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N=4 Super-Yang-Mills

The boundary theory in the canonical AdS/CFT example is four-dimensional N=4\mathcal N=4 super-Yang-Mills theory with gauge group SU(N)SU(N). It is the low-energy interacting theory on NN coincident D3-branes after the decoupled center-of-mass U(1)U(1) sector is removed.

This theory is special for three closely related reasons.

First, it is a four-dimensional conformal field theory with a Lagrangian. The coupling does not run, so the theory exists as a continuous family of CFTs labeled by the complexified gauge coupling

τYM=θ2π+4πigYM2.\tau_{\mathrm{YM}} = \frac{\theta}{2\pi} + \frac{4\pi i}{g_{\mathrm{YM}}^2}.

Second, it is maximally supersymmetric without gravity. In four-dimensional notation it has 1616 Poincare supercharges and, because it is conformal, 1616 conformal supercharges. Together with the conformal group and R-symmetry, these generate the superconformal algebra

psu(2,24).\mathfrak{psu}(2,2|4).

Third, it is a large-NN matrix CFT. Gauge-invariant single-trace operators behave like single-particle bulk fields, multi-trace operators behave like multiparticle states, and large-NN factorization is the field-theory origin of semiclassical bulk physics.

Field content and holographic role of N=4 super-Yang-Mills theory

The elementary fields of N=4\mathcal N=4 SU(N)SU(N) super-Yang-Mills form one adjoint vector multiplet. The six scalars transform as the vector of SO(6)RSU(4)RSO(6)_R\simeq SU(4)_R, matching the rotations of the six transverse directions to the D3-branes and the isometries of S5S^5 in the dual geometry.

This page is not trying to teach supersymmetric gauge theory from scratch. The goal is to isolate exactly what an AdS/CFT user needs to know about N=4\mathcal N=4 SYM: its fields, action, symmetries, parameters, operator spectrum, and large-NN dictionary.

A single D3-brane fills four directions and sits at a point in six transverse directions. The massless open-string modes on the brane are:

ModeFour-dimensional fieldMeaning
open-string vector polarization along the braneAμA_\mugauge field on the D3-brane
transverse oscillationsΦI\Phi^I, I=1,,6I=1,\ldots,6position of the brane in R6\mathbb R^6
fermionic partnersλαA\lambda^A_\alpha, A=1,,4A=1,\ldots,4superpartners required by type IIB supersymmetry

For NN coincident D3-branes, Chan-Paton labels turn these fields into N×NN\times N matrices. The full low-energy gauge group is U(N)U(N), but the overall U(1)U(1) describes the free center-of-mass motion of the brane stack. The interacting theory used in AdS/CFT is usually the SU(N)SU(N) part:

U(N)SU(N)×U(1)ZN,interacting sector: SU(N).U(N)\simeq \frac{SU(N)\times U(1)}{\mathbb Z_N}, \qquad \text{interacting sector: }SU(N).

The six scalar matrices are especially important. If they acquire mutually commuting expectation values, their eigenvalues describe the positions of the individual D3-branes in the transverse R6\mathbb R^6. The conformal point dual to AdS5×S5\mathrm{AdS}_5\times S^5 is the point where all scalar expectation values vanish and the branes are coincident.

In four-dimensional N=4\mathcal N=4 notation, the interacting theory contains the following fields, all in the adjoint representation of SU(N)SU(N):

FieldSpinMultiplicitySU(4)RSU(4)_R representationOn-shell degrees of freedom per color
AμA_\mu11111{\bf 1}22
λαA\lambda^A_\alpha1/21/244 Weyl fermions4{\bf 4}88 real fermionic
ΦI\Phi^I0066 real scalars6{\bf 6}66

The bosonic on-shell count is

2+6=8,2+6=8,

and the fermionic on-shell count is

4×2=8.4\times 2=8.

The equality is the first quick check that the fields can form a supersymmetric multiplet. The deeper statement is that this is the unique four-dimensional gauge multiplet with maximal supersymmetry and no spin larger than one.

