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Closed-String T-Duality and Enhanced Symmetry

A closed string on a circle carries both momentum and winding. Exchanging these two integers turns a circle of radius RR into one of radius α′/R\alpha'/R without changing the physical spectrum. At the fixed radius R=α′R=\sqrt{\alpha'}, additional vector particles become massless and enlarge the gauge algebra from two Abelian factors to su(2)L⊕su(2)R\mathfrak{su}(2)_L\oplus\mathfrak{su}(2)_R. The same calculation also reveals extra scalar fields and explains how changing the radius gives masses to the charged vectors.

We develop this example for the critical closed bosonic string, including its thermal winding mode. The course overview fixes the worldsheet coordinates, free-boson normalization, spacetime signature and string coupling. The bosonic ground-state tachyon remains present throughout; the exact compact-boson conformal field theory and its spectrum can be studied without interpreting the background as a stable vacuum.

Compactify one spatial coordinate,

Y≡X25∼Y+2πR,Y\equiv X^{25}\sim Y+2\pi R,

and denote the noncompact momentum by kμk^\mu, μ=0,…,24\mu=0,\ldots,24. A periodic center-of-mass wavefunction has compact momentum pY=n/Rp_Y=n/R, with n∈Zn\in\mathbb Z. A closed string can also satisfy

Y(τ,σ+2π)−Y(τ,σ)=2πwR,w∈Z.Y(\tau,\sigma+2\pi)-Y(\tau,\sigma)=2\pi wR, \qquad w\in\mathbb Z.

The integer ww counts winding around the target circle. It is conserved in a continuous deformation of a closed-string configuration; at a string interaction, total winding is conserved even though individual strings can join or split.

Write Y=YL(τ+σ)+YR(τ−σ)Y=Y_L(\tau+\sigma)+Y_R(\tau-\sigma). Its mode expansion is

Y=y+α′2pL(τ+σ)+α′2pR(τ−σ)+iα′2∑m≠01m(αmYe−im(τ+σ)+α~mYe−im(τ−σ)).\begin{aligned} Y={}&y+\frac{\alpha'}2p_L(\tau+\sigma) +\frac{\alpha'}2p_R(\tau-\sigma)\\ &+i\sqrt{\frac{\alpha'}2}\sum_{m\ne0}\frac1m \left(\alpha_m^Y e^{-im(\tau+\sigma)} +\widetilde\alpha_m^Y e^{-im(\tau-\sigma)}\right). \end{aligned}

The canonical momentum density is PY=Y˙/(2πα′)P_Y=\dot Y/(2\pi\alpha'). Its integral and the winding condition give

∫02πPY dσ=pL+pR2=nR,πα′(pL−pR)=2πwR.\int_0^{2\pi}P_Y\,d\sigma=\frac{p_L+p_R}{2}=\frac nR, \qquad \pi\alpha'(p_L-p_R)=2\pi wR.

Thus

pL=nR+wRα′,pR=nR−wRα′.p_L=\frac nR+\frac{wR}{\alpha'}, \qquad p_R=\frac nR-\frac{wR}{\alpha'}.

Both momenta have dimensions of inverse length. Momentum costs an energy proportional to 1/R1/R, whereas the energy of a wound string is proportional to its length, hence to R/α′R/\alpha'. Their competition is the origin of radius inversion.

Let NN and N~\widetilde N be the nonnegative left and right oscillator levels. The two physical-state conditions are

α′4(k2+pL2)+N=1,α′4(k2+pR2)+N~=1.\frac{\alpha'}4(k^2+p_L^2)+N=1, \qquad \frac{\alpha'}4(k^2+p_R^2)+\widetilde N=1.

These are the bosonic intercept conditions. The corresponding plane matter vertices have weights (1,1)(1,1); the intercept is not an additional subtraction from those plane weights. Defining the 25-dimensional mass by M2=−k2M^2=-k^2, each equation separately gives

M2=pL2+4α′(N−1)=pR2+4α′(N~−1).M^2=p_L^2+\frac4{\alpha'}(N-1) =p_R^2+\frac4{\alpha'}(\widetilde N-1).

Subtracting them uses pL2−pR2=4nw/α′p_L^2-p_R^2=4nw/\alpha' and yields level matching:

N−N~+nw=0.N-\widetilde N+nw=0.

Averaging them gives the symmetric mass formula

M2=n2R2+w2R2α′2+2α′(N+N~−2).M^2=\frac{n^2}{R^2}+\frac{w^2R^2}{\alpha'^2} +\frac2{\alpha'}(N+\widetilde N-2).

Both conditions are needed. For example, (n,w)=(1,1)(n,w)=(1,1) allows (N,N~)=(0,1)(N,\widetilde N)=(0,1), but not (0,0)(0,0). A number obtained from the averaged mass formula for a level-mismatched assignment is not a physical string mass.

At a generic radius, the massless states have n=w=0n=w=0 and N=N~=1N=\widetilde N=1. Each side has 24 transverse oscillator polarizations, so there are 242=57624^2=576 real physical polarizations. Under the 25-dimensional massless little group SO(23)SO(23) they become

FieldPhysical polarizations
Graviton gμνg_{\mu\nu}23⋅24/2−1=27523\cdot24/2-1=275
Two-form BμνB_{\mu\nu}23⋅22/2=25323\cdot22/2=253
Two vectors from gμYg_{\mu Y} and BμYB_{\mu Y}2⋅23=462\cdot23=46
Dilaton and radius scalar22

The two vectors couple to momentum and winding. Their left/right linear combinations correspond to the two compact-boson currents ∂YL\partial Y_L and ∂ˉYR\bar\partial Y_R.

