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N=4 Super-Yang-Mills

The canonical example of AdS/CFT begins with one very special four-dimensional quantum field theory:

N=4  SU(N)  super-Yang–Mills theory.\mathcal N=4\; SU(N)\; \text{super-Yang–Mills theory}.

It is the boundary theory in the duality

N=4  SU(N)  SYM in d=4type IIB string theory on AdS5×S5.\mathcal N=4\; SU(N)\; \text{SYM in } d=4 \quad \longleftrightarrow \quad \text{type IIB string theory on } \mathrm{AdS}_5\times S^5 .

This page explains what an AdS/CFT user needs to know about this theory. We will not develop supersymmetric gauge theory from scratch. Instead, we isolate the structural facts that make N=4\mathcal N=4 SYM the cleanest laboratory for holography: it is conformal, it is a large-NN matrix theory, all fields are adjoint-valued, its symmetries match the geometry of AdS5×S5\mathrm{AdS}_5\times S^5, and its two dimensionless parameters become bulk string-theory parameters.

The most important moral is this:

large N controls bulk quantum effects,large λ=gYM2N controls stringy curvature corrections.\text{large } N \text{ controls bulk quantum effects}, \qquad \text{large } \lambda=g_{\mathrm{YM}}^2N \text{ controls stringy curvature corrections}.

So N=4\mathcal N=4 SYM is not merely a historical example. It is the prototype from which much of the holographic dictionary is learned.

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

The canonical AdS5_5/CFT4_4 example is organized by a tight matching of field-theory data and bulk data. The adjoint fields of N=4\mathcal N=4 SYM generate gauge-invariant operators; the conformal and R-symmetry groups become the isometry groups of AdS5\mathrm{AdS}_5 and S5S^5; and the parameters NN and λ\lambda become flux, curvature, and loop-expansion data in the bulk.

The previous pages explained the field-theory ingredients needed for holography: conformal symmetry, radial quantization, large-NN counting, single-trace operators, and large-NN factorization. N=4\mathcal N=4 SYM is where those ingredients come together in a real, fully defined quantum field theory.

It has three properties that are individually important and collectively extraordinary.

First, it is a four-dimensional conformal field theory with a Lagrangian. This gives us a familiar starting point: fields, an action, gauge symmetry, local operators, and a path integral.

Second, it is a large-NN matrix theory. All elementary fields transform in the adjoint representation of the gauge group, so gauge-invariant operators naturally organize into traces. This is exactly the structure needed for the single-trace/multi-trace dictionary.

Third, it is maximally supersymmetric without including gravity. Supersymmetry protects many quantities, forces the beta function to vanish, and gives enough analytic control that the theory can be compared sharply to string theory.

The result is a rare situation: a nontrivial interacting QFT that is exactly conformal, has a controllable large-NN limit, and has a known string-theory construction.

There is an annoying but unavoidable notation issue.

The symbol NN in SU(N)SU(N) is the number of colors. It controls the size of matrices and the number of degrees of freedom. This is the NN that appears in large-NN holography.

The symbol N\mathcal N in N=4\mathcal N=4 counts supersymmetry in four-dimensional notation. It does not mean four colors. It means that the theory has four copies of the minimal four-dimensional supersymmetry algebra. Equivalently, it has

1616

Poincaré supercharges. Because the theory is conformal, these are accompanied by another 1616 superconformal charges. Together with conformal symmetry and R-symmetry, they form the superconformal algebra

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

So the full phrase

N=4  SU(N)  SYM\mathcal N=4\; SU(N)\; \text{SYM}

contains two different pieces of information: maximal supersymmetry and color rank NN.

The elementary fields form one adjoint vector multiplet. In four-dimensional language they are:

FieldNumberRepresentation under SU(N)SU(N)Simple meaning
AμA_\mu11 gauge fieldadjointYang–Mills gauge field
ΦI\Phi^I, I=1,,6I=1,\ldots,666 real scalarsadjointtransverse D3-brane fluctuations
λαA\lambda^A_\alpha, A=1,,4A=1,\ldots,444 Weyl fermionsadjointsuperpartners

More explicitly, the fields are matrices:

Aμ(x)=Aμa(x)Ta,ΦI(x)=ΦI,a(x)Ta,λαA(x)=λαA,a(x)Ta,A_\mu(x)=A_\mu^a(x)T^a, \qquad \Phi^I(x)=\Phi^{I,a}(x)T^a, \qquad \lambda^A_\alpha(x)=\lambda^{A,a}_\alpha(x)T^a,

where TaT^a are generators of su(N)\mathfrak{su}(N) and

a=1,,N21.a=1,\ldots,N^2-1.

This adjoint matrix structure is the reason large-NN counting works so naturally. Every propagator carries two color lines, and gauge-invariant local operators are built by tracing matrix products.

The six scalars transform as the vector representation of

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

which is the R-symmetry of the theory. This symmetry will later become the isometry group of the S5S^5 in the bulk geometry.