The R-symmetry has two useful descriptions:

SO(6)RSU(4)R.SO(6)_R \simeq SU(4)_R.

The six real scalars transform as the vector 6{\bf 6} of SO(6)RSO(6)_R, or equivalently the antisymmetric representation of SU(4)RSU(4)_R. The four Weyl fermions transform as the fundamental 4{\bf 4} of SU(4)RSU(4)_R. In the D3-brane construction, this SO(6)RSO(6)_R is simply the rotation group of the six directions transverse to the branes. In the gravity dual, it becomes the isometry group of S5S^5:

SO(6)RIsom(S5).SO(6)_R \quad\longleftrightarrow\quad \mathrm{Isom}(S^5).

A compact way to write the theory is to start from ten-dimensional N=1\mathcal N=1 super-Yang-Mills and dimensionally reduce to four dimensions. Let M,N=0,,9M,N=0,\ldots,9 and let AMA_M be a ten-dimensional gauge field. Reducing on six flat directions means that the fields do not depend on x4,,x9x^4,\ldots,x^9, so

AM(Aμ,ΦI),μ=0,,3,I=1,,6.A_M \longrightarrow (A_\mu,\Phi^I), \qquad \mu=0,\ldots,3, \qquad I=1,\ldots,6.

The ten-dimensional field strength contains

Fμν,FμI=DμΦI,FIJ=i[ΦI,ΦJ],F_{\mu\nu}, \qquad F_{\mu I}=D_\mu \Phi^I, \qquad F_{IJ}=-i[\Phi^I,\Phi^J],

where the factor of ii depends on whether the Lie-algebra generators are taken Hermitian or anti-Hermitian. This immediately produces the schematic bosonic action

Sbos=1gYM2d4xTr[14FμνFμν12DμΦIDμΦI+14[ΦI,ΦJ]2]+θ8π2TrFF.S_{\mathrm{bos}} = \frac{1}{g_{\mathrm{YM}}^2} \int d^4x\, \operatorname{Tr} \left[ -\frac14 F_{\mu\nu}F^{\mu\nu} -\frac12 D_\mu\Phi^I D^\mu\Phi^I +\frac14[\Phi^I,\Phi^J]^2 \right] + \frac{\theta}{8\pi^2} \int \operatorname{Tr}F\wedge F.

The full theory also contains fermion kinetic terms and Yukawa couplings of the schematic form

Tr(iλˉγμDμλ+λˉΓI[ΦI,λ]).\operatorname{Tr} \left( i\bar\lambda \gamma^\mu D_\mu\lambda + \bar\lambda \Gamma_I[\Phi^I,\lambda] \right).

The relative coefficients are not optional. Supersymmetry fixes the gauge interactions, scalar quartic interactions, and Yukawa interactions in terms of one coupling gYMg_{\mathrm{YM}}.

A useful way to remember the interactions is:

interactions vanish on the Coulomb branch[ΦI,ΦJ]=0.\text{interactions vanish on the Coulomb branch} \quad \Longleftrightarrow \quad [\Phi^I,\Phi^J]=0.

When the scalar matrices commute, they can be diagonalized simultaneously. Their eigenvalues are the separated D3-brane positions.

Convention warning: where the factors of 2π2\pi hide

Section titled “Convention warning: where the factors of 2π2\pi2π hide”

The D3-brane literature uses several normalizations for gYMg_{\mathrm{YM}}. In this course we follow the convention already used in the D3-brane page:

gYM2=4πgs,λ=gYM2N=4πgsN.g_{\mathrm{YM}}^2=4\pi g_s, \qquad \lambda=g_{\mathrm{YM}}^2N=4\pi g_sN.

Then the type IIB axio-dilaton and the Yang-Mills coupling combine naturally as

τIIB=C0+ieϕτYM=θ2π+4πigYM2,\tau_{\mathrm{IIB}} = C_0+i e^{-\phi} \quad\longleftrightarrow\quad \tau_{\mathrm{YM}} = \frac{\theta}{2\pi} + \frac{4\pi i}{g_{\mathrm{YM}}^2},

with the identification

C0=θ2π,eϕ=gs=gYM24π.C_0=\frac{\theta}{2\pi}, \qquad e^\phi=g_s=\frac{g_{\mathrm{YM}}^2}{4\pi}.