Here “generic” excludes isolated radii where a Fourier or winding mode of the bosonic tachyon happens to become massless. Such extra scalar states do not by themselves enhance the gauge algebra. Exercise 2 classifies those exceptions.

Introduce the dimensionless radius r=R/α′r=R/\sqrt{\alpha'}. Under

R⟼R~=α′R,(n,w)⟼(w,n),R\longmapsto\widetilde R=\frac{\alpha'}R, \qquad (n,w)\longmapsto(w,n),

the left momentum stays fixed and the right momentum reverses:

p~L=pL,p~R=−pR.\widetilde p_L=p_L, \qquad \widetilde p_R=-p_R.

The oscillator map that accompanies this transformation is

αmY⟼αmY,α~mY⟼−α~mY.\alpha_m^Y\longmapsto\alpha_m^Y, \qquad \widetilde\alpha_m^Y\longmapsto-\widetilde\alpha_m^Y.

The levels, commutators, mass formula and level-matching condition are therefore preserved. On the chiral coordinate fields this is

Y=YL+YR⟼Y~=YL−YR.Y=Y_L+Y_R\longmapsto\widetilde Y=Y_L-Y_R.

The compact-boson operator products are preserved as well, with appropriate transformations of the zero-mode cocycles that ensure mutual locality of charged vertices. The coordinate and oscillator statement does not mean that every vertex is unchanged in a fixed cocycle basis. Exercise 1 constructs an explicit lift and displays its phases. This operator-algebra statement is stronger than agreement of mass eigenvalues alone; see Tong, §8.3 and the fuller compact-boson treatment in String II.

Radius inversion exchanges momentum and winding, preserves the left momentum, reverses the right momentum, and exchanges the canonical momentum with the spatial derivative.

T-duality relates RR and α′/R\alpha'/R by exchanging the integer charges and reflecting the compact right mover. The lower relations use P=Y˙/(2πα′)P=\dot Y/(2\pi\alpha'); primes there denote spatial derivatives. The diagram shows exact relationships, with no numerical coordinate scale. Charged-vertex cocycle phases are additional to the coordinate map.

Equations of motion and the canonical transformation

Section titled “Equations of motion and the canonical transformation”

Differentiating YL+YRY_L+Y_R and YL−YRY_L-Y_R gives

∂τY~=∂σY,∂σY~=∂τY.\partial_\tau\widetilde Y=\partial_\sigma Y, \qquad \partial_\sigma\widetilde Y=\partial_\tau Y.

The equality of the mixed derivatives of Y~\widetilde Y then requires

∂τ2Y−∂σ2Y=0.\partial_\tau^2Y-\partial_\sigma^2Y=0.

Thus the wave equation for YY is the integrability condition for its dual. Conversely, the wave equation for Y~\widetilde Y follows from equality of mixed derivatives of YY. This explains the interchange between an equation of motion and a differential identity without an unspecified Hodge-star sign.

There is an important distinction between this on-shell relation and an off-shell substitution into an action. The Lorentzian compact-coordinate Lagrangian density is

L=14πα′(Y˙2−Y′2).\mathcal L=\frac1{4\pi\alpha'}(\dot Y^2-Y'^2).

Swapping Y˙\dot Y with Y′Y' negates this expression. It does not directly prove equality of the two Lagrangian densities. The canonical description gives the correct statement. With P=Y˙/(2πα′)P=\dot Y/(2\pi\alpha'),

H=πα′P2+Y′24πα′,P~=Y′2πα′,Y~′=2πα′P.\mathcal H=\pi\alpha'P^2+\frac{Y'^2}{4\pi\alpha'}, \qquad \widetilde P=\frac{Y'}{2\pi\alpha'}, \qquad \widetilde Y'=2\pi\alpha'P.

The two positive terms in H\mathcal H exchange, so the Hamiltonian is invariant. The momentum density is also preserved: P~Y~′=PY′\widetilde P\widetilde Y'=PY'. Exercise 4 explains a local generating functional and the care required by winding at its boundary.

The compact-boson conformal field theories are equivalent at fixed worldsheet topology. To relate perturbative interacting string theories, the constant dilaton must transform too. Dimensional reduction of the string-frame gravitational term makes its 25-dimensional coefficient proportional to

Re−2Φ.R e^{-2\Phi}.

Keeping this coefficient invariant under R↦α′/RR\mapsto\alpha'/R gives

Φ~=Φ−log⁡r,g~s=gsr.\widetilde\Phi=\Phi-\log r, \qquad \widetilde g_s=\frac{g_s}{r}.

This agrees with the path-integral measure transformation described by Tong, §8.3. The constant shift weights different worldsheet Euler characteristics correctly. It is not needed merely to check a free mass eigenvalue. For the bosonic theory, statements about vacuum amplitudes remain formal in the presence of the tachyon divergence.

Winding marginality and the thermal circle

Section titled “Winding marginality and the thermal circle”

Consider first a spatial circle and the winding ground states

n=0,w=±1,N=N~=0.n=0,\qquad w=\pm1,\qquad N=\widetilde N=0.

They satisfy level matching, and their masses are

Mw2=R2α′2−4α′,α′Mw2=r2−4.M_w^2=\frac{R^2}{\alpha'^2}-\frac4{\alpha'}, \qquad \alpha'M_w^2=r^2-4.

They become massless at R=2α′R=2\sqrt{\alpha'}. This is already different from the self-dual radius α′\sqrt{\alpha'}.

