=az+bcz+d,ad−bc≠0.f(z)=\frac{az+b}{cz+d},\qquad ad-bc\ne0.

Their group is PSL(2,C)\mathrm{PSL}(2,\mathbb C): a common nonzero rescaling of the four coefficients changes no map; after setting the determinant to one, an overall sign remains redundant. This gives three complex, or six real, parameters. For real Euclidean coordinate transformations the barred map is conjugate, so it is not a second independent set of three complex parameters. A degree-two rational map is also a map of the sphere, but its branching prevents it from being an invertible coordinate transformation.

Three distinct sphere points can consequently be moved to 0,1,∞0,1,\infty. Four points leave a cross-ratio and therefore genuine functional freedom in a correlator. This distinction will matter when worldsheet symmetries are used to fix insertion positions in string amplitudes.

Exercise 1. Determine the stress normalization from a metric response

Section titled “Exercise 1. Determine the stress normalization from a metric response”

For one spacelike scalar, work on a unit coordinate-area patch with the classical profile X=ux+vyX=ux+vy, where u,vu,v are constant target-length parameters. Vary the inverse metric through hab=diag⁡(1+λ,1−λ)h^{ab}=\operatorname{diag}(1+\lambda,1-\lambda). Compute dSE/dλdS_E/d\lambda at zero directly, recover Txx−Tyy\mathcal T_{xx}-\mathcal T_{yy}, and compare the resulting TT with the free-field expression. Then use X=ℓ(x2−y2)X=\ell(x^2-y^2) to check holomorphicity explicitly, where ℓ\ell is a constant target length and x,yx,y are dimensionless worldsheet coordinates.

Solution

The determinant of the covariant metric is (1−λ2)−1(1-\lambda^2)^{-1}, so the action for the linear profile is

SE(λ)=(1+λ)u2+(1−λ)v24πα′1−λ2,SE′(0)=u2−v24πα′.S_E(\lambda)=\frac{(1+\lambda)u^2+(1-\lambda)v^2} {4\pi\alpha'\sqrt{1-\lambda^2}}, \qquad S_E'(0)=\frac{u^2-v^2}{4\pi\alpha'}.

The stress definition gives SE′(0)=−12(Txx−Tyy)S_E'(0)=-\tfrac12(\mathcal T_{xx}-\mathcal T_{yy}). Directly,

Txx=−u2−v24πα′,Tyy=u2−v24πα′,Txy=−uv2πα′.\mathcal T_{xx}=-\frac{u^2-v^2}{4\pi\alpha'}, \quad \mathcal T_{yy}=\frac{u^2-v^2}{4\pi\alpha'}, \quad \mathcal T_{xy}=-\frac{uv}{2\pi\alpha'}.

Changing tensor components, rather than identifying real and complex components, gives

Tzz=14(Txx−Tyy−2iTxy)=−(u−iv)28πα′,2πTzz=−(∂X)2α′.\mathcal T_{zz}=\frac14(\mathcal T_{xx}-\mathcal T_{yy}-2i\mathcal T_{xy}) =-\frac{(u-iv)^2}{8\pi\alpha'}, \qquad 2\pi\mathcal T_{zz}=-\frac{(\partial X)^2}{\alpha'}.

For the quadratic profile, ∂X=ℓz\partial X=\ell z, hence T=−ℓ2z2/α′T=-\ell^2z^2/\alpha' and ∂ˉT=0\bar\partial T=0. This profile solves the Laplace equation. The qualification is necessary: the off-shell profile X=ℓ(x2+y2)X=\ell(x^2+y^2) instead has ∂X=ℓzˉ\partial X=\ell\bar z and ∂ˉT=−2ℓ2zˉ/α′≠0\bar\partial T=-2\ell^2\bar z/\alpha'\ne0. Tracelessness of the classical expression alone does not imply conservation for an arbitrary off-shell field.

Exercise 2. Recover a complete target-space translation

Section titled “Exercise 2. Recover a complete target-space translation”

On a physical counterclockwise contour define the target momentum operator by

Pμ=12πi∮γ[dz jμ(z)−dzˉ jˉμ(zˉ)],jμ=iα′∂Xμ,jˉμ=iα′∂ˉXμ.P^\mu=\frac{1}{2\pi i}\oint_\gamma \left[dz\,j^\mu(z)-d\bar z\,\bar j^\mu(\bar z)\right], \qquad j^\mu=\frac{i}{\alpha'}\partial X^\mu, \quad \bar j^\mu=\frac{i}{\alpha'}\bar\partial X^\mu.

Compute its commutator with XνX^\nu and the transformation δaXν=iaμ[Pμ,Xν]\delta_a X^\nu=i a_\mu[P^\mu,X^\nu]. Explain what goes wrong if the barred minus sign is omitted or if only one chiral sector is kept. Check the normalization against the noncompact closed-string zero mode.