Other authors absorb factors of 2π2\pi differently. Do not compare formulas for gYM2g_{\mathrm{YM}}^2, L4/α2L^4/\alpha'^2, or τ\tau across references unless you first check the normalization of the Yang-Mills action and the trace.

The robust physical statements are:

L4α2λ,gsλN,L3G5N2.\frac{L^4}{\alpha'^2}\sim \lambda, \qquad g_s\sim \frac{\lambda}{N}, \qquad \frac{L^3}{G_5}\sim N^2.

The next two pages will fix the detailed version of these relations in the conventions of the course.

Classically, the Yang-Mills coupling is dimensionless in four dimensions. Quantum mechanically, most gauge theories develop a scale through renormalization. N=4\mathcal N=4 SYM is exceptional: its beta function vanishes.

At one loop, the coefficient of the Yang-Mills beta function for adjoint matter is proportional to

b0=113CA23nWeylCA16nrealCA.b_0 = \frac{11}{3}C_A - \frac{2}{3}n_{\mathrm{Weyl}}C_A - \frac{1}{6}n_{\mathrm{real}}C_A.

For N=4\mathcal N=4 SYM,

nWeyl=4,nreal=6,n_{\mathrm{Weyl}}=4, \qquad n_{\mathrm{real}}=6,

so

b0=(113831)CA=0.b_0 = \left( \frac{11}{3} - \frac{8}{3} - 1 \right)C_A =0.

Supersymmetry strengthens this one-loop cancellation into exact conformal invariance. The theory therefore has no intrinsic mass scale on R1,3\mathbb R^{1,3} at the conformal point. The only scales in observables come from sources, temperature, chemical potential, compactification radii, operator insertions, or chosen states.

This is why the canonical dual is pure AdS5×S5\mathrm{AdS}_5\times S^5 rather than a geometry with a running radial profile. A running coupling would correspond to a nontrivial radial dependence of bulk scalar fields.

The bosonic conformal group in four-dimensional Minkowski space is

SO(2,4).SO(2,4).

The R-symmetry is

SO(6)RSU(4)R.SO(6)_R\simeq SU(4)_R.

Including supersymmetry, the full superconformal group is

PSU(2,24),PSU(2,2|4),

whose bosonic subgroup is

SO(2,4)×SU(4)R.SO(2,4)\times SU(4)_R.

On the gravity side,

SO(2,4)Isom(AdS5),SO(2,4) \quad\longleftrightarrow\quad \mathrm{Isom}(\mathrm{AdS}_5),

and

SO(6)Isom(S5).SO(6) \quad\longleftrightarrow\quad \mathrm{Isom}(S^5).

Thus the spacetime symmetries of the bulk geometry already know about the conformal and R-symmetries of the boundary theory.

This symmetry matching is one of the cleanest first tests of the canonical duality:

AdS5×S5has isometrySO(2,4)×SO(6),\mathrm{AdS}_5\times S^5 \quad\text{has isometry}\quad SO(2,4)\times SO(6),

while N=4\mathcal N=4 SYM has bosonic global symmetry

SO(2,4)×SO(6)R.SO(2,4)\times SO(6)_R.

The match is not decorative. It determines the representation theory of protected operators and organizes the Kaluza-Klein spectrum on S5S^5.

The exactly marginal coupling and S-duality

Section titled “The exactly marginal coupling and S-duality”

The complex coupling

τ=θ2π+4πigYM2\tau = \frac{\theta}{2\pi} + \frac{4\pi i}{g_{\mathrm{YM}}^2}

is exactly marginal. Moving τ\tau changes the CFT but does not break conformal invariance. In the canonical AdS/CFT example, this continuous conformal manifold maps to the constant type IIB axio-dilaton.