The distinction is equally clear on the worldsheet. At zero noncompact momentum the two winding operators have compact-coordinate factors

W±=:exp⁡ ⁣[±iRα′(YL−YR)]:,h=hˉ=R24α′.\mathcal W_\pm =:\exp\!\left[\pm i\frac R{\alpha'}(Y_L-Y_R)\right]:, \qquad h=\bar h=\frac{R^2}{4\alpha'}.

Their real combination is proportional to cos⁡(RY~/α′)\cos(R\widetilde Y/\alpha'). As an integrated perturbation it is irrelevant for r>2r>2, linearly marginal at r=2r=2, and relevant for r<2r<2. This is the compact-boson relevance criterion behind the Kosterlitz–Thouless analogy. Establishing a complete transition would require the coupled running of the perturbation and radius; the weight calculation alone does not establish it.

For thermal physics, Euclidean time is periodic with circumference β=1/T\beta=1/T, so its circle radius is R0=β/(2π)R_0=\beta/(2\pi). The first thermal winding pair consequently has the spatial fluctuation mass

mth2=β2−βH24π2α′2,βH=4πα′,TH=14πα′.m_{\mathrm{th}}^2 =\frac{\beta^2-\beta_H^2}{4\pi^2\alpha'^2}, \qquad \beta_H=4\pi\sqrt{\alpha'}, \qquad T_H=\frac1{4\pi\sqrt{\alpha'}}.

The states of opposite thermal winding form one complex thermal scalar. This Euclidean mode is not an ordinary particle winding a Lorentzian time circle. Its threshold agrees with the density-of-states calculation. A worldsheet modular transformation relates the large density of highly excited strings to the infrared behavior of this winding mode; Kruczenski and Lawrence, §§2–3 explain this relation through the thermal scalar and random walks.

Two limitations matter. First, the zero-winding bosonic tachyon still has M2=−4/α′M^2=-4/\alpha' at every β\beta, so this calculation does not produce a stable bosonic ensemble below THT_H. Second, the precise nonanalyticity depends on the number of noncompact spatial dimensions: a massless winding mode need not make the infinite-volume free energy itself diverge at the threshold. Exercise 6 isolates this infrared question. Neither limitation changes the mass formula or the distinction between r=2r=2 and r=1r=1.

At R=α′R=\sqrt{\alpha'}, the chiral momenta become

pL=n+wα′,pR=n−wα′.p_L=\frac{n+w}{\sqrt{\alpha'}}, \qquad p_R=\frac{n-w}{\sqrt{\alpha'}}.

For a massless state, the two shell conditions are

(n+w)2+4N=4,(n−w)2+4N~=4.(n+w)^2+4N=4, \qquad (n-w)^2+4\widetilde N=4.

Since each term is nonnegative, N,N~≤1N,\widetilde N\le1 and ∣n±w∣≤2|n\pm w|\le2. These bounds make the following list exhaustive:

Momentum and winding(N,N~)(N,\widetilde N)Physical polarizations
(0,0)(0,0)(1,1)(1,1)242=57624^2=576
(1,1),(−1,−1)(1,1),(-1,-1)(0,1)(0,1)2⋅242\cdot24
(1,−1),(−1,1)(1,-1),(-1,1)(1,0)(1,0)2⋅242\cdot24
(2,0),(−2,0),(0,2),(0,−2)(2,0),(-2,0),(0,2),(0,-2)(0,0)(0,0)44

The total is 676676. A one-oscillator sector supplies a 25-dimensional massless vector with 23 polarizations and a compact scalar with one. Therefore the full massless content is

275+253+6⋅23+1+9=676:275+253+6\cdot23+1+9=676:

a graviton, a two-form, six vectors, a dilaton and nine compact scalars. The additional states contribute 4⋅23+8=1004\cdot23+8=100 polarizations beyond the generic spectrum. These counts refer to physical polarizations at nonzero null noncompact momentum; exceptional zero-momentum cohomology is not being counted.

The dimensionless current charges at this radius are

qL=α′2pL=n+w2,qR=α′2pR=n−w2.q_L=\frac{\sqrt{\alpha'}}2p_L=\frac{n+w}{2}, \qquad q_R=\frac{\sqrt{\alpha'}}2p_R=\frac{n-w}{2}.

For the compact scalars, (qL,qR)(q_L,q_R) fills the nine weights of (3,3)(\mathbf3,\mathbf3):

qL,qR∈{−1,0,1},n=qL+qR,w=qL−qR.q_L,q_R\in\{-1,0,1\}, \qquad n=q_L+q_R, \qquad w=q_L-q_R.

The center (0,0)(0,0) is the neutral radius scalar. The four axial weights arise from the internal polarization of the one-oscillator sectors. The four corners arise from the zero-oscillator states with two units of momentum or winding. Opposite weights describe conjugate fields, so the center plus four conjugate pairs gives nine real scalar components, eight of which are charged under the Cartan generators.

The nine scalar weights form a three-by-three grid: the neutral radius scalar is central, four axial weights are Goldstone directions, and four corner weights are physical scalar branches.

At R=α′R=\sqrt{\alpha'}, the nine real scalar components transform as (3,3)(\mathbf3,\mathbf3) with qL,R=α′pL,R/2q_{L,R}=\sqrt{\alpha'}p_{L,R}/2. The coordinate scales are equal. Opposite points are conjugate fields. The four extra vector fields have the axial charges too, with noncompact rather than compact oscillator polarizations. Under a radius deformation, the four axial scalars supply their longitudinal polarizations.

