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Vertex Operators, OPEs, and the Virasoro Algebra

A string’s spacetime momentum and polarization become local worldsheet operators. Their stress-tensor OPEs determine whether they can represent physical external states. The same method, applied to two stress tensors, produces the Virasoro algebra and its central charge. This page derives both results and explains why an oscillator expansion can contain several conformal families.

Use the global conventions, the free-field contractions and normal ordering from page 10, and the active contour action from page 11. We study the flat bosonic matter theory. Local contractions are understood with the earlier zero-mode and infrared prescription; they are not unqualified vacuum correlators of the noncompact field XX.

Exponential vertices and their quantum weights

Section titled “Exponential vertices and their quantum weights”

Define the momentum-carrying operator

Vk(w,wˉ)=:eik⋅X(w,wˉ):.V_k(w,\bar w)=:e^{ik\cdot X(w,\bar w)}:.

Here kk has inverse-length units, so k⋅Xk\cdot X and α′k2\alpha'k^2 are dimensionless. The colons subtract self-contractions within the operator. They do not remove contractions with another insertion. Expand the exponential and contract one field with ∂Xμ(z)\partial X^\mu(z). In the term with rr powers of k⋅Xk\cdot X, there are rr choices, converting 1/r!1/r! into 1/(r−1)!1/(r-1)!. Resumming gives

∂Xμ(z)Vk(w,wˉ)∼−iα′2kμz−wVk(w,wˉ).\partial X^\mu(z)V_k(w,\bar w) \sim-\frac{i\alpha'}2\frac{k^\mu}{z-w}V_k(w,\bar w).

Now insert T=−:∂X⋅∂X:/α′T=-:\partial X\cdot\partial X:/\alpha'. Two kinds of cross-contraction can be singular. Contracting both fields in TT with the exponential gives

−1α′(−iα′2)2k2(z−w)2Vk=α′k24Vk(z−w)2.-\frac1{\alpha'}\left(-\frac{i\alpha'}2\right)^2 \frac{k^2}{(z-w)^2}V_k =\frac{\alpha'k^2}{4}\frac{V_k}{(z-w)^2}.

There is no extra factor of two here: the two identical exponential contractions have already been counted by its power-series coefficients. For a single contraction there are two choices of stress-tensor field. Their contribution is

ikμz−w:∂Xμ(z)eik⋅X(w,wˉ):=∂Vk(w,wˉ)z−w+O(1).\frac{i k_\mu}{z-w}:\partial X^\mu(z)e^{ik\cdot X(w,\bar w)}: =\frac{\partial V_k(w,\bar w)}{z-w}+O(1).

The last equality Taylor expands the uncontracted field about ww and uses ∂Vk=:ik⋅∂Xeik⋅X:\partial V_k=:i k\cdot\partial X e^{ik\cdot X}:. Consequently

T(z)Vk(w,wˉ)∼hkVk(w,wˉ)(z−w)2+∂Vk(w,wˉ)z−w,hk=α′k24.T(z)V_k(w,\bar w) \sim\frac{h_kV_k(w,\bar w)}{(z-w)^2} +\frac{\partial V_k(w,\bar w)}{z-w}, \qquad h_k=\frac{\alpha'k^2}{4}.

The barred calculation gives hˉk=hk\bar h_k=h_k. There are no higher poles: the exponential is a primary, not merely an operator with a particular scaling dimension. Its weight is a quantum effect of contractions, and need not be positive in the covariant theory with a timelike coordinate. Tong’s §4.3.3 develops this free-field calculation.

CFT operators and physical string insertions

Section titled “CFT operators and physical string insertions”

The local CFT operator VkV_k exists for general allowed kk; imposing a string mass shell is an additional step. For an integrated bosonic closed-string matter insertion ∫d2z U\int d^2z\,U, coordinate invariance requires UU to be a primary of weights (1,1)(1,1). Indeed, under a regular local map the measure supplies f′fˉ′f'\bar f', while a primary supplies (f′)−h(fˉ′)−hˉ(f')^{-h}(\bar f')^{-\bar h}.

For the exponential alone, the condition is

hk=hˉk=1,k2=4α′,M2=−4α′.h_k=\bar h_k=1, \qquad k^2=\frac4{\alpha'}, \qquad M^2=-\frac4{\alpha'}.

This is the bosonic closed-string tachyon. A fixed-position, unintegrated representative instead includes the reparametrization ghosts, cc~ Uc\widetilde c\,U, whose weights are then (0,0)(0,0). Physical states also require the gauge quotient and consistency of the total matter-plus-ghost theory. These statements describe the usual on-shell bosonic construction; they are not a claim that every local CFT operator is physical or that all superstring pictures obey the same matter-only rule. The BRST page supplies the cohomological formulation.

For a Neumann open-string boundary, the image contraction doubles ∂X(z)X(t)\partial X(z)X(t) at the real insertion tt. Thus ∂X(z)Vk(t)∼−iα′kVk/(z−t)\partial X(z)V_k(t)\sim-i\alpha'kV_k/(z-t), and the double stress contraction gives boundary weight hbdry=α′k2h_{\rm bdry}=\alpha'k^2. An integrated boundary vertex uses ∫dt\int dt and weight one. The resulting open-string tachyon has M2=−1/α′M^2=-1/\alpha'. This factor of four relative to the bulk holomorphic weight follows from the doubled contraction squared, not a different value of α′\alpha'. See Tong’s §§5.4–5.4.2 for the distinction between the two constructions.