The theory is also expected to have an SL(2,Z)SL(2,\mathbb Z) duality action

τaτ+bcτ+d,(abcd)SL(2,Z),\tau \longrightarrow \frac{a\tau+b}{c\tau+d}, \qquad \begin{pmatrix} a & b\\ c & d \end{pmatrix} \in SL(2,\mathbb Z),

together with the appropriate action on line operators and, more carefully, on the global form of the gauge group. The generator

S:τ1τS:\tau\mapsto -\frac{1}{\tau}

exchanges electric and magnetic descriptions. In type IIB string theory, the same SL(2,Z)SL(2,\mathbb Z) is the nonperturbative duality acting on the axio-dilaton and on fundamental/D-string charges.

For most classical supergravity calculations, S-duality is not the first thing one uses. But conceptually it is a powerful warning: N=4\mathcal N=4 SYM is not merely a weakly coupled gauge theory with many symmetries. It is a nonperturbative quantum theory with multiple equivalent descriptions.

The two parameters most often used in holography are

N,λ=gYM2N.N, \qquad \lambda=g_{\mathrm{YM}}^2N.

The ‘t Hooft large-NN limit is

N,λ fixed.N\to\infty, \qquad \lambda\ \text{fixed}.

In perturbation theory, each planar diagram contributes a function of λ\lambda, and nonplanar diagrams are suppressed by powers of 1/N21/N^2. Holographically,

1N2counts bulk loops,\frac{1}{N^2} \quad\text{counts bulk loops},

while

1λcounts stringy curvature corrections\frac{1}{\sqrt{\lambda}} \quad\text{counts stringy curvature corrections}

in the canonical AdS5×S5\mathrm{AdS}_5\times S^5 background.

The classical Einstein-gravity limit requires both

N1,λ1.N\gg 1, \qquad \lambda\gg 1.

This is one of the most important lessons of the canonical example. The field theory is easiest at weak coupling λ1\lambda\ll1, while the bulk gravity description is easiest at strong coupling λ1\lambda\gg1. The duality is powerful precisely because it relates difficult field-theory questions to easier gravitational ones.

The elementary fields AμA_\mu, λ\lambda, and ΦI\Phi^I are not gauge-invariant local observables. Physical local operators are gauge-invariant combinations, especially traces of adjoint fields.

A basic class is

OkI1Ik=Tr(Φ(I1ΦIk))traces,\mathcal O_k^{I_1\cdots I_k} = \operatorname{Tr} \left( \Phi^{(I_1}\cdots\Phi^{I_k)} \right) -\text{traces},

where the parentheses indicate symmetrization in SO(6)RSO(6)_R indices and subtracting traces makes the operator transform in a symmetric traceless representation of SO(6)RSO(6)_R.

These are chiral primary operators. Their dimensions are protected:

Δ=k.\Delta=k.

The lowest nontrivial example is

O2IJ=Tr(ΦIΦJ16δIJΦKΦK),\mathcal O_2^{IJ} = \operatorname{Tr} \left( \Phi^I\Phi^J-\frac16\delta^{IJ}\Phi^K\Phi^K \right),

which transforms in the 20{\bf 20'} of SU(4)RSU(4)_R and lies in the same supermultiplet as the stress tensor.

The contrast with the Konishi operator is instructive. The schematic operator

K=Tr(ΦIΦI)\mathcal K = \operatorname{Tr}(\Phi^I\Phi^I)

is an SU(4)RSU(4)_R singlet and is not protected. Its dimension depends on λ\lambda:

ΔK=2+O(λ)(λ1),\Delta_{\mathcal K} = 2+O(\lambda) \quad (\lambda\ll1),

while at strong coupling it becomes a stringy excitation whose dimension grows parametrically. This is an early glimpse of the distinction between supergravity modes and massive string modes.