Solution

Differentiating the logarithmic contraction gives

jμ(z)Xν(w,wˉ)∼−iημν2(z−w),jˉμ(zˉ)Xν(w,wˉ)∼−iημν2(zˉ−wˉ).j^\mu(z)X^\nu(w,\bar w)\sim-\frac{i\eta^{\mu\nu}}{2(z-w)}, \qquad \bar j^\mu(\bar z)X^\nu(w,\bar w) \sim-\frac{i\eta^{\mu\nu}}{2(\bar z-\bar w)}.

The holomorphic normalized integral contributes −iημν/2-i\eta^{\mu\nu}/2. The barred normalized integral before the charge’s extra minus sign contributes +iημν/2+i\eta^{\mu\nu}/2. Thus

[Pμ,Xν]=−iημν,δaXν=aν.[P^\mu,X^\nu]=-i\eta^{\mu\nu}, \qquad \delta_a X^\nu=a^\nu.

Omitting the relative minus sign would make the two contributions cancel. Keeping only the holomorphic charge gives half the translation with the displayed normalization. Here the conventional Hermitian momentum generates a translation through i[P,X]i[P,X]; the conformal Q[ϵ,ϵˉ]Q[\epsilon,\bar\epsilon] above was defined directly by its active commutator, without an extra ii.

The noncompact closed-string expansion has

∂Xμ(z)=−iα′2∑nαnμz−n−1,α0μ=α~0μ=α′2 pμ.\partial X^\mu(z)=-i\sqrt{\frac{\alpha'}2} \sum_n\alpha_n^\mu z^{-n-1}, \qquad \alpha_0^\mu=\tilde\alpha_0^\mu=\sqrt{\frac{\alpha'}2}\,p^\mu.

The two integrals extract α0μ/2α′\alpha_0^\mu/\sqrt{2\alpha'} and α~0μ/2α′\tilde\alpha_0^\mu/\sqrt{2\alpha'}, respectively. Their sum is pμp^\mu, as required. This last equality uses the unwound noncompact zero mode; it is not a general equality of the two chiral fields.

Exercise 3. A descendant under a genuinely local map

Section titled “Exercise 3. A descendant under a genuinely local map”

Starting from the finite primary law, derive the transformation of ∂ϕ\partial\phi. Compare it with the stress OPE of ∂ϕ\partial\phi. As a concrete test take a holomorphic primary of weight one, f(z)=z+λz2f(z)=z+\lambda z^2, and evaluate the transformed derivative at z=z′=0z=z'=0. Why would testing translations and dilations alone miss the result?

Solution

For the holomorphic derivative, use ∂z′=(f′)−1∂z\partial_{z'}=(f')^{-1}\partial_z while holding zˉ′\bar z' fixed:

∂z′ϕ′(z′,zˉ′)=(f′)−h−1(fˉ′)−hˉ[∂ϕ−hf′′f′ϕ].\partial_{z'}\phi'(z',\bar z') =(f')^{-h-1}(\bar f')^{-\bar h} \left[\partial\phi-h\frac{f''}{f'}\phi\right].

The extra term is absent from the primary law of weight (h+1,hˉ)(h+1,\bar h). For f(z)=z+ϵ(z)f(z)=z+\epsilon(z), expansion at fixed numerical coordinates gives

δpass(∂ϕ)=−ϵ∂2ϕ−(h+1)ϵ′∂ϕ−hϵ′′ϕ−ϵˉ∂ˉ∂ϕ−hˉϵˉ′∂ϕ.\delta_{\mathrm{pass}}(\partial\phi) =-\epsilon\partial^2\phi-(h+1)\epsilon'\partial\phi-h\epsilon''\phi -\bar\epsilon\bar\partial\partial\phi -\bar h\bar\epsilon'\partial\phi.

The contour OPE gives the negative of this expression. In particular, the third-order pole contributes (2hϕ)ϵ′′/2=hϵ′′ϕ(2h\phi)\epsilon''/2=h\epsilon''\phi, including the factorial from Taylor expansion.

At the origin in the stated weight-one example, f′=1f'=1 and f′′=2λf''=2\lambda, so

∂z′ϕ′(0)=∂ϕ(0)−2λϕ(0).\partial_{z'}\phi'(0)=\partial\phi(0)-2\lambda\phi(0).

A weight-two primary would give only ∂ϕ(0)\partial\phi(0). Translations and dilations have f′′=0f''=0, so they do not detect this failure. Applying the result to ϕ=∂Xμ\phi=\partial X^\mu yields the nonprimary transformation of ∂2Xμ\partial^2X^\mu. For a genuine h=0h=0 primary, this derivative does pass the holomorphic primary test; XX itself still requires the infrared qualification in the main text.