The enhanced symmetry can be derived directly from the common free-boson OPE. On the left, define the currents

J3=iα′∂YL,J±∝:e±2iYL/α′:.J^3=\frac{i}{\sqrt{\alpha'}}\partial Y_L, \qquad J^\pm\propto :e^{\pm2iY_L/\sqrt{\alpha'}}:.

The proportionality includes zero-mode cocycles and constant phases, chosen so that J+J^+ and J−J^- are conjugate and their opposite-charge OPE has positive leading coefficient. These phases do not change conformal weights. A lattice convention and a compatible choice are given in Exercise 1.

Each exponential has h=α′(2/α′)2/4=1h=\alpha'(2/\sqrt{\alpha'})^2/4=1. Differentiating YL(z)YL(w)∼−α′log⁡(z−w)/2Y_L(z)Y_L(w)\sim-\alpha'\log(z-w)/2 gives

∂YL(z)∂YL(w)∼−α′2(z−w)2,J3(z)J3(w)∼12(z−w)2.\partial Y_L(z)\partial Y_L(w) \sim-\frac{\alpha'}{2(z-w)^2}, \qquad J^3(z)J^3(w)\sim\frac1{2(z-w)^2}.

Contracting one derivative with an exponential yields

J3(z)J±(w)∼±J±(w)z−w.J^3(z)J^\pm(w)\sim\frac{\pm J^\pm(w)}{z-w}.

For opposite charges, the exponential contraction produces a double pole. Expanding the remaining normal-ordered exponential one order further gives

J+(z)J−(w)∼1(z−w)2[1+2iα′(z−w)∂YL(w)+⋯ ]∼1(z−w)2+2J3(w)z−w.\begin{aligned} J^+(z)J^-(w) &\sim\frac1{(z-w)^2} \left[1+\frac{2i}{\sqrt{\alpha'}}(z-w)\partial Y_L(w)+\cdots\right]\\ &\sim\frac1{(z-w)^2}+\frac{2J^3(w)}{z-w}. \end{aligned}

Equal-charge products start at order (z−w)2(z-w)^2 and have no singular term. With J±=J1±iJ2J^\pm=J^1\pm iJ^2, these results combine into

Ja(z)Jb(w)∼δab2(z−w)2+iϵabcJc(w)z−w.J^a(z)J^b(w)\sim \frac{\delta^{ab}}{2(z-w)^2} +\frac{i\epsilon^{ab}{}_{c}J^c(w)}{z-w}.

This is the affine SU(2)SU(2) algebra at level one. In modes,

[Jma,Jnb]=iϵabcJm+nc+m2δabδm+n,0.[J_m^a,J_n^b] =i\epsilon^{ab}{}_{c}J_{m+n}^c +\frac m2\delta^{ab}\delta_{m+n,0}.

Its zero modes form the ordinary su(2)\mathfrak{su}(2) Lie algebra. The right currents Jˉa\bar J^a satisfy the same algebra and commute with the left currents. Ginsparg, §§8.6–8.7 derives this compact-boson enhancement; his Cartesian currents have a different normalization, so the coefficients above follow from the course OPE rather than an implicit change of convention.

Currents, vector particles and scalar particles

Section titled “Currents, vector particles and scalar particles”

The matter parts of the massless vector vertices are proportional to

ALμa Ja∂ˉXμeik⋅X,ARμa ∂XμJˉaeik⋅X.A_{L\mu}^{a}\,J^a\bar\partial X^\mu e^{ik\cdot X}, \qquad A_{R\mu}^{a}\,\partial X^\mu\bar J^a e^{ik\cdot X}.

Each current supplies weight one on its side, and the derivative supplies weight one on the other. Physical polarization constraints impose transversality and identify longitudinal gauge representatives. The three left and three right currents therefore create six vector fields. Their zero-mode OPE residues explain the enhanced non-Abelian gauge algebra, not merely its dimension.

The nine scalar vertices instead have matter factors

φab JaJˉbeik⋅X.\varphi_{ab}\,J^a\bar J^b e^{ik\cdot X}.

For unintegrated closed-string vertices, multiply the weight-(1,1)(1,1) matter operator by ccˉc\bar c. The expressions above specify particle content and charges; they do not replace the ghost prescription for amplitudes.

In a real Cartesian current basis, φab\varphi_{ab} is a real 3×33\times3 matrix transforming in (3,3)(\mathbf3,\mathbf3). Under the specified full perturbative compact-boson spectrum, the faithful action of the enhanced group is (SU(2)L×SU(2)R)/Z2(SU(2)_L\times SU(2)_R)/\mathbb Z_2, with the diagonal center removed. Exercise 1 explains why the full charge lattice, including massive states, is needed to determine this global statement.

Radius deformation and the Higgs mechanism

Section titled “Radius deformation and the Higgs mechanism”

To vary the radius while keeping the coordinate periodicity fixed, write Y=RθY=R\theta, where θ∼θ+2π\theta\sim\theta+2\pi. The Euclidean action is

Sθ=R22πα′∫d2z ∂θ∂ˉθ.S_\theta=\frac{R^2}{2\pi\alpha'}\int d^2z\, \partial\theta\bar\partial\theta.

Changing R2R^2 changes the coefficient of a free Gaussian theory. The corresponding operator is proportional to ∂YL∂ˉYR\partial Y_L\bar\partial Y_R, hence to J3Jˉ3J^3\bar J^3. This is an exactly marginal deformation: it moves along the family of compact-boson conformal field theories. In spacetime it is an expectation value of the neutral component φ33\varphi_{33}, leaving the two Cartan gauge generators unbroken.