Consider a jointly normal-ordered tensor insertion,

Uϵ(k)=ϵμν:∂Xμ∂ˉXνeik⋅X:.U_\epsilon(k)=\epsilon_{\mu\nu} :\partial X^\mu\bar\partial X^\nu e^{ik\cdot X}:.

Joint normal ordering matters because the derivative fields and exponential occupy the same point. Adding their individual weights identifies the double poles, but does not test for higher ones.

A useful intermediate operator is Wa(p)=:a⋅∂Xeip⋅X:W_a(p)=:a\cdot\partial X e^{ip\cdot X}:, with constant aa. In T(z)Wa(w)T(z)W_a(w), contract one field in TT with a⋅∂Xa\cdot\partial X and the other with the exponential. There are two assignments. Their total is

−2α′(−α′2aμ(z−w)2)(−iα′2pμz−w)Vp=−iα′2a⋅p(z−w)3Vp.-\frac2{\alpha'} \left(-\frac{\alpha'}2\frac{a_\mu}{(z-w)^2}\right) \left(-\frac{i\alpha'}2\frac{p^\mu}{z-w}\right)V_p =-\frac{i\alpha'}2\frac{a\cdot p}{(z-w)^3}V_p.

The remaining contractions and the Taylor expansion give

T(z)Wa(w)∼−iα′(a⋅p)Vp2(z−w)3+(hp+1)Wa(z−w)2+∂Waz−w.T(z)W_a(w) \sim-\frac{i\alpha'(a\cdot p)V_p}{2(z-w)^3} +\frac{(h_p+1)W_a}{(z-w)^2} +\frac{\partial W_a}{z-w}.

Thus WaW_a is holomorphically primary exactly when a⋅p=0a\cdot p=0, apart from an identically vanishing operator. The tensor calculation has the same mixed double contraction, with the uncontracted barred derivative as a spectator:

T(z)Uϵ(w,wˉ)∼−iα′kμϵμν2(z−w)3:∂ˉXνeik⋅X:+(1+hk)Uϵ(z−w)2+∂Uϵz−w.\begin{aligned} T(z)U_\epsilon(w,\bar w)\sim{}& -\frac{i\alpha' k^\mu\epsilon_{\mu\nu}}{2(z-w)^3} :\bar\partial X^\nu e^{ik\cdot X}:\\ &+\frac{(1+h_k)U_\epsilon}{(z-w)^2} +\frac{\partial U_\epsilon}{z-w}. \end{aligned}

The barred third-order pole has coefficient −iα′ϵμνkν:∂Xμeik⋅X:/2-i\alpha'\epsilon_{\mu\nu}k^\nu:\partial X^\mu e^{ik\cdot X}:/2. At separated points there is no holomorphic contraction with ∂ˉX\bar\partial X; the coincident contact subtraction is already part of the composite’s definition. Therefore the conditions for this massless matter vertex are

k2=0,kμϵμν=0,ϵμνkν=0.k^2=0, \qquad k^\mu\epsilon_{\mu\nu}=0, \qquad \epsilon_{\mu\nu}k^\nu=0.

They reproduce the oscillator constraints of page 7. The physical polarization also has the equivalence

ϵμν∼ϵμν+kμλν+λ~μkν,k⋅λ=k⋅λ~=0.\epsilon_{\mu\nu}\sim\epsilon_{\mu\nu} +k_\mu\lambda_\nu+\widetilde\lambda_\mu k_\nu, \qquad k\cdot\lambda=k\cdot\widetilde\lambda=0.

For example, away from contacts, Ukλ=−i∂:λ⋅∂ˉXeik⋅X:U_{k\lambda}=-i\partial:\lambda\cdot\bar\partial X e^{ik\cdot X}:. It is a total derivative in the integrated description. Decoupling in amplitudes requires the usual treatment of other punctures, moduli boundaries, and BRST-exact states; a local total derivative is not a license to discard arbitrary contact contributions. The transverse symmetric traceless, antisymmetric, and trace polarizations describe the graviton, antisymmetric tensor, and dilaton. The trace is taken in the physical transverse space, not by assuming ϵμν∝ημν\epsilon_{\mu\nu}\propto\eta_{\mu\nu} is transverse.

Exponential fusion contains more than one conformal family

Section titled “Exponential fusion contains more than one conformal family”

Wick’s theorem resums all cross-contractions between two exponentials:

Vk(z,zˉ)Vq(w,wˉ)=∣z−w∣α′k⋅q:eik⋅X(z,zˉ)+iq⋅X(w,wˉ):.V_k(z,\bar z)V_q(w,\bar w) =|z-w|^{\alpha'k\cdot q} :e^{ik\cdot X(z,\bar z)+iq\cdot X(w,\bar w)}:.

This is a local free-field identity in radially ordered correlators, with the prescribed contractions. To expand it about ww, write δ=z−w\delta=z-w and p=k+qp=k+q. The first terms are

Vk(z,zˉ)Vq(w,wˉ)=∣δ∣α′k⋅q[Vp+iδ:k⋅∂Xeip⋅X:+iδˉ:k⋅∂ˉXeip⋅X:+O(δ2,δδˉ,δˉ2)].\begin{aligned} V_k(z,\bar z)V_q(w,\bar w) =|\delta|^{\alpha'k\cdot q}\bigl[&V_p +i\delta:k\cdot\partial X e^{ip\cdot X}:\\ &+i\bar\delta:k\cdot\bar\partial X e^{ip\cdot X}: +O(\delta^2,\delta\bar\delta,\bar\delta^2)\bigr]. \end{aligned}

Every term carries momentum pp. The tower is built by the free-boson, or Heisenberg, oscillators acting on that momentum sector. It need not be a single Virasoro family, which is generated from one primary by negative stress-tensor modes.