Exercise 4. One-point functions and the logarithmic scalar

Section titled “Exercise 4. One-point functions and the logarithmic scalar”

In a translation-, dilation-, and rotation-invariant plane vacuum, determine when a primary can have a nonzero one-point function. Does symmetry alone show that every nonidentity primary has zero expectation? Compare the two-point constraints with both ∂Xμ\partial X^\mu and the formal logarithmic XμXνX^\mu X^\nu contraction.

Solution

Translations first give ⟨ϕ(z,zˉ)⟩=A\langle\phi(z,\bar z)\rangle=A, a constant. Dilations require A=λ−ΔAA=\lambda^{-\Delta}A for every positive λ\lambda, so ΔA=0\Delta A=0. Rotations similarly give sA=0sA=0. A nonzero AA therefore requires h=hˉ=0h=\bar h=0. Translation invariance by itself does not force A=0A=0.

The conformal Ward identities leave AA arbitrary for a weight-zero primary. Concluding that only the identity can occur needs extra information about the theory and its vacuum, such as the absence of other independent weight-zero vacuum states. Those assumptions are not part of the local OPE.

For the derivative fields, the two-point result takes the form

⟨∂Xμ(z)∂Xν(w)⟩=Cμν(z−w)2,Cμν=−α′2ημν.\langle\partial X^\mu(z)\partial X^\nu(w)\rangle =\frac{C^{\mu\nu}}{(z-w)^2}, \qquad C^{\mu\nu}=-\frac{\alpha'}2\eta^{\mu\nu}.

This is exactly the free contraction, with its normalization and target tensor retained. In contrast, under a simultaneous real dilation of both arguments, the regulated logarithmic contraction changes by

−α′2ημνlog⁡∣λ(z−w)∣2=−α′2ημνlog⁡∣z−w∣2−α′ημνlog⁡λ.-\frac{\alpha'}2\eta^{\mu\nu}\log|\lambda(z-w)|^2 =-\frac{\alpha'}2\eta^{\mu\nu}\log|z-w|^2 -\alpha'\eta^{\mu\nu}\log\lambda.

It is not the constant two-point function required of two ordinary weight-zero primaries. An arbitrary infrared additive constant does not solve this covariance requirement for every dilation while preserving a fixed vacuum prescription. This illustrates why the local scalar TXTX OPE must be distinguished from a globally well-defined primary state and correlator.

Exercise 5. Check a Ward identity by independent Wick contractions

Section titled “Exercise 5. Check a Ward identity by independent Wick contractions”

For one spacelike scalar define the normalized current J=i2/α′ ∂XJ=i\sqrt{2/\alpha'}\,\partial X, so that ⟨J(z)J(w)⟩=(z−w)−2\langle J(z)J(w)\rangle=(z-w)^{-2} and T=12:JJ:T=\tfrac12:JJ:. Compute ⟨T(z)J(z1)J(z2)⟩\langle T(z)J(z_1)J(z_2)\rangle directly and from the Ward identity. Then extend the argument to four current insertions, exhibiting the terms and their combinatorial factors.

Solution

Normal ordering removes the self-contraction inside TT. Its two currents must contract with the two external currents. There are two assignments, cancelling the factor 1/21/2, so

⟨T(z)J(z1)J(z2)⟩=1(z−z1)2(z−z2)2.\langle T(z)J(z_1)J(z_2)\rangle =\frac{1}{(z-z_1)^2(z-z_2)^2}.

Let a=z−z1a=z-z_1, b=z−z2b=z-z_2, and d=z1−z2=b−ad=z_1-z_2=b-a. The Ward expression, using weight one for each current, is

1d2(1a2+1b2)−2d3(1a−1b)=(b−a)2a2b2d2=1a2b2.\frac{1}{d^2}\left(\frac1{a^2}+\frac1{b^2}\right) -\frac2{d^3}\left(\frac1a-\frac1b\right) =\frac{(b-a)^2}{a^2b^2d^2} =\frac1{a^2b^2}.

The simple-pole derivative terms are indispensable for this cancellation.

For four currents write cab=(za−zb)−2c_{ab}=(z_a-z_b)^{-2}. Wick’s theorem gives three pairings,

G4=⟨J1J2J3J4⟩=c12c34+c13c24+c14c23.G_4=\langle J_1J_2J_3J_4\rangle =c_{12}c_{34}+c_{13}c_{24}+c_{14}c_{23}.