Vector masses and the missing polarizations

Section titled “Vector masses and the missing polarizations”

Follow, for example, the states (n,w)=(1,1)(n,w)=(1,1), (N,N~)=(0,1)(N,\widetilde N)=(0,1) away from the self-dual point. The right shell gives

MW2=pR2=1α′(r−r−1)2.M_W^2=p_R^2 =\frac1{\alpha'}(r-r^{-1})^2.

All four charged vector branches have this mass. Their internal oscillator polarizations explain how the vectors acquire a longitudinal mode.

For this branch, combine the noncompact momentum and right compact momentum into the null 26-vector KR=(kμ,pR)K_R=(k^\mu,p_R). A level-one right polarization satisfies

KR⋅ζ=0,ζ∼ζ+λKR,KR2=0.K_R\cdot\zeta=0, \qquad \zeta\sim\zeta+\lambda K_R, \qquad K_R^2=0.

The constraint and the gauge identification leave 26−1−1=2426-1-1=24 physical polarizations. When pR≠0p_R\ne0, choose λ=−ζY/pR\lambda=-\zeta_Y/p_R to set the compact component to zero. The remaining polarization is a massive vector in 25 dimensions, with 24 physical modes. When pR=0p_R=0, this gauge transformation no longer removes ζY\zeta_Y; the modes reorganize into a massless vector with 23 polarizations plus a scalar. The other charged branches work in the same way, using pLp_L where appropriate.

Thus the four axial scalar weights supply the Goldstone directions for the four broken generators. Exercise 3 exhibits a smooth physical polarization class through the massless limit, rather than relying only on a count.

The corner weights have no oscillator polarization to absorb. The pure momentum pair (n,w)=(±2,0)(n,w)=(\pm2,0) and pure winding pair (0,±2)(0,\pm2) have

α′Mn2=4r−2−4,α′Mw2=4r2−4.\alpha'M_n^2=4r^{-2}-4, \qquad \alpha'M_w^2=4r^2-4.

They are massless at r=1r=1, but one conjugate pair is tachyonic on either side: momentum scalars for r>1r>1 and winding scalars for r<1r<1. This is compatible with exact marginality of the radius operator. A consistent worldsheet CFT need not describe a stable spacetime vacuum.

With u=log⁡ru=\log r, the vector mass behaves quadratically near the symmetric point, while the scalar masses have opposite linear slopes:

α′MW2=4sinh⁡2u=4u2+O(u4),α′Mn2=−8u+O(u2),α′Mw2=8u+O(u2).\begin{gathered} \alpha'M_W^2=4\sinh^2u=4u^2+O(u^4),\\ \alpha'M_n^2=-8u+O(u^2), \qquad \alpha'M_w^2=8u+O(u^2). \end{gathered}

The four charged-vector masses touch zero quadratically at the self-dual radius, while the two scalar pairs cross zero with opposite slopes.

Exact bosonic-circle mass branches in dimensionless coordinates u=log⁡(R/α′)u=\log(R/\sqrt{\alpha'}) and α′M2\alpha'M^2. The vector curve represents four real charged-vector components; each scalar curve represents a conjugate pair, or two real scalar components. Negative values indicate tachyonic fluctuations. The neutral radius scalar remains massless. Radius inversion reflects uu and exchanges the two scalar curves; the thermal first-winding threshold concerns different states.

Why nine massless scalars do not mean nine moduli

Section titled “Why nine massless scalars do not mean nine moduli”

At the enhanced point every JaJˉbJ^a\bar J^b has weights (1,1)(1,1), so all nine scalar deformations are marginal to first order. Higher orders depend on their OPEs. A product of one chosen left current and one chosen right current can be rotated to J3Jˉ3J^3\bar J^3, and therefore generates the same radius family in a rotated basis. An arbitrary sum of products need not do so.

For example, the simple-pole terms in the two current algebras imply

V=∑a=13JaJˉa,V(z,zˉ)V(0)⊃−2V(0)∣z∣2.V=\sum_{a=1}^3J^a\bar J^a, \qquad V(z,\bar z)V(0)\supset-\frac{2V(0)}{|z|^2}.

Integrating the 1/∣z∣21/|z|^2 term produces a logarithm, so this perturbation is not exactly marginal. Exercise 5 derives the general matrix criterion at this order and explains the separate all-order argument for rank-one products. The distinction between conformal weight (1,1)(1,1) and exact marginality is developed in Ginsparg, §8.6.

The enhancement described here is specific to the bosonic spectrum. On a supersymmetric Type II circle with the standard GSO projection, each allowed chiral oscillator level is at least its intercept. A massless state then requires both compact chiral momenta to vanish, so there are no analogous finite-radius extra vector states with nonzero momentum or winding. T-duality still acts, but the enhanced bosonic spectrum is not carried over unchanged. The next page instead applies the dual coordinate to open-string boundary conditions.

Using the mass formula without level matching. Both chiral physical-state conditions must hold. A state that has M2=0M^2=0 in the average but violates N−N~+nw=0N-\widetilde N+nw=0 is absent from the closed-string spectrum.

Identifying every special radius with gauge enhancement. The first winding ground state becomes massless at r=2r=2, whereas the extra vector currents appear at r=1r=1. Other isolated radii also support massless scalar modes of the bosonic tachyon.

Counting every charged scalar as a modulus. The enhanced theory has nine real compact scalars, including one neutral component. Along the radius family four become longitudinal vector polarizations, four acquire the scalar masses above, and one remains the radius modulus.