The distinction is already visible in the first holomorphic term. If p2≠0p^2\ne0, decompose

k=k⋅pp2p+k⊥,k⊥⋅p=0.k=\frac{k\cdot p}{p^2}p+k_\perp, \qquad k_\perp\cdot p=0.

Then

i:k⋅∂Xeip⋅X:=k⋅pp2 ∂Vp+i:k⊥⋅∂Xeip⋅X:.i:k\cdot\partial X e^{ip\cdot X}: =\frac{k\cdot p}{p^2}\,\partial V_p +i:k_\perp\cdot\partial X e^{ip\cdot X}:.

The first term is a derivative descendant of VpV_p. The second passes the WaW_a primary test just derived, and has weights (hp+1,hˉp)(h_p+1,\bar h_p). For generic noncollinear momenta in more than one target dimension it is nonzero: another Virasoro family is needed. Orthogonality here uses the target metric; it does not assume a positive Euclidean inner product. When p2=0p^2=0, this projection is unavailable. One should use the unsplit operator and its OPE, not divide by zero. At p=0p=0, for example, ∂V0=0\partial V_0=0 while ik⋅∂Xi k\cdot\partial X can be a nonzero primary current.

The first oscillator term at fixed non-null momentum splits into a Virasoro descendant and an independent transverse primary.

For p=k+qp=k+q with p2≠0p^2\ne0, the component of kk parallel to pp produces ∂Vp\partial V_p. Its metric-orthogonal component produces a primary of weight (hp+1,hˉp)(h_p+1,\bar h_p). Both belong to the same momentum sector, but generically to different Virasoro families. The diagram is an algebraic decomposition, not a picture of positive-norm target-space directions. Higher terms in the OPE can require additional families.

Scaling determines OPE powers, not all coefficients

Section titled “Scaling determines OPE powers, not all coefficients”

Suppose Ai,AjA_i,A_j have definite weights and a local operator OA\mathcal O_A of weights (hA,hˉA)(h_A,\bar h_A) occurs in their product. Under a simultaneous dilation of the separation and insertion point, the left side scales with weight hi+hjh_i+h_j in the holomorphic sector. Covariance therefore fixes its coefficient’s power to δhA−hi−hj\delta^{h_A-h_i-h_j}. The barred argument is independent. A complete operator-basis expansion has the form

Ai(z,zˉ)Aj(w,wˉ)=∑ACijA δhA−hi−hjδˉhˉA−hˉi−hˉjOA(w,wˉ).A_i(z,\bar z)A_j(w,\bar w) =\sum_A C_{ij}{}^A\, \delta^{h_A-h_i-h_j}\bar\delta^{\bar h_A-\bar h_i-\bar h_j} \mathcal O_A(w,\bar w).

The basis includes descendants as well as primaries. If one organizes the sum by primaries, each family must contain its descendant series with the corresponding additional integer powers. In a noncompact theory the primary label may include continuous momentum, with sums replaced by integrals as appropriate. This expression assumes a basis of scaling eigenoperators; logarithmic representation theory needs a more general form.

For the leading exponential, hp−hk−hq=α′k⋅q/2h_p-h_k-h_q=\alpha'k\cdot q/2. Combining holomorphic and barred factors gives precisely ∣δ∣α′k⋅q|\delta|^{\alpha'k\cdot q}. Symmetry fixes such powers, but the primary coefficients remain dynamical data. Relative descendant coefficients can then be constrained by Ward identities.

A full OPE is used inside a correlator with a separating circle containing the fused pair and excluding all other insertions. In the free-field examples its local Taylor series converges within that separation domain, with branches chosen consistently. The symbol ∼\sim below keeps only singular terms relevant to residues; it does not assert that regular terms vanish. Expanding in complete local states also underlies factorization of string amplitudes, but only after the physical-state and ghost prescriptions are included.

Put Aμ=∂XμA^\mu=\partial X^\mu temporarily to expose the contraction counting. The two fields at zz and the two at ww have two complete cross-matchings and four choices of a single cross-contraction. No self-contraction within a stress tensor is allowed. The double contractions give

1α′2 2(α′2)2ημνηρσημρηνσ(z−w)4=D/2(z−w)4.\frac1{\alpha'^2}\,2\left(\frac{\alpha'}2\right)^2 \frac{\eta_{\mu\nu}\eta_{\rho\sigma} \eta^{\mu\rho}\eta^{\nu\sigma}}{(z-w)^4} =\frac{D/2}{(z-w)^4}.

The four single contractions leave a bilocal normal product:

T(z)T(w)∼D/2(z−w)4−2α′(z−w)2:A(z)⋅A(w):.T(z)T(w)\sim\frac{D/2}{(z-w)^4} -\frac{2}{\alpha'(z-w)^2}:A(z)\cdot A(w):.

Taylor expansion supplies both remaining poles:

:A(z)⋅A(w):=−α′T(w)−α′2(z−w)∂T(w)+O((z−w)2).:A(z)\cdot A(w): =-\alpha'T(w)-\frac{\alpha'}2(z-w)\partial T(w)+O((z-w)^2).

We obtain

T(z)T(w)∼c/2(z−w)4+2T(w)(z−w)2+∂T(w)z−w,c=D.T(z)T(w)\sim\frac{c/2}{(z-w)^4} +\frac{2T(w)}{(z-w)^2} +\frac{\partial T(w)}{z-w}, \qquad c=D.

Two complete Wick matchings produce the fourth-order stress pole, while four single pairings leave the operator-valued poles.