Single-trace, multi-trace, and bulk particles

Section titled “Single-trace, multi-trace, and bulk particles”

For matrix fields, single-trace operators are the natural large-NN building blocks:

Tr(Φk),Tr(FμνΦk),Tr(λλΦk),Tr(FμνFμνΦk),\operatorname{Tr}(\Phi^k), \qquad \operatorname{Tr}(F_{\mu\nu}\Phi^k), \qquad \operatorname{Tr}(\lambda\lambda\Phi^k), \qquad \operatorname{Tr}(F_{\mu\nu}F^{\mu\nu}\Phi^k), \quad \ldots

Very schematically,

single-trace primarysingle-particle bulk field.\text{single-trace primary} \quad\longleftrightarrow\quad \text{single-particle bulk field}.

Products of traces correspond to multiparticle states:

O1O2two-particle bulk state.\mathcal O_1\mathcal O_2 \quad\longleftrightarrow\quad \text{two-particle bulk state}.

At infinite NN, multi-trace dimensions are approximately additive:

ΔO1O2=ΔO1+ΔO2+O ⁣(1N2).\Delta_{\mathcal O_1\mathcal O_2} = \Delta_{\mathcal O_1} + \Delta_{\mathcal O_2} + O\!\left(\frac{1}{N^2}\right).

This is the CFT version of the statement that weakly interacting particles in the bulk have energies that add.

The word “single-trace” is most natural for SU(N)SU(N) or U(N)U(N) matrix theories. In a more abstract CFT, one should say “single-particle” or “single-string” operators. But for N=4\mathcal N=4 SYM, the trace language is both literal and useful.

Every CFT has a stress tensor TμνT_{\mu\nu} with protected dimension

ΔT=d=4.\Delta_T=d=4.

In N=4\mathcal N=4 SYM, the stress tensor belongs to a protected supermultiplet whose bottom component is the dimension-two chiral primary O2IJ\mathcal O_2^{IJ} above.

The four-dimensional Weyl anomaly on a curved background takes the schematic form

Tμμ=c16π2WμνρσWμνρσa16π2E4+,\langle T^\mu{}_\mu\rangle = \frac{c}{16\pi^2}W_{\mu\nu\rho\sigma}W^{\mu\nu\rho\sigma} - \frac{a}{16\pi^2}E_4 +\cdots,

where E4E_4 is the Euler density and the dots denote possible background-gauge-field terms and scheme-dependent total derivatives.

For N=4\mathcal N=4 SYM with gauge algebra su(N)\mathfrak{su}(N),

a=c=N214a=c=\frac{N^2-1}{4}

in the common convention where a free real scalar has

ascalar=1360,cscalar=1120.a_{\mathrm{scalar}}=\frac{1}{360}, \qquad c_{\mathrm{scalar}}=\frac{1}{120}.

The large-NN scaling

acN2a\sim c\sim N^2

is the field-theory origin of

L3G5N2.\frac{L^3}{G_5}\sim N^2.

In holography, CTC_T, aa, cc, and L3/G5L^3/G_5 are different normalizations of the same central idea: the number of stress-tensor degrees of freedom is of order N2N^2.

The scalar potential is proportional to

V(Φ)Tr[ΦI,ΦJ]2,V(\Phi) \propto \operatorname{Tr} [\Phi^I,\Phi^J]^2,

with the sign chosen so that the energy is nonnegative. Its minima satisfy

[ΦI,ΦJ]=0for all I,J.[\Phi^I,\Phi^J]=0 \qquad \text{for all } I,J.

For Hermitian scalar matrices, commuting matrices can be diagonalized simultaneously:

ΦI=diag(x1I,,xNI),\Phi^I = \operatorname{diag} \left( x_1^I,\ldots,x_N^I \right),

up to gauge transformations and subject to the tracelessness condition for SU(N)SU(N). The eigenvalue vector

xa=(xa1,,xa6)\vec x_a=(x_a^1,\ldots,x_a^6)

is the position of the aa-th D3-brane in the transverse R6\mathbb R^6.

For U(N)U(N), the classical moduli space is

MU(N)=(R6)NSN,\mathcal M_{U(N)} = \frac{(\mathbb R^6)^N}{S_N},

where the symmetric group permutes identical branes. For SU(N)SU(N), the center-of-mass coordinate is removed:

a=1Nxa=0.\sum_{a=1}^N \vec x_a=0.