Exercise 1. Charge lattice, cocycles and the center

Section titled “Exercise 1. Charge lattice, cocycles and the center”

Set QL,R=α′/2 pL,RQ_{L,R}=\sqrt{\alpha'/2}\,p_{L,R}. For charges a=(n,w)a=(n,w) and b=(m,v)b=(m,v), show that QL(a)QL(b)−QR(a)QR(b)=nv+wmQ_L(a)Q_L(b)-Q_R(a)Q_R(b)=nv+wm. Prove that the lattice is even and unimodular. Use

ϵ(a,b)=(−1)wm\epsilon(a,b)=(-1)^{wm}

as the cocycle in the leading product of lattice vertices VaVbV_aV_b. Check associativity and the exchange sign, and find a lift of T(n,w)=(w,n)T(n,w)=(w,n) of the form Va↦ξ(a)VTaV_a\mapsto\xi(a)V_{Ta}. Finally determine the kernel of the center of SU(2)L×SU(2)RSU(2)_L\times SU(2)_R on this perturbative compact-boson spectrum.

Solution

Expanding the two products cancels the momentum–momentum and winding–winding terms and leaves B(a,b)=nv+wmB(a,b)=nv+wm. In the integer basis (n,w)(n,w) its Gram matrix is

U=(0110).U=\begin{pmatrix}0&1\\1&0\end{pmatrix}.

Its determinant is −1-1, so the integral lattice is unimodular. Its norm B(a,a)=2nwB(a,a)=2nw is even. The signature is (1,1)(1,1); this is not a positive-definite Euclidean charge lattice.

For a third charge c=(ℓ,t)c=(\ell,t), the two associativity exponents are

wm+(w+v)ℓandvℓ+w(m+ℓ),wm+(w+v)\ell \quad\hbox{and}\quad v\ell+w(m+\ell),

which agree. Also ϵ(a,b)/ϵ(b,a)=(−1)wm−vn=(−1)B(a,b)\epsilon(a,b)/\epsilon(b,a)=(-1)^{wm-vn}=(-1)^{B(a,b)}. This compensates the exchange sign of the left/right exponential factors.

Preserving the product under the duality map requires

ϵ(a,b)ξ(a+b)=ξ(a)ξ(b)ϵ(Ta,Tb).\epsilon(a,b)\xi(a+b)=\xi(a)\xi(b)\epsilon(Ta,Tb).

The choice ξ(n,w)=(−1)nw\xi(n,w)=(-1)^{nw} works: the two sides have the same exponent modulo two after expanding (n+m)(w+v)(n+m)(w+v). It also obeys ξ(a)ξ(Ta)=1\xi(a)\xi(Ta)=1, so this chosen lift squares to the identity. Omitting the phase fails, for example, for a=(1,0)a=(1,0) and b=(0,1)b=(0,1): their cocycle changes sign under exchange of momentum and winding.

In this cocycle convention, Va†=(−1)nwV−aV_a^\dagger=(-1)^{nw}V_{-a}. For the left roots a=±(1,1)a=\pm(1,1), choosing J±=iV±(1,1)J^\pm=iV_{\pm(1,1)} makes them conjugate and gives a positive leading opposite-root OPE. The analogous choice works for right roots ±(1,−1)\pm(1,-1). The chosen lift sends JL±↦−JL±J_L^\pm\mapsto-J_L^\pm and JR±↦−JR∓J_R^\pm\mapsto-J_R^\mp, while JL3J_L^3 stays fixed and JR3J_R^3 changes sign. Thus preserving YLY_L, pLp_L and the left oscillators does not imply preserving all left charged vertices in a fixed cocycle basis. Other basis phases change the formula for the lift without changing the radius equivalence.

At the self-dual radius, the Cartan weights of any lattice state are qL=(n+w)/2q_L=(n+w)/2 and qR=(n−w)/2q_R=(n-w)/2. The two individual center elements act as (−1)n+w(-1)^{n+w} and (−1)n−w(-1)^{n-w}. Their product is always (−1)2n=1(-1)^{2n}=1, but either separate center acts nontrivially on the allowed state n=1,w=0n=1,w=0. Current descendants preserve this parity. Therefore the kernel on the full specified perturbative spectrum is the diagonal Z2\mathbb Z_2, and the faithful group is (SU(2)L×SU(2)R)/Z2(SU(2)_L\times SU(2)_R)/\mathbb Z_2. Inspecting only the adjoint massless fields would not determine this kernel.

For arbitrary r>0r>0, classify all integer (n,w)(n,w) and oscillator levels that can give M2=0M^2=0. Distinguish the states responsible for vector enhancement from isolated massless scalar modes.

Solution

The two equations are

(n/r+wr)2+4N=4,(n/r−wr)2+4N~=4.(n/r+wr)^2+4N=4, \qquad (n/r-wr)^2+4\widetilde N=4.

Nonnegativity forces N,N~∈{0,1}N,\widetilde N\in\{0,1\}.

If both levels equal one, both squares vanish. Adding and subtracting gives n=w=0n=w=0, valid for every radius.

If (N,N~)=(0,1)(N,\widetilde N)=(0,1), the right square vanishes, so n=wr2n=wr^2. The left square then gives 4nw=44nw=4, hence nw=1nw=1. Integrality implies n=w=±1n=w=\pm1 and r=1r=1. If the levels are (1,0)(1,0), the same reasoning gives nw=−1nw=-1, n=−w=±1n=-w=\pm1, again at r=1r=1. These four sectors contain the extra vector particles.

If both levels vanish, subtracting the squares gives nw=0nw=0. A nonzero pure momentum state has

w=0,r=∣n∣2,w=0,\qquad r=\frac{|n|}{2},

and a nonzero pure winding state has

n=0,r=2∣w∣.n=0,\qquad r=\frac2{|w|}.