The slot numbers label individual fields, not target-space indices, and make the factors two and four explicit. The complete pairings yield D/[2(z−w)4]D/[2(z-w)^4]; the single pairings leave −2:∂X(z)⋅∂X(w):/[α′(z−w)2]-2:\partial X(z)\cdot\partial X(w):/[\alpha'(z-w)^2]. Taylor expansion of that bilocal product gives 2T2T and ∂T\partial T. Lines represent contractions, not propagating worldsheet trajectories.

A timelike boson contributes +1+1 to cc, just as a spacelike one does. The two inverse metrics from contractions multiply the two metrics in the stress tensors to give DD, not D−2D-2. The covariant matter Hilbert space can nevertheless have negative norms. Central charge is not a signature count or a proof of unitarity. The negative central charge of the bcbc ghosts arises from their own statistics and conformal weights.

The fourth-order pole is proportional to the identity, and so is called central. It also proves that TT is not a primary when c≠0c\ne0, even though its weights are (2,0)(2,0). Using the active contour rule of page 11 gives

δactT=ϵ∂T+2(∂ϵ)T+c12∂3ϵ.\delta_{\rm act}T =\epsilon\partial T+2(\partial\epsilon)T +\frac{c}{12}\partial^3\epsilon.

For ϵ=1,z,z2\epsilon=1,z,z^2 the last term vanishes: the stress tensor still transforms covariantly under the global Möbius transformations. Its finite anomalous transformation and the cylinder vacuum shift are developed on the next page. The free-field derivation and its general CFT interpretation are discussed in Tong’s §§4.3.3–4.4 and Ginsparg’s §3.1.

Radial modes and the ordered contour difference

Section titled “Radial modes and the ordered contour difference”

On an annulus around the origin, the Laurent expansion and its inverse are

T(z)=∑n∈ZLnz−n−2,Ln=12πi∮0dz zn+1T(z).T(z)=\sum_{n\in\mathbb Z}L_n z^{-n-2}, \qquad L_n=\frac1{2\pi i}\oint_0 dz\,z^{n+1}T(z).

The contour is counterclockwise. Since increasing radius means later Euclidean cylinder time, LmLnL_mL_n places the zz contour outside the ww contour, while LnLmL_nL_m reverses their radial order.

Fix ∣w∣=r|w|=r, and choose R−<r<R+R_-<r<R_+. The whole commutator is represented by

[Lm,Ln]=1(2πi)2∮∣w∣=rdw wn+1(∮∣z∣=R+−∮∣z∣=R−)dz zm+1R[T(z)T(w)].\begin{aligned} [L_m,L_n]=\frac1{(2\pi i)^2}\oint_{|w|=r}dw\,w^{n+1} \left(\oint_{|z|=R_+}-\oint_{|z|=R_-}\right) dz\,z^{m+1}\mathcal R[T(z)T(w)]. \end{aligned}

Both zz contours are counterclockwise before subtraction; R\mathcal R denotes radial ordering. With no additional insertion in the intervening annulus, their difference deforms to a single small contour around ww. Thus

[Lm,Ln]=1(2πi)2∮0dw wn+1∮wdz zm+1T(z)T(w).[L_m,L_n]=\frac1{(2\pi i)^2} \oint_0dw\,w^{n+1}\oint_wdz\,z^{m+1}T(z)T(w).

There is no further subtraction with mm and nn exchanged. The outer-minus-inner contour has already performed that subtraction. Adding it again would double the answer. This contour operation is described explicitly in Ginsparg’s §3.3 and Tong’s §4.5.2.

The difference of the two radial orderings becomes one local stress-tensor contour around the other insertion.

The two radial orderings are subtracted once. At fixed ww, the remaining zz contour surrounds ww and excludes the origin; the ww contour still surrounds the origin. Every displayed holomorphic contour is counterclockwise. For barred modes on the same physical loop, the barred coordinate runs clockwise and the mode integral needs a minus sign. The radii are schematic and may be deformed without crossing other insertions.

On the small contour about w≠0w\ne0, the function f(z)=zm+1f(z)=z^{m+1} is analytic, even for negative integer mm, provided that contour excludes the origin. Cauchy’s differentiation formula gives

12πi∮wf(z) dz(z−w)r=f(r−1)(w)(r−1)!.\frac1{2\pi i}\oint_w\frac{f(z)\,dz}{(z-w)^r} =\frac{f^{(r-1)}(w)}{(r-1)!}.

Applying it to the fourth-, second-, and first-order stress poles yields

[Lm,Ln]=12πi∮0dw wn+1[c12(m+1)m(m−1)wm−2+2(m+1)wmT(w)+wm+1∂T(w)].\begin{aligned} [L_m,L_n]=\frac1{2\pi i}\oint_0dw\,w^{n+1} \biggl[&\frac{c}{12}(m+1)m(m-1)w^{m-2}\\ &+2(m+1)w^mT(w)+w^{m+1}\partial T(w)\biggr]. \end{aligned}

For the operator terms, integrate the last term by parts on the closed contour:

∮0dw wm+n+2∂T=−(m+n+2)∮0dw wm+n+1T.\oint_0dw\,w^{m+n+2}\partial T =-(m+n+2)\oint_0dw\,w^{m+n+1}T.

Its coefficient combines with 2(m+1)2(m+1) to give m−nm-n. The identity term has the remaining integral ∮dw wm+n−1/(2πi)=δm+n,0\oint dw\,w^{m+n-1}/(2\pi i)=\delta_{m+n,0}. Therefore

[Lm,Ln]=(m−n)Lm+n+c12m(m2−1)δm+n,0.[L_m,L_n]=(m-n)L_{m+n} +\frac{c}{12}m(m^2-1)\delta_{m+n,0}.