To include TT, choose any unordered pair {a,b}\{a,b\} of external currents to contract with it. The remaining two labels are {c,d}\{c,d\}. There are six choices and two assignments within each choice; again the assignments cancel 1/21/2. Therefore

⟨T(z)J1J2J3J4⟩=∑1≤a<b≤4ccd(z−za)2(z−zb)2,{c,d}={1,2,3,4}∖{a,b}.\langle T(z)J_1J_2J_3J_4\rangle =\sum_{1\le a<b\le4} \frac{c_{cd}}{(z-z_a)^2(z-z_b)^2}, \qquad \{c,d\}=\{1,2,3,4\}\setminus\{a,b\}.

Acting with the Ward differential operator on each of the three products in G4G_4 gives two contributions: it acts on either pair. The two-current identity just proved turns each contribution into one term of the six-term Wick result. This checks the four-point Ward identity without assuming it in the Wick calculation. Each term decays as z−4z^{-4}, also checking the vacuum condition at infinity.

Exercise 6. The sphere, three points, and the remaining cross-ratio

Section titled “Exercise 6. The sphere, three points, and the remaining cross-ratio”

Show that a vector field zn∂zz^n\partial_z, with integer nn, is regular on the sphere only for n=0,1,2n=0,1,2. Construct a Möbius map taking three distinct finite points z1,z2,z3z_1,z_2,z_3 to 0,1,∞0,1,\infty. Derive the coordinate dependence of a three-point primary correlator and explain why four points are different.

Solution

Regularity at z=0z=0 requires n≥0n\ge0. In the infinity chart,

zn∂z=−u2−n∂u,z^n\partial_z=-u^{2-n}\partial_u,

so regularity at u=0u=0 requires n≤2n\le2. This proves the three-generator statement directly. Exponentiating their flows gives translations, rescalings, and maps z↦z/(1−tz)z\mapsto z/(1-tz), which together generate the Möbius group.

The required map is

f(z)=(z−z1)(z2−z3)(z−z3)(z2−z1).f(z)=\frac{(z-z_1)(z_2-z_3)}{(z-z_3)(z_2-z_1)}.

The zero, value one, and pole are immediate. The pole at z3z_3 is regular as a map to the target’s infinity chart; it is not a branch point. Distinctness of the three points ensures a nonzero determinant.

Translations and dilations suggest writing the holomorphic factor of a three-point function as z12−az13−bz23−cz_{12}^{-a}z_{13}^{-b}z_{23}^{-c}. The special-conformal Ward equation fixes the three exponents by

a+b=2h1,a+c=2h2,b+c=2h3.a+b=2h_1,\qquad a+c=2h_2,\qquad b+c=2h_3.

For example, the contribution of z12−az_{12}^{-a} to the special-conformal derivative is −a(z1+z2)-a(z_1+z_2); gathering the coefficient of each ziz_i gives these equations. Their solution is a=h1+h2−h3a=h_1+h_2-h_3, b=h1+h3−h2b=h_1+h_3-h_2, c=h2+h3−h1c=h_2+h_3-h_1. The barred equations work independently. Thus, defining aij=hi+hj−hka_{ij}=h_i+h_j-h_k with kk the remaining label,

⟨ϕ1ϕ2ϕ3⟩=C123∏i<jzij−aijzˉij−aˉij.\langle\phi_1\phi_2\phi_3\rangle =C_{123}\prod_{i<j}z_{ij}^{-a_{ij}}\bar z_{ij}^{-\bar a_{ij}}.

Branches and any exchange phases are fixed consistently for the chosen local fields. There is no additional position-dependent invariant of three distinct sphere points: the displayed map sends every such triple to the same reference triple. Hence the power-law ansatz loses no functional freedom. The constant C123C_{123} is dynamical data, not fixed by conformal symmetry.

A fourth point maps to a nontrivial number f(z4)f(z_4). Equivalently, the cross-ratio

χ=z12z34z13z24\chi=\frac{z_{12}z_{34}}{z_{13}z_{24}}

is unchanged by a Möbius map: each difference transforms with the same determinant and two denominator factors, which cancel in the ratio. Consequently a four-point correlator can retain a function of χ,χˉ\chi,\bar\chi after its required Jacobian factors are extracted. Local conformal symmetry supplies further tools, but global covariance alone does not determine that function.

  • Paul Ginsparg, “Applied Conformal Field Theory,” in Fields, Strings and Critical Phenomena, Les Houches, Session XLIX (1988), edited by É. Brézin and J. Zinn-Justin (North-Holland, 1989), pp. 1–168; arXiv:hep-th/9108028. §§2.1–2.4 develop primary correlators, free-field examples, and contour Ward identities.
  • David Tong, Lectures on String Theory (2009), arXiv:0908.0333. §§4.2.2–4.2.3 derive the local Ward identities and primary transformation law; §4.3.3 checks free-boson primaries and higher derivatives. His passive variation and the active variation defined here differ by the explicitly stated sign.