The choice n=w=0n=w=0 cannot satisfy the shell equations in this case. These states have no oscillator index, so they are scalar modes. At r=1r=1 they are precisely (±2,0)(\pm2,0) and (0,±2)(0,\pm2), the four corner weights. The first winding pair w=±1w=\pm1 instead becomes massless at r=2r=2.

This classification is exhaustive because there are no other allowed oscillator levels. It also shows why an accidental scalar threshold at another radius does not generate the chiral weight-one currents needed for an extra spacetime vector.

Exercise 3. Follow a longitudinal polarization through enhancement

Section titled “Exercise 3. Follow a longitudinal polarization through enhancement”

Use three active components with metric diag⁡(−1,1,1)\operatorname{diag}(-1,1,1) and let

K=(E,p,q),E=p2+q2,p,q>0.K=(E,p,q),\qquad E=\sqrt{p^2+q^2},\qquad p,q>0.

The last component is a compact chiral momentum. Show that ζ=(p/q,E/q,0)\zeta=(p/q,E/q,0) represents a unit physical polarization. Find an equivalent representative with a finite limit as q→0q\to0 at fixed pp, and interpret the limit.

Solution

First K2=−E2+p2+q2=0K^2=-E^2+p^2+q^2=0. The proposed polarization obeys

K⋅ζ=−Epq+pEq=0,ζ2=E2−p2q2=1.K\cdot\zeta=-\frac{Ep}{q}+\frac{pE}{q}=0, \qquad \zeta^2=\frac{E^2-p^2}{q^2}=1.

Although its first two components diverge when q→0q\to0, physical polarizations are equivalence classes modulo multiples of KK. Choose

ζsmooth=ζ−Kq=(p−Eq,E−pq,−1).\zeta_{\rm smooth}=\zeta-\frac Kq =\left(\frac{p-E}{q},\frac{E-p}{q},-1\right).

Since E−p=q2/(E+p)E-p=q^2/(E+p), its first two components tend to zero. Thus

lim⁡q→0+ζsmooth=(0,0,−1).\lim_{q\to0^+}\zeta_{\rm smooth}=(0,0,-1).

Its norm remains one because K2=K⋅ζ=0K^2=K\cdot\zeta=0. At nonzero qq the representative with vanishing compact component is a longitudinal polarization of the massive 25-dimensional vector. At zero qq the same physical class becomes a compact scalar. The singularity in the first representative was a gauge-choice singularity, not loss of a physical state.

Taking q=∣pR∣q=|p_R| for a left-root branch, or ∣pL∣|p_L| for a right-root branch with the appropriate compact sign, makes this the string Higgs mechanism. The limit is taken at fixed nonzero noncompact spatial momentum, so it does not invoke exceptional zero-momentum states.

Exercise 4. Canonical duality and winding at a cut

Section titled “Exercise 4. Canonical duality and winding at a cut”

Consider the local generating functional

F[Y,Y~]=12πα′∫02πYY~′ dσ.F[Y,\widetilde Y]=\frac1{2\pi\alpha'}\int_0^{2\pi}Y\widetilde Y'\,d\sigma.

Derive the canonical transformation for variations fixed at a chosen cut. Explain why merely requiring periodic variations is insufficient when YY has winding. Then integrate the canonical relations to derive the global charge exchange and check the Hamiltonian and momentum densities.

Solution

Variation and integration by parts give

δF=12πα′[∫02π(Y~′δY−Y′δY~) dσ+[YδY~]02π].\delta F=\frac1{2\pi\alpha'}\left[ \int_0^{2\pi}(\widetilde Y'\delta Y-Y'\delta\widetilde Y)\,d\sigma +[Y\delta\widetilde Y]_0^{2\pi}\right].

For variations with δY~=0\delta\widetilde Y=0 at the cut, the endpoint term vanishes. The type-one generating-functional relations then give

P=δFδY=Y~′2πα′,P~=−δFδY~=Y′2πα′.P=\frac{\delta F}{\delta Y}=\frac{\widetilde Y'}{2\pi\alpha'}, \qquad \widetilde P=-\frac{\delta F}{\delta\widetilde Y}=\frac{Y'}{2\pi\alpha'}.

Periodic variations alone do not remove the endpoint term. If Y(2π)−Y(0)=2πwRY(2\pi)-Y(0)=2\pi wR and δY~(2π)=δY~(0)\delta\widetilde Y(2\pi)=\delta\widetilde Y(0), it equals

[YδY~]02π=2πwR δY~(0).[Y\delta\widetilde Y]_0^{2\pi}=2\pi wR\,\delta\widetilde Y(0).

Thus the displayed functional is a local description with a fixed basepoint/cut prescription. It is not, without zero-mode and boundary treatment, a globally single-valued generating function on all winding sectors. The global charges can instead be checked directly from the canonical relations:

n~R~=∫P~ dσ=wRα′,2πw~R~=∫Y~′ dσ=2πα′nR.\frac{\widetilde n}{\widetilde R} =\int\widetilde P\,d\sigma=\frac{wR}{\alpha'}, \qquad 2\pi\widetilde w\widetilde R =\int\widetilde Y'\,d\sigma=\frac{2\pi\alpha'n}{R}.

With R~=α′/R\widetilde R=\alpha'/R, these equations become n~=w\widetilde n=w and w~=n\widetilde w=n. Conversely, exchanging the primitive momentum and winding units fixes this dual radius.