This is the Virasoro algebra. The central coefficient is odd in mm on the support n=−mn=-m, as antisymmetry demands. It vanishes for m=−1,0,1m=-1,0,1, so the global conformal generators close without a central term. The cubic polynomial, including its linear subtraction, follows from a third derivative; it is not an arbitrary extra constant.

The vector fields ℓn=−zn+1∂z\ell_n=-z^{n+1}\partial_z obey [ℓm,ℓn]=(m−n)ℓm+n[\ell_m,\ell_n]=(m-n)\ell_{m+n}, the Witt algebra. They provide the geometric algebra to which Virasoro is a central extension. Their sign refers to coordinate vector fields; the positive local residue action on an operator remains [Ln,ϕ]=(zn+1∂+h(n+1)zn)ϕ[L_n,\phi]=(z^{n+1}\partial+h(n+1)z^n)\phi. For the unimproved classical free-boson stress tensor the Poisson-bracket algebra has no such central term. In the quantum calculation above it comes from double contractions. This last statement does not exclude classical central extensions in other, improved systems or boundary charge algebras.

Two chiral algebras and the oscillator construction

Section titled “Two chiral algebras and the oscillator construction”

Using a single counterclockwise physical contour γ\gamma in the zz plane, define

Lˉn=−12πi∮γdzˉ zˉn+1Tˉ(zˉ),Tˉ(zˉ)=∑nLˉnzˉ−n−2.\bar L_n=-\frac1{2\pi i}\oint_\gamma d\bar z\,\bar z^{n+1}\bar T(\bar z), \qquad \bar T(\bar z)=\sum_n\bar L_n\bar z^{-n-2}.

This is equivalent to a positive integral on a separate counterclockwise contour in the zˉ\bar z plane. For z=reiθz=re^{i\theta}, one has dzˉ=−izˉ dθd\bar z=-i\bar z\,d\theta, which verifies the sign directly. The same local residue derivation gives

[Lˉm,Lˉn]=(m−n)Lˉm+n+cˉ12m(m2−1)δm+n,0,[Lm,Lˉn]=0.[\bar L_m,\bar L_n]=(m-n)\bar L_{m+n} +\frac{\bar c}{12}m(m^2-1)\delta_{m+n,0}, \qquad [L_m,\bar L_n]=0.

Here Lˉn\bar L_n is the same antiholomorphic operator denoted L~n\widetilde L_n in the oscillator discussion. For the present free matter theory, cˉ=c=D\bar c=c=D. Mixed holomorphic–antiholomorphic contractions have contact support, not separated chiral poles; the independent chiral oscillator algebras of page 6 commute. The contact distribution in differentiated XX correlators does not generate a mixed Virasoro central term. An open-string boundary instead glues the two chiral components into one mode family.

Substituting the previously derived plane expansion of ∂X\partial X into the stress tensor gives

Ln=12∑r∈Z:αn−r⋅αr:,L0=α′p24+N,N=∑r>0α−r⋅αrL_n=\frac12\sum_{r\in\mathbb Z}:\alpha_{n-r}\cdot\alpha_r:, \qquad L_0=\frac{\alpha' p^2}{4}+N, \qquad N=\sum_{r>0}\alpha_{-r}\cdot\alpha_r

for the unwound noncompact closed string. Normal ordering is the plane prescription: the oscillator vacuum at fixed pp has N=0N=0. The eigenvalue of L0L_0 is a holomorphic weight. Neither a cylinder vacuum shift nor the physical intercept is to be inserted again into this definition. The critical bosonic physical condition is (L0−1)∣phys⟩=0(L_0-1)|\mathrm{phys}\rangle=0, accompanied by the positive-mode constraints and gauge quotient; the independent barred condition gives level matching. The derivation of the total critical theory is separate from the local matter identity c=Dc=D.

Exercise 1. A neutral correlator checks the exponential weights

Section titled “Exercise 1. A neutral correlator checks the exponential weights”

For separated exponential insertions with ∑iki=0\sum_i k_i=0, factor out the momentum delta function and use

G=⟨∏iVki(zi,zˉi)⟩stripped=∏i<j∣zi−zj∣α′ki⋅kj.G=\left\langle\prod_iV_{k_i}(z_i,\bar z_i)\right\rangle_{\rm stripped} =\prod_{i<j}|z_i-z_j|^{\alpha'k_i\cdot k_j}.

Compute ⟨T(z)∏iVki⟩stripped/G\langle T(z)\prod_iV_{k_i}\rangle_{\rm stripped}/G directly by Wick contraction. Show that it equals the primary Ward expression, including the simple-pole terms, and check its large-zz decay. Explain the role of momentum neutrality.

Solution

Each field in TT contracts with the exponential product with coefficient −iα′∑iki/[2(z−zi)]-i\alpha'\sum_i k_i/[2(z-z_i)]. Its two contractions therefore give

⟨T(z)∏iVki⟩strippedG=α′4(∑ikiz−zi)2.\frac{\langle T(z)\prod_iV_{k_i}\rangle_{\rm stripped}}{G} =\frac{\alpha'}4\left(\sum_i\frac{k_i}{z-z_i}\right)^2.

Both fields can contract with the same exponential, or with two different ones; the square includes both possibilities. Expanding it gives diagonal terms hki/(z−zi)2h_{k_i}/(z-z_i)^2 and cross terms

α′2∑i<jki⋅kj(z−zi)(z−zj).\frac{\alpha'}2\sum_{i<j} \frac{k_i\cdot k_j}{(z-z_i)(z-z_j)}.