The conformal vacuum dual to AdS5×S5\mathrm{AdS}_5\times S^5 sits at the origin of this moduli space:

x1==xN=0.\vec x_1=\cdots=\vec x_N=0.

Moving onto the Coulomb branch breaks the gauge group and changes the bulk geometry. It should not be confused with changing the state of the same exact AdS5×S5\mathrm{AdS}_5\times S^5 background.

Line operators and the global form of the gauge group

Section titled “Line operators and the global form of the gauge group”

For many local-operator calculations, it is enough to say “gauge group SU(N)SU(N).” For line operators and S-duality, the global form matters.

The Lie algebra su(N)\mathfrak{su}(N) can correspond to different global gauge groups, such as

SU(N),SU(N)/ZN,SU(N), \qquad SU(N)/\mathbb Z_N,

with different allowed Wilson and ‘t Hooft line operators. In the string dual, Wilson lines are represented by fundamental strings ending on the boundary, while magnetic line operators are related to D-strings. The SL(2,Z)SL(2,\mathbb Z) duality rotates these line operators.

This subtlety is not needed for the first derivation of the correspondence, but it becomes important in serious discussions of S-duality, one-form symmetries, confinement diagnostics, and the precise classification of boundary conditions.

It is tempting to think of N=4\mathcal N=4 SYM as “QCD but supersymmetric.” That slogan is too crude.

FeatureN=4\mathcal N=4 SYMQCD-like theory
Matteradjoint scalars and fermionsfundamental quarks, gluons
Supersymmetrymaximalnone in real QCD
Couplingexactly marginalruns with scale
Vacuum at originconformalconfining/chiral symmetry breaking in QCD
Degrees of freedom at large NNO(N2)O(N^2) adjointgluons O(N2)O(N^2), quarks often O(N)O(N) in the ‘t Hooft limit
Best classical gravity regimelarge NN, large λ\lambdano known exact classical gravity dual for real QCD

The point of N=4\mathcal N=4 SYM is not realism. It is control. It is an exactly defined interacting CFT that admits a string-theoretic dual and, in a strong-coupling large-NN regime, a classical gravitational description.

Many later holographic models deform or generalize this example to study confinement, flavor, finite density, hydrodynamics, and condensed-matter-like phenomena. But the canonical example is the calibration point. It teaches which results are universal consequences of gravity, which depend on supersymmetry or conformality, and which are merely model-building assumptions.

The next pages will build the bulk side and the precise parameter map. For now, the basic entries are:

N=4\mathcal N=4 SYMType IIB on AdS5×S5\mathrm{AdS}_5\times S^5
SU(N)SU(N) rankNN units of five-form flux through S5S^5
SO(2,4)SO(2,4) conformal symmetryAdS5\mathrm{AdS}_5 isometry
SO(6)RSU(4)RSO(6)_R\simeq SU(4)_RS5S^5 isometry
τYM\tau_{\mathrm{YM}}type IIB axio-dilaton τIIB\tau_{\mathrm{IIB}}
λ=gYM2N\lambda=g_{\mathrm{YM}}^2Nstring tension in AdS units, L2/αλL^2/\alpha'\sim \sqrt\lambda
1/N21/N^2bulk quantum-loop expansion
single-trace operatorssingle-particle/string states
chiral primariesKaluza-Klein supergravity modes on S5S^5
stress tensor TμνT_{\mu\nu}graviton in AdS5\mathrm{AdS}_5
R-current Jμ[IJ]J_\mu^{[IJ]}gauge fields from S5S^5 isometries

This table is deliberately schematic. The exact coefficients and normalization conventions are the subject of the next two pages.

Mistake 1: Treating N=4\mathcal N=4 SYM as weakly coupled in the gravity regime.
The classical gravity limit requires λ1\lambda\gg1, where ordinary perturbation theory in gYMg_{\mathrm{YM}} is not useful, even though gYM2=λ/Ng_{\mathrm{YM}}^2=\lambda/N may be small at large NN.