Finally,

πα′P~2+Y~′24πα′=Y′24πα′+πα′P2,P~Y~′=PY′.\pi\alpha'\widetilde P^2+\frac{\widetilde Y'^2}{4\pi\alpha'} =\frac{Y'^2}{4\pi\alpha'}+\pi\alpha'P^2, \qquad \widetilde P\widetilde Y'=PY'.

The energy and spatial momentum densities are preserved. This canonical result does not require the false assertion that a direct derivative swap leaves the Lorentzian Lagrangian density unchanged.

Exercise 5. Current products and marginality

Section titled “Exercise 5. Current products and marginality”

For a real matrix λ\lambda, set Vλ=λabJaJˉbV_\lambda=\lambda_{ab}J^a\bar J^b, with repeated indices summed from one to three. Show that its self-OPE contains

Vλ(z,zˉ)Vλ(0)⊃−2cof⁡(λ)ef∣z∣2JeJˉf(0).V_\lambda(z,\bar z)V_\lambda(0) \supset-\frac{2\operatorname{cof}(\lambda)_{ef}}{|z|^2} J^e\bar J^f(0).

Determine when this leading logarithmic obstruction vanishes, and explain which part of the conclusion can be promoted to an all-order statement.

Solution

The required term is the product of the simple poles in the two current OPEs. Their factors of ii multiply to −1-1, giving the coefficient

−λabλcdϵaceϵbdf.-\lambda_{ab}\lambda_{cd}\epsilon^{ac}{}_{e}\epsilon^{bd}{}_{f}.

For a 3×33\times3 matrix, the cofactor formula is

cof⁡(λ)ef=12ϵeacϵfbdλabλcd.\operatorname{cof}(\lambda)_{ef} =\frac12\epsilon_{eac}\epsilon_{fbd}\lambda_{ab}\lambda_{cd}.

Cyclically permuting the three indices of either epsilon introduces no sign, so these expressions agree as stated. The integral ∫d2z/∣z∣2\int d^2z/|z|^2 is logarithmic; a nonzero coefficient produces a leading renormalization of the couplings.

Every cofactor is a signed 2×22\times2 minor. All such minors vanish precisely when rank⁡λ≤1\operatorname{rank}\lambda\le1. For nonzero rank one, write λab=uavb\lambda_{ab}=u_av_b. Independent real rotations of the two current triplets align uu and vv with their respective third axes. The perturbation then becomes a multiple of J3Jˉ3J^3\bar J^3, which changes the coefficient of a free compact-boson action. This independent Gaussian-theory argument establishes exact marginality along that direction to all orders, within the radius family.

Vanishing of a leading beta-function coefficient alone would not prove that general conclusion. Here the all-order result follows because the rank-one operator is symmetry-related to the known radius deformation. Conversely, for λ=I\lambda=I the cofactor matrix is II, giving V(z,zˉ)V(0)⊃−2V(0)/∣z∣2V(z,\bar z)V(0)\supset-2V(0)/|z|^2. The isotropic sum is already obstructed at this order.

Thus the nine scalar fields are legitimate linearized massless excitations, but arbitrary independent constant values of their nine components do not parameterize a nine-dimensional family of circle CFTs.

Exercise 6. Infrared behavior of the thermal winding mode

Section titled “Exercise 6. Infrared behavior of the thermal winding mode”

Isolate the formal Gaussian contribution of the first thermal winding mode in d>0d>0 noncompact spatial dimensions. Introduce a positive reference mass μ\mu and write the large-proper-time tail, up to a constant, as

FIR∝∫1∞dt t−1−d/2e−m^2t,m^2=mth2μ2,t=μ2s.F_{\rm IR}\propto\int_1^\infty dt\,t^{-1-d/2}e^{-\widehat m^2t}, \qquad \widehat m^2=\frac{m_{\rm th}^2}{\mu^2}, \qquad t=\mu^2s.

Here ss is a dimensionful proper time, and the lower cutoff separates the infrared tail from short-distance contributions. Determine which derivatives with respect to m^2\widehat m^2 remain finite as m^2→0+\widehat m^2\to0^+. Explain the result for d=25d=25 and its limitations.

Solution

The free spatial heat kernel contributes s−d/2s^{-d/2}, while the determinant contributes ds/sds/s. After kk derivatives, the infrared integral is proportional to

(−1)k∫1∞dt tk−1−d/2e−m^2t.(-1)^k\int_1^\infty dt\,t^{k-1-d/2}e^{-\widehat m^2t}.

At zero mass, a power integral at its upper limit converges exactly when its exponent is less than −1-1. Therefore

k<d2k<\frac d2

is the convergence criterion. If k=d/2k=d/2, the integral is logarithmic and behaves as −log⁡m^2-\log\widehat m^2 up to finite terms. If k>d/2k>d/2, setting x=m^2tx=\widehat m^2t gives the leading behavior

∫1∞dt tk−1−d/2e−m^2t∼Γ ⁣(k−d2)(m^2)d/2−k.\int_1^\infty dt\,t^{k-1-d/2}e^{-\widehat m^2t} \sim\Gamma\!\left(k-\frac d2\right) (\widehat m^2)^{d/2-k}.

For d=25d=25, the free energy itself and its first twelve mass-squared derivatives have finite infrared limits; the thirteenth derivative is the first integer derivative that diverges. For negative m^2\widehat m^2, the exponential grows at large proper time and the Gaussian expression loses convergence.

This calculation concerns an isolated winding-mode contribution per spatial volume with a fixed infrared separation scale. It does not assert that the full bosonic string partition function is finite, because the zero-winding tachyon is still present. It also does not decide an interacting phase transition. It shows precisely why the appearance of a massless thermal scalar and divergence of the free energy itself are different claims.

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