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Superconformal Algebra and NS/R Sectors

The NSR matter theory is not just a free boson CFT plus some extra fermions. The stress tensor TT and supercurrent GG form a closed chiral algebra, and the allowed boundary conditions of the fermions split the Hilbert space into two sectors with very different spacetime interpretations.

The whole story begins with the two OPEs

Xμ(z,zˉ)Xν(w,wˉ)α2ημνlnzw2,ψμ(z)ψν(w)ημνzw.X^\mu(z,\bar z)X^\nu(w,\bar w) \sim -\frac{\alpha'}{2}\eta^{\mu\nu}\ln |z-w|^2, \qquad \psi^\mu(z)\psi^\nu(w) \sim \frac{\eta^{\mu\nu}}{z-w}.

With the normalization used in the previous page, the matter currents are

T(z)=1α:XμXμ:12:ψμψμ:,G(z)=i2α:ψμXμ:.T(z) = -\frac{1}{\alpha'}:\partial X^\mu\partial X_\mu: -\frac12:\psi^\mu\partial\psi_\mu:, \qquad G(z)=i\sqrt{\frac{2}{\alpha'}}:\psi^\mu\partial X_\mu:.

The stress tensor generates conformal transformations; the supercurrent generates the residual worldsheet supersymmetry left after superconformal gauge fixing.

The stress tensor and supercurrent generate the N equals one superconformal algebra.

The chiral NSR matter CFT is controlled by the stress tensor T(z)T(z) and its spin-3/23/2 superpartner G(z)G(z).

The singular OPEs are

T(z)T(w)c/2(zw)4+2T(w)(zw)2+T(w)zw,T(z)T(w) \sim \frac{c/2}{(z-w)^4} + \frac{2T(w)}{(z-w)^2} + \frac{\partial T(w)}{z-w}, T(z)G(w)32G(w)(zw)2+G(w)zw,T(z)G(w) \sim \frac{\frac32G(w)}{(z-w)^2} + \frac{\partial G(w)}{z-w},

and

G(z)G(w)2c/3(zw)3+2T(w)zw.G(z)G(w) \sim \frac{2c/3}{(z-w)^3} + \frac{2T(w)}{z-w}.

For DD free bosons and DD free Majorana fermions,

cmatter=D+D2=3D2.c_{\rm matter}=D+\frac{D}{2}=\frac{3D}{2}.

The second OPE says that GG is a primary field of weight 3/23/2. The third OPE is the supersymmetric analogue of the T(z)T(w)T(z)T(w) OPE: the anticommutator of two supersymmetry generators produces a translation, represented here by the stress tensor.

Expand the currents as

T(z)=nZLnzn2,G(z)=rGrzr3/2.T(z)=\sum_{n\in\mathbb Z}L_n z^{-n-2}, \qquad G(z)=\sum_r G_r z^{-r-3/2}.

The allowed values of rr depend on the fermion spin structure:

rZ+12in the NS sector,rZin the R sector.r\in\mathbb Z+\frac12 \quad\text{in the NS sector}, \qquad r\in\mathbb Z \quad\text{in the R sector}.

Contour manipulations then give the matter super-Virasoro algebra

[Lm,Ln]=(mn)Lm+n+c12(m3m)δm+n,0,[L_m,L_n] =(m-n)L_{m+n} +\frac{c}{12}(m^3-m)\delta_{m+n,0}, [Lm,Gr]=(m2r)Gm+r,[L_m,G_r] =\left(\frac{m}{2}-r\right)G_{m+r}, {Gr,Gs}=2Lr+s+c3(r214)δr+s,0.\{G_r,G_s\} = 2L_{r+s} +\frac{c}{3}\left(r^2-\frac14\right)\delta_{r+s,0}.

The mode expansions of T and G give the super-Virasoro algebra.

The super-Virasoro algebra is the mode algebra of T(z)T(z) and G(z)G(z). The same formula applies in the NS and R sectors, but the allowed labels rr are different.

In the full string theory, the matter algebra is accompanied by the bcbc ghosts and the commuting βγ\beta\gamma superghosts. The critical dimension D=10D=10 follows from cancellation of the total central charge. For the spectrum, however, the key point is simpler: physical states are annihilated by the positive modes of both TT and GG.

A worldsheet fermion can be antiperiodic or periodic around the spatial circle of the cylinder. For a chiral fermion,

ψμ(σ+2π)=ηψμ(σ),\psi^\mu(\sigma+2\pi)=\eta\,\psi^\mu(\sigma),

with

η=1for the Neveu–Schwarz sector,η=+1for the Ramond sector.\eta=-1 \quad\text{for the Neveu--Schwarz sector}, \qquad \eta=+1 \quad\text{for the Ramond sector}.