Mistake 2: Forgetting the decoupled U(1)U(1).
The D3-brane worldvolume theory is naturally U(N)U(N), but the interacting AdS/CFT dual usually refers to the SU(N)SU(N) sector. The overall U(1)U(1) is a free center-of-mass multiplet.

Mistake 3: Confusing elementary fields with local CFT observables.
The scalar ΦI\Phi^I is not a gauge-invariant local operator. Operators like Tr(ΦIΦJ)\operatorname{Tr}(\Phi^I\Phi^J) are.

Mistake 4: Thinking all operator dimensions are protected.
Chiral primaries and conserved currents have protected dimensions. Generic single-trace operators, such as the Konishi operator, acquire anomalous dimensions and become heavy at strong coupling.

Mistake 5: Ignoring the global form of the gauge group.
For local single-trace correlators, the Lie algebra often suffices. For line operators, S-duality, one-form symmetries, and precise nonperturbative statements, the global form matters.

Mistake 6: Equating conformality with triviality.
The theory is conformal for all τ\tau, but it is still interacting. A CFT can have nontrivial anomalous dimensions, OPE coefficients, thermal physics, and transport.

Show that the N=4\mathcal N=4 vector multiplet has equal bosonic and fermionic on-shell degrees of freedom per generator of the gauge algebra.

Solution

A massless four-dimensional gauge field has two physical polarizations. The six real scalars contribute six bosonic degrees of freedom. Hence

nbos=2+6=8.n_{\mathrm{bos}}=2+6=8.

A four-dimensional Weyl fermion has two real on-shell degrees of freedom. There are four Weyl fermions, so

nferm=4×2=8.n_{\mathrm{ferm}}=4\times 2=8.

Thus the on-shell bosonic and fermionic degrees of freedom match:

nbos=nferm=8.n_{\mathrm{bos}}=n_{\mathrm{ferm}}=8.

All fields are adjoint-valued, so this count is multiplied by dimSU(N)=N21\dim SU(N)=N^2-1 for the interacting SU(N)SU(N) theory.

Exercise 2: One-loop beta-function cancellation

Section titled “Exercise 2: One-loop beta-function cancellation”

Using

b0=113CA23nWeylCA16nrealCA,b_0 = \frac{11}{3}C_A - \frac{2}{3}n_{\mathrm{Weyl}}C_A - \frac{1}{6}n_{\mathrm{real}}C_A,

show that the one-loop beta function vanishes for N=4\mathcal N=4 SYM.

Solution

For N=4\mathcal N=4 SYM, all matter fields are in the adjoint representation, so they carry the same group factor CAC_A as the gauge boson. There are

nWeyl=4,nreal=6.n_{\mathrm{Weyl}}=4, \qquad n_{\mathrm{real}}=6.

Therefore

b0=(113234166)CA.b_0 = \left( \frac{11}{3} - \frac{2}{3}\cdot 4 - \frac{1}{6}\cdot 6 \right)C_A.

This is

b0=(113831)CA=0.b_0 = \left( \frac{11}{3} - \frac{8}{3} - 1 \right)C_A = 0.

The one-loop cancellation is a quick perturbative signal of conformality. In the full theory, extended supersymmetry implies exact vanishing of the beta function.

Exercise 3: The Coulomb-branch moduli space

Section titled “Exercise 3: The Coulomb-branch moduli space”

Assume the scalar fields ΦI\Phi^I are Hermitian matrices and the potential is minimized when

[ΦI,ΦJ]=0for all I,J.[\Phi^I,\Phi^J]=0 \qquad \text{for all }I,J.

Explain why the classical moduli space for the U(N)U(N) theory is

MU(N)=(R6)NSN.\mathcal M_{U(N)} = \frac{(\mathbb R^6)^N}{S_N}.
Solution

If the six Hermitian matrices ΦI\Phi^I commute pairwise, they can be diagonalized simultaneously by a unitary gauge transformation. We can write

ΦI=diag(x1I,,xNI).\Phi^I = \operatorname{diag} (x_1^I,\ldots,x_N^I).