On the other hand,

∂zilog⁡G=α′2∑j≠iki⋅kjzi−zj.\partial_{z_i}\log G =\frac{\alpha'}2\sum_{j\ne i}\frac{k_i\cdot k_j}{z_i-z_j}.

Combining the i,ji,j contributions to the Ward simple poles uses

1zi−zj(1z−zi−1z−zj)=1(z−zi)(z−zj).\frac1{z_i-z_j}\left(\frac1{z-z_i}-\frac1{z-z_j}\right) =\frac1{(z-z_i)(z-z_j)}.

Thus the Wick result is exactly ∑i[hki/(z−zi)2+(∂zilog⁡G)/(z−zi)]\sum_i[h_{k_i}/(z-z_i)^2+(\partial_{z_i}\log G)/(z-z_i)]. Omitting the simple poles would miss all cross terms.

At infinity the vector in parentheses is

∑ikiz−zi=1z∑iki+1z2∑ikizi+O(z−3).\sum_i\frac{k_i}{z-z_i} =\frac1z\sum_i k_i+\frac1{z^2}\sum_i k_i z_i+O(z^{-3}).

Neutrality removes the first term, so the stress insertion decays as z−4z^{-4}. In the noncompact theory the zero-mode integral enforces precisely that neutrality. A nonneutral expression without an additional charged state at infinity is not the vacuum correlator assumed in this Ward check. The stripped formula is used on the support of the momentum delta function.

Exercise 2. The trace polarization and a pure-gauge vertex

Section titled “Exercise 2. The trace polarization and a pure-gauge vertex”

Let k≠0k\ne0 be null in DD-dimensional Minkowski space, and choose a null reference vector qq with k⋅q=−1k\cdot q=-1. Show that

Πμν=ημν+kμqν+qμkν\Pi_{\mu\nu}=\eta_{\mu\nu}+k_\mu q_\nu+q_\mu k_\nu

gives a transverse massless tensor vertex, while ϵμν=ημν\epsilon_{\mu\nu}=\eta_{\mu\nu} does not. Find the trace of Π\Pi. Next take ϵμν=kμλν\epsilon_{\mu\nu}=k_\mu\lambda_\nu with k⋅λ=0k\cdot\lambda=0 and express its vertex as a derivative. Does the absence of third-order poles alone remove this polarization from the physical spectrum?

Solution

Contraction with kk gives kν+k2qν+(k⋅q)kν=0k_\nu+k^2q_\nu+(k\cdot q)k_\nu=0, and the other contraction vanishes as well. Raising one index shows that Π2=Π\Pi^2=\Pi: it annihilates k,qk,q and acts as the identity on vectors orthogonal to both. Its trace is D+2k⋅q=D−2D+2k\cdot q=D-2.

Hence UΠU_\Pi has weights (1,1)(1,1) and no third-order pole. It represents the transverse trace polarization. In contrast, kμημν=kν≠0k^\mu\eta_{\mu\nu}=k_\nu\ne0, so UηU_\eta fails the primary test despite its double-pole weights. In D=26D=26 the transverse trace contains 24 directions; it is the scalar polarization in the physical 24⊗2424\otimes24 decomposition. A unit-normalized transverse trace tensor is Πμν/24\Pi_{\mu\nu}/\sqrt{24}.

For the second polarization, kμϵμν=k2λν=0k^\mu\epsilon_{\mu\nu}=k^2\lambda_\nu=0 and ϵμνkν=kμ(λ⋅k)=0\epsilon_{\mu\nu}k^\nu=k_\mu(\lambda\cdot k)=0. Thus it also passes the primary test. Using the free equation away from insertions,

∂:λ⋅∂ˉXeik⋅X:=i:k⋅∂X λ⋅∂ˉXeik⋅X:,Ukλ=−i∂:λ⋅∂ˉXeik⋅X:.\partial:\lambda\cdot\bar\partial X e^{ik\cdot X}: =i:k\cdot\partial X\,\lambda\cdot\bar\partial X e^{ik\cdot X}:, \qquad U_{k\lambda}=-i\partial:\lambda\cdot\bar\partial X e^{ik\cdot X}:.

The field being differentiated has holomorphic weight zero, so its derivative has no third-order obstruction. Primarity therefore does not distinguish this pure-gauge insertion from nontrivial physical polarizations. Removing it uses the null-state or BRST quotient. This example separates the mass-shell condition, transversality, and gauge equivalence into three distinct steps.

Exercise 3. A new primary in a fixed momentum sector

Section titled “Exercise 3. A new primary in a fixed momentum sector”

Take two orthonormal spacelike directions e1,e2e_1,e_2, with k=ae1k=a e_1, q=ae2q=a e_2, a≠0a\ne0. Decompose the first holomorphic term in Vk(z)Vq(w)V_k(z)V_q(w) into a derivative of Vk+qV_{k+q} and a separate primary. Independently derive the coefficient of the derivative from global conformal covariance. Finally explain what changes for q=−kq=-k.

Solution

For p=a(e1+e2)p=a(e_1+e_2), one has p2=2a2p^2=2a^2 and k⋅p=a2k\cdot p=a^2. Therefore

i:k⋅∂Xeip⋅X:=12∂Vp+ia2:(∂X1−∂X2)eip⋅X:.i:k\cdot\partial X e^{ip\cdot X}: =\frac12\partial V_p +\frac{ia}{2}:(\partial X^1-\partial X^2)e^{ip\cdot X}:.