NS and R spin structures on the cylinder.

The NS sector is antiperiodic around the cylinder; the R sector is periodic. For closed strings the left- and right-moving sectors can be chosen independently.

For open strings, the boundary conditions at σ=0,π\sigma=0,\pi relate the left- and right-moving fermions, so there is one NS sector and one R sector. For closed strings, left and right movers are independent, giving

NS-NS,NS-R,R-NS,R-R.\text{NS-NS}, \qquad \text{NS-R}, \qquad \text{R-NS}, \qquad \text{R-R}.

The first contains familiar bosons such as the graviton, the mixed sectors contain spacetime fermions, and the R-R sector contains antisymmetric tensor gauge potentials.

On the plane the holomorphic fermion has the mode expansion

ψμ(z)=rψrμzr1/2,\psi^\mu(z)=\sum_r \psi_r^\mu z^{-r-1/2},

with oscillator algebra

{ψrμ,ψsν}=ημνδr+s,0.\{\psi_r^\mu,\psi_s^\nu\} = \eta^{\mu\nu}\delta_{r+s,0}.

Thus

sectorrzero mode?NSZ+12noRZyes, ψ0μ\begin{array}{c|c|c} \text{sector} & r & \text{zero mode?}\\ \hline \text{NS} & \mathbb Z+\frac12 & \text{no}\\ \text{R} & \mathbb Z & \text{yes, }\psi_0^\mu \end{array}

Allowed fermion mode labels in the NS and R sectors.

The absence or presence of the zero mode ψ0μ\psi_0^\mu is the crucial difference between the two sectors. The Ramond zero modes generate spacetime spinors.

The NS vacuum is comparatively simple: it is annihilated by all positive half-integer modes. The R vacuum is degenerate because the zero modes do not annihilate the state. Instead,

{ψ0μ,ψ0ν}=ημν.\{\psi_0^\mu,\psi_0^\nu\}=\eta^{\mu\nu}.

Equivalently,

Γμ=2ψ0μ{Γμ,Γν}=2ημν.\Gamma^\mu=\sqrt2\,\psi_0^\mu \quad\Longrightarrow\quad \{\Gamma^\mu,\Gamma^\nu\}=2\eta^{\mu\nu}.

So the Ramond ground states furnish a representation of the spacetime Clifford algebra. This is the first place where spacetime spinors enter the NSR formalism.

Let

z=eiw,w=σ+iτE.z=e^{-iw}, \qquad w=\sigma+i\tau_E.

A primary field of weight hh transforms as

ϕcyl(w)=(dzdw)hϕplane(z).\phi_{\rm cyl}(w)=\left(\frac{dz}{dw}\right)^h\phi_{\rm plane}(z).

For a fermion, h=1/2h=1/2, so the square root matters:

ψcyl(w)=(dzdw)1/2ψplane(z).\psi_{\rm cyl}(w)=\left(\frac{dz}{dw}\right)^{1/2}\psi_{\rm plane}(z).

The cylinder-plane map for a fermion includes a square root and creates the Ramond branch cut.

Because ψ\psi has weight 1/21/2, the cylinder-plane map includes a square root. On the plane the Ramond sector is naturally described by a branch cut ending on a spin-field insertion.

The Ramond ground state is therefore created by a spin field. The detailed construction by bosonization will come later; for now the important fact is that R-sector operators change the boundary condition of ψ\psi around the insertion.

In light-cone gauge there are D2D-2 transverse bosons and D2D-2 transverse fermions. The open NS zero-point energy is

E0NS=(D2)(124+148)=D216.E_0^{\rm NS} =-(D-2)\left(\frac{1}{24}+\frac{1}{48}\right) =-\frac{D-2}{16}.

For D=10D=10 this is

E0NS=12.E_0^{\rm NS}=-\frac12.

The R-sector fermions are periodic. Their zero-point energy cancels the bosonic contribution, so

E0R=0.E_0^{\rm R}=0.

Hence the open-string mass formulas in the critical NSR string are

αMNS2=N12,αMR2=N.\boxed{\alpha'M^2_{\rm NS}=N-\frac12,} \qquad \boxed{\alpha'M^2_{\rm R}=N.}

Normal-ordering constants in the NS and R sectors.

The NS and R sectors have different zero-point energies. In D=10D=10, aNS=1/2a_{\rm NS}=1/2 and aR=0a_{\rm R}=0 for the open superstring.

Before the GSO projection, the NS sector therefore has a tachyonic ground state, while the R ground state is massless. The next page builds these states explicitly.