For each eigenvalue label a=1,,Na=1,\ldots,N, the six numbers

xa=(xa1,,xa6)\vec x_a=(x_a^1,\ldots,x_a^6)

define a point in R6\mathbb R^6. Thus a generic commuting configuration describes NN points in R6\mathbb R^6.

The remaining Weyl group of U(N)U(N) permutes the eigenvalues. Since the D3-branes are identical, configurations related by permutations are gauge-equivalent. Therefore

MU(N)=(R6)NSN.\mathcal M_{U(N)} = \frac{(\mathbb R^6)^N}{S_N}.

For SU(N)SU(N), one removes the center-of-mass coordinate by imposing

a=1Nxa=0.\sum_{a=1}^N \vec x_a=0.

Exercise 4: Central charges from free fields

Section titled “Exercise 4: Central charges from free fields”

Use the free-field anomaly coefficients

as=1360,af=11720,av=31180a_s=\frac{1}{360}, \qquad a_f=\frac{11}{720}, \qquad a_v=\frac{31}{180}

for a real scalar, Weyl fermion, and vector field, respectively. Show that one N=4\mathcal N=4 vector multiplet has

a=14.a=\frac14.

Then infer the value for gauge algebra su(N)\mathfrak{su}(N).

Solution

One N=4\mathcal N=4 vector multiplet contains one vector, four Weyl fermions, and six real scalars. Therefore

aN=4=av+4af+6as.a_{\mathcal N=4} = a_v+4a_f+6a_s.

Substituting the given values,

aN=4=31180+411720+61360.a_{\mathcal N=4} = \frac{31}{180} + 4\cdot\frac{11}{720} + 6\cdot\frac{1}{360}.

With denominator 720720,

aN=4=124720+44720+12720=180720=14.a_{\mathcal N=4} = \frac{124}{720} + \frac{44}{720} + \frac{12}{720} = \frac{180}{720} = \frac14.

For gauge algebra su(N)\mathfrak{su}(N), this is multiplied by

dimSU(N)=N21.\dim SU(N)=N^2-1.

Thus

a=N214.a=\frac{N^2-1}{4}.

Supersymmetry also gives

c=a=N214.c=a=\frac{N^2-1}{4}.

Exercise 5: Which operators are light at strong coupling?

Section titled “Exercise 5: Which operators are light at strong coupling?”

Classify the following schematic single-trace operators as protected or generally unprotected:

Tr ⁣(Φ(IΦJ)traces),Tr(ΦIΦI),Tμν,TrΦ(I1ΦIk)traces.\operatorname{Tr}\!\left(\Phi^{(I}\Phi^{J)}-\text{traces}\right), \qquad \operatorname{Tr}(\Phi^I\Phi^I), \qquad T_{\mu\nu}, \qquad \operatorname{Tr}\Phi^{(I_1}\cdots\Phi^{I_k)}-\text{traces}.

Explain what this means for the bulk dual at λ1\lambda\gg1.

Solution

The symmetric traceless scalar operators

Tr ⁣(Φ(IΦJ)traces)\operatorname{Tr}\!\left(\Phi^{(I}\Phi^{J)}-\text{traces}\right)

and more generally

TrΦ(I1ΦIk)traces\operatorname{Tr}\Phi^{(I_1}\cdots\Phi^{I_k)}-\text{traces}

are chiral primaries. Their dimensions are protected, with

Δ=k.\Delta=k.

The stress tensor TμνT_{\mu\nu} is also protected because it is conserved, and every conserved stress tensor in a four-dimensional CFT has

ΔT=4.\Delta_T=4.

The Konishi operator

Tr(ΦIΦI)\operatorname{Tr}(\Phi^I\Phi^I)

is generally unprotected. Its dimension depends on the coupling and becomes large at strong ‘t Hooft coupling.

In the bulk dual, protected operators correspond to light supergravity modes or their Kaluza-Klein excitations on S5S^5. Unprotected generic single-trace operators correspond to stringy states whose masses in AdS units grow when λ1\lambda\gg1.