The second polarization is orthogonal to pp, so it is primary of weights (hp+1,hp)(h_p+1,h_p), where hp=α′a2/2h_p=\alpha'a^2/2. It is nonzero and cannot be replaced by ∂Vp\partial V_p: the two have different stress third-order poles. In particular, ∂Vp\partial V_p has coefficient 2hpVp2h_pV_p, whereas the new primary has none.

For an independent coefficient check, use holomorphic three-point covariance. Put the fused operators at zz and 00 and their momentum-dual primary V−pV_{-p}, of weight hph_p, at yy. The three momenta now sum to zero. After stripping a common structure constant, its holomorphic dependence is

zhp−hk−hq(z−y)−hk−hp+hq(−y)−hq−hp+hk.z^{h_p-h_k-h_q}(z-y)^{-h_k-h_p+h_q} (-y)^{-h_q-h_p+h_k}.

Expanding in z/yz/y gives relative linear coefficient (hk+hp−hq)z/y(h_k+h_p-h_q)z/y. In an OPE term zhp−hk−hq[Vp(0)+βz∂Vp(0)+⋯ ]z^{h_p-h_k-h_q}[V_p(0)+\beta z\partial V_p(0)+\cdots], differentiation of the two-point factor (w−y)−2hp(w-y)^{-2h_p} at w=0w=0 gives relative 2hp/y2h_p/y. Thus

β=hp+hk−hq2hp=k⋅pp2=12.\beta=\frac{h_p+h_k-h_q}{2h_p} =\frac{k\cdot p}{p^2}=\frac12.

This projects onto the VpV_p family; it does not assert that this is the only family. The separate primary has a different weight and no two-point pairing with VpV_p in the plane vacuum.

If q=−kq=-k, then p=0p=0 and Vp=1V_p=1, so ∂Vp=0\partial V_p=0. The first term of the expansion is still izk⋅∂Xi z k\cdot\partial X, a nonzero weight-one primary for nonzero spacelike kk. It belongs to a current family rather than the identity family. The expression for β\beta cannot be used at hp=0h_p=0. This example makes the failure of a universal single-family interpretation especially explicit.

Exercise 4. Three stress tensors and the timelike sign

Section titled “Exercise 4. Three stress tensors and the timelike sign”

Compute the separated plane-vacuum correlator ⟨T(z1)T(z2)T(z3)⟩\langle T(z_1)T(z_2)T(z_3)\rangle for DD free coordinates by enumerating Wick pairings. Verify its leading OPE as z1→z2z_1\to z_2. Explain why a timelike coordinate contributes with the same sign as a spacelike one.

Solution

There are six fields in total, two at each insertion, and normal ordering forbids an edge joining fields at the same insertion. A complete pairing must join each pair of distinct insertions once: its contraction graph is a triangle. There are eight assignments to the two labeled field slots at each vertex. For one spacelike coordinate, their common factor including the three stress normalizations is

8(−1α′)3(−α′2)3=1.8\left(-\frac1{\alpha'}\right)^3 \left(-\frac{\alpha'}2\right)^3=1.

The target-index contraction around the triangle is the trace of the identity, giving DD. Hence

⟨T1T2T3⟩=Dz122z232z312.\langle T_1T_2T_3\rangle =\frac{D}{z_{12}^2z_{23}^2z_{31}^2}.

For a timelike field each propagator changes sign, but each occurrence of that field in TT also changes sign. There are three of each, so the two sign changes cancel. The coordinate contributes +1+1 to the displayed coefficient.

Let z1=z2+δz_1=z_2+\delta and d=z2−z3d=z_2-z_3. The result expands as

Dδ2d2(d+δ)2=Dδ2d4−2Dδd5+O(1).\frac{D}{\delta^2d^2(d+\delta)^2} =\frac{D}{\delta^2d^4}-\frac{2D}{\delta d^5}+O(1).

The stress OPE predicts 2⟨T2T3⟩/δ2+∂z2⟨T2T3⟩/δ2\langle T_2T_3\rangle/\delta^2+\partial_{z_2}\langle T_2T_3\rangle/\delta. Since ⟨T2T3⟩=D/(2d4)\langle T_2T_3\rangle=D/(2d^4), both terms agree. The fourth-order identity pole multiplies ⟨T3⟩=0\langle T_3\rangle=0 and contributes nothing here. This checks the single-contraction coefficients independently of the two-point central term.

Exercise 5. Residues, negative modes, and a Jacobi check

Section titled “Exercise 5. Residues, negative modes, and a Jacobi check”

Use the single local contour formula to compute [L2,L−2][L_2,L_{-2}] and [L−3,L1][L_{-3},L_1], keeping the integration-by-parts contribution visible. Check the Jacobi identity for modes (2,1,−3)(2,1,-3). What algebra would result if the minus sign in the barred physical-contour definition were omitted?

Solution

For m=2,n=−2m=2,n=-2, the inner residue is c/2+6w2T+w3∂Tc/2+6w^2T+w^3\partial T. Multiplying by w−1w^{-1} and integrating gives

[L2,L−2]=c2+6L0−2L0=4L0+c2.[L_2,L_{-2}]=\frac c2+6L_0-2L_0=4L_0+\frac c2.

The derivative contribution is ∮w2∂T=−2∮wT\oint w^2\partial T=-2\oint wT. Antisymmetrizing this answer again would erroneously give 8L0+c8L_0+c.

For m=−3m=-3, the fourth-pole residue is −2c w−5-2c\,w^{-5}, the second-pole residue is −4w−3T-4w^{-3}T, and the simple-pole residue is w−2∂Tw^{-2}\partial T. With n=1n=1, multiplication by w2w^2 leaves

[L−3,L1]=12πi∮0dw [−2c w−3−4w−1T+∂T]=−4L−2.[L_{-3},L_1]=\frac1{2\pi i}\oint_0dw\, \left[-2c\,w^{-3}-4w^{-1}T+\partial T\right] =-4L_{-2}.