Exercise 1. The weight of the supercurrent

Section titled “Exercise 1. The weight of the supercurrent”

Using h(ψ)=1/2h(\psi)=1/2 and h(X)=1h(\partial X)=1, explain why the supercurrent G=i2/α:ψX:G=i\sqrt{2/\alpha'}:\psi\cdot\partial X: has conformal weight 3/23/2.

Solution

For a normal-ordered product of free primary fields, the leading conformal weight is the sum of the weights unless singular contractions create additional anomalous terms. Here

h(ψμ)+h(Xμ)=12+1=32.h(\psi^\mu)+h(\partial X_\mu)=\frac12+1=\frac32.

A direct OPE computation gives

T(z)G(w)32G(w)(zw)2+G(w)zw,T(z)G(w) \sim \frac{\frac32G(w)}{(z-w)^2} + \frac{\partial G(w)}{z-w},

confirming that GG is a primary field of weight 3/23/2.

Exercise 2. Fermion modes from boundary conditions

Section titled “Exercise 2. Fermion modes from boundary conditions”

Show that antiperiodic boundary conditions imply rZ+1/2r\in\mathbb Z+1/2, while periodic boundary conditions imply rZr\in\mathbb Z.

Solution

Write a chiral fermion on the cylinder as

ψ(σ,τ)=rψr(τ)eirσ.\psi(\sigma,\tau)=\sum_r \psi_r(\tau)e^{-ir\sigma}.

Then

ψ(σ+2π,τ)=re2πirψr(τ)eirσ.\psi(\sigma+2\pi,\tau) =\sum_r e^{-2\pi i r}\psi_r(\tau)e^{-ir\sigma}.

Periodic boundary conditions require e2πir=1e^{-2\pi i r}=1, so rZr\in\mathbb Z. Antiperiodic boundary conditions require e2πir=1e^{-2\pi i r}=-1, so rZ+1/2r\in\mathbb Z+1/2.

Exercise 3. Super-Virasoro action on GrG_r

Section titled “Exercise 3. Super-Virasoro action on GrG_rGr​”

Use the fact that GG is a primary field of weight 3/23/2 to derive

[Lm,Gr]=(m2r)Gm+r.[L_m,G_r]=\left(\frac{m}{2}-r\right)G_{m+r}.
Solution

For a primary field ϕ\phi of weight hh with modes ϕr\phi_r, the Virasoro action is

[Lm,ϕr]=((h1)mr)ϕm+r.[L_m,\phi_r]=\big((h-1)m-r\big)\phi_{m+r}.

Setting h=3/2h=3/2 and ϕr=Gr\phi_r=G_r gives

[Lm,Gr]=(m2r)Gm+r.[L_m,G_r] =\left(\frac{m}{2}-r\right)G_{m+r}.

Exercise 4. NS zero-point energy in D=10D=10

Section titled “Exercise 4. NS zero-point energy in D=10D=10D=10”

Using ζ(1)=1/12\zeta(-1)=-1/12 and ζ(1,1/2)=1/24\zeta(-1,1/2)=1/24, compute the open NS zero-point energy in D=10D=10.

Solution

For one transverse boson,

E0boson=12n=1n=12ζ(1)=124.E_0^{\rm boson}=\frac12\sum_{n=1}^{\infty}n =\frac12\zeta(-1) =-\frac{1}{24}.

For one transverse NS fermion,

E0fermion=12r=1/2r=12ζ(1,12)=148.E_0^{\rm fermion} =-\frac12\sum_{r=1/2}^{\infty}r =-\frac12\zeta\left(-1,\frac12\right) =-\frac{1}{48}.

One transverse boson-fermion pair contributes

124148=116.-\frac{1}{24}-\frac{1}{48}=-\frac{1}{16}.

In D=10D=10 there are D2=8D-2=8 transverse pairs, hence

E0NS=8(116)=12.E_0^{\rm NS}=8\left(-\frac{1}{16}\right)=-\frac12.

Show that the Ramond zero modes generate the spacetime Clifford algebra.

Solution

The R-sector fermion modes obey

{ψrμ,ψsν}=ημνδr+s,0.\{\psi_r^\mu,\psi_s^\nu\}=\eta^{\mu\nu}\delta_{r+s,0}.

Taking r=s=0r=s=0 gives

{ψ0μ,ψ0ν}=ημν.\{\psi_0^\mu,\psi_0^\nu\}=\eta^{\mu\nu}.

Define Γμ=2ψ0μ\Gamma^\mu=\sqrt2\psi_0^\mu. Then

{Γμ,Γν}=2{ψ0μ,ψ0ν}=2ημν.\{\Gamma^\mu,\Gamma^\nu\} =2\{\psi_0^\mu,\psi_0^\nu\} =2\eta^{\mu\nu}.

This is the Clifford algebra in spacetime. Therefore the Ramond ground states transform as spacetime spinors.