Neither the identity Laurent monomial nor the total derivative has a residue. Negative powers of zz did not obstruct the local Taylor expansion: its center was w≠0w\ne0, and its circle excluded z=0z=0.

The three Jacobi terms are

[L2,[L1,L−3]]=16L0+2c,[L1,[L−3,L2]]=−10L0,[L−3,[L2,L1]]=−6L0−2c.\begin{aligned} [L_2,[L_1,L_{-3}]]&=16L_0+2c,\\ [L_1,[L_{-3},L_2]]&=-10L_0,\\ [L_{-3},[L_2,L_1]]&=-6L_0-2c. \end{aligned}

They sum to zero, including the central parts. This finite check is not a proof of all Jacobi identities, but it would detect several normalization or sign mistakes.

Without the barred minus sign the proposed operators would be Bn=−LˉnB_n=-\bar L_n. They would obey

[Bm,Bn]=−(m−n)Bm+n+cˉ12m(m2−1)δm+n,0.[B_m,B_n]=-(m-n)B_{m+n} +\frac{\bar c}{12}m(m^2-1)\delta_{m+n,0}.

The central coefficient retains its sign because there are two minus signs on the left, while the linear term reverses because expressing the result in terms of BB introduces one more. Thus the error cannot be repaired by simply declaring a negative barred central charge.

Exercise 6. A level-two Gram matrix from the algebra

Section titled “Exercise 6. A level-two Gram matrix from the algebra”

As an algebraic application, take a normalized highest-weight vector satisfying L0∣h⟩=h∣h⟩L_0|h\rangle=h|h\rangle, Ln∣h⟩=0L_n|h\rangle=0 for n>0n>0, and Ln†=L−nL_n^\dagger=L_{-n}, with real c,hc,h. Compute the Gram matrix of L−2∣h⟩L_{-2}|h\rangle and L−12∣h⟩L_{-1}^2|h\rangle. At c=1,h=1/4c=1,h=1/4, find the null combination and verify that positive modes annihilate it. Check its image in the one-spacelike-boson Fock representation with α0=u\alpha_0=u and h=u2/2h=u^2/2.

Solution

Move each positive mode to the right with the commutator. The diagonal first entry is ⟨h∣[L2,L−2]∣h⟩=4h+c/2\langle h|[L_2,L_{-2}]|h\rangle=4h+c/2. For the off-diagonal entry,

L2L−12∣h⟩=3(L1L−1+L−1L1)∣h⟩=6h∣h⟩.L_2L_{-1}^2|h\rangle =3(L_1L_{-1}+L_{-1}L_1)|h\rangle =6h|h\rangle.

For the other diagonal entry, first use

L1L−12∣h⟩=2(L0L−1+L−1L0)∣h⟩=2(2h+1)L−1∣h⟩.L_1L_{-1}^2|h\rangle =2(L_0L_{-1}+L_{-1}L_0)|h\rangle =2(2h+1)L_{-1}|h\rangle.

Applying L1L_1 again gives 4h(2h+1)∣h⟩4h(2h+1)|h\rangle. Therefore

G(2)=(4h+c/26h6h4h(2h+1)).G^{(2)}= \begin{pmatrix} 4h+c/2&6h\\ 6h&4h(2h+1) \end{pmatrix}.

At c=1,h=1/4c=1,h=1/4, all four entries equal 3/23/2. The null vector is

∣χ⟩=(L−2−L−12)∣h⟩.|\chi\rangle=(L_{-2}-L_{-1}^2)|h\rangle.

Its positive-mode conditions follow directly:

L1∣χ⟩=[3−2(2h+1)]L−1∣h⟩=0,L2∣χ⟩=(4h+c/2−6h)∣h⟩=0.L_1|\chi\rangle=[3-2(2h+1)]L_{-1}|h\rangle=0, \qquad L_2|\chi\rangle=(4h+c/2-6h)|h\rangle=0.

Modes n>2n>2 vanish after commutation because every resulting positive mode annihilates ∣h⟩|h\rangle. Thus the null vector is also highest weight in the abstract module, not merely a vector with zero diagonal norm.

For the free boson, the oscillator formula yields

L−2∣u⟩=uα−2∣u⟩+12α−12∣u⟩,L−12∣u⟩=uα−2∣u⟩+u2α−12∣u⟩.L_{-2}|u\rangle =u\alpha_{-2}|u\rangle+\frac12\alpha_{-1}^2|u\rangle, \qquad L_{-1}^2|u\rangle =u\alpha_{-2}|u\rangle+u^2\alpha_{-1}^2|u\rangle.

At h=u2/2=1/4h=u^2/2=1/4, these vectors coincide. The abstract null combination is therefore represented by zero in this Fock realization. A Virasoro module and its independent physical states must not be counted by listing descendant symbols alone. This is a small example of the representation theory developed on page 14; it is not a general no-ghost proof for the covariant string.

  • 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. §§3.1 and 3.3 discuss the central stress pole and the contour construction of the Virasoro algebra; §§3.6 and 4.1 develop descendants and their inner products.
  • David Tong, Lectures on String Theory (2009); arXiv:0908.0333. §4.3.3 derives the exponential and stress OPEs; §4.5.2 evaluates the Virasoro contour commutator; §§5.4–5.4.2 distinguish physical matter vertices, tensor primarity, and boundary weights.