Suppressing spinor indices and convention-dependent signs, the Euclidean action has the schematic form

SE=1gYM2d4xTr[14FμνFμν+12DμΦIDμΦI+14I,J[ΦI,ΦJ][ΦI,ΦJ]+fermion kinetic terms+Yukawa terms]+iθ8π2TrFF.S_E = \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\sum_{I,J} [\Phi^I,\Phi^J]^\dagger[\Phi^I,\Phi^J] + \text{fermion kinetic terms} + \text{Yukawa terms} \right] + i\frac{\theta}{8\pi^2}\int \operatorname{Tr} F\wedge F .

The exact coefficients in the fermion and Yukawa terms are fixed by supersymmetry. The important structural points are:

  1. all fields are adjoint-valued matrices;
  2. all interactions are controlled by one gauge coupling gYMg_{\mathrm{YM}};
  3. the scalar potential vanishes when the scalars commute;
  4. the theory also has a topological theta angle θ\theta.

The field strength and covariant derivative are

Fμν=μAννAμ+[Aμ,Aν],DμΦI=μΦI+[Aμ,ΦI].F_{\mu\nu} = \partial_\mu A_\nu- \partial_\nu A_\mu+[A_\mu,A_\nu], \qquad D_\mu\Phi^I = \partial_\mu\Phi^I+[A_\mu,\Phi^I].

For many holographic questions, one does not need the full component action. What matters is the symmetry, the matrix structure, the coupling dependence, and the operator content.

Four-dimensional Yang–Mills theory has a classically dimensionless coupling. In ordinary nonsupersymmetric Yang–Mills theory, quantum effects make the coupling run. In N=4\mathcal N=4 SYM, the beta function vanishes exactly:

β(gYM)=0.\beta(g_{\mathrm{YM}})=0.

Thus the theory is not merely scale invariant at tree level. It is an exact quantum conformal field theory.

The two parameters usually used in AdS/CFT are the complexified gauge coupling

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

and the ‘t Hooft coupling

λ=gYM2N.\lambda=g_{\mathrm{YM}}^2N.

The large-NN limit is taken with λ\lambda held fixed:

N,λ=gYM2N  fixed.N\to\infty, \qquad \lambda=g_{\mathrm{YM}}^2N\;\text{fixed}.

This is the limit in which planar diagrams dominate. In the canonical holographic example, the gravity description becomes weakly curved when

λ1.\lambda\gg 1.

This is one of the great inversions of AdS/CFT. Perturbative field theory is easy when λ1\lambda\ll 1, but classical gravity is easy when λ1\lambda\gg 1.

For type IIB string theory on AdS5×S5\mathrm{AdS}_5\times S^5, the standard relations are convention-dependent in factors of 2π2\pi. A common convention gives

gYM2=4πgs,L4=4πgsNα2,g_{\mathrm{YM}}^2 = 4\pi g_s, \qquad L^4 = 4\pi g_s N\alpha'^2,

and therefore

L4α2=λ.\frac{L^4}{\alpha'^2}=\lambda.

Here LL is the common radius of AdS5\mathrm{AdS}_5 and S5S^5, gsg_s is the string coupling, and α\alpha' is the square of the string length.

The practical dictionary is:

λ1L2αsmall stringy curvature corrections,\lambda \gg 1 \quad\Longleftrightarrow\quad L^2\gg \alpha' \quad\Longleftrightarrow\quad \text{small stringy curvature corrections},

while

N1small bulk quantum corrections.N\gg 1 \quad\Longleftrightarrow\quad \text{small bulk quantum corrections}.

More precisely, the five-dimensional Newton constant satisfies

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

This is the gravitational version of the fact that N=4\mathcal N=4 SYM has order N2N^2 degrees of freedom.

The symmetry matching is one of the cleanest pieces of evidence for the duality.

The conformal group of four-dimensional Minkowski space is

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

up to global and covering-group subtleties. The isometry group of AdS5\mathrm{AdS}_5 is also

Isom(AdS5)=SO(2,4).\operatorname{Isom}(\mathrm{AdS}_5)=SO(2,4).

The R-symmetry group of N=4\mathcal N=4 SYM is

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

The isometry group of the five-sphere is

Isom(S5)=SO(6).\operatorname{Isom}(S^5)=SO(6).

Thus

SO(2,4)×SO(6)RSO(2,4)\times SO(6)_R

on the boundary matches

Isom(AdS5)×Isom(S5)\operatorname{Isom}(\mathrm{AdS}_5)\times \operatorname{Isom}(S^5)

in the bulk.

Including supersymmetry, the full superconformal symmetry is

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

which also appears as the symmetry supergroup of the maximally supersymmetric AdS5×S5\mathrm{AdS}_5\times S^5 background.

This matching does not prove the duality, but it is too rigid to be accidental. It tells us that if a four-dimensional CFT is going to be dual to type IIB string theory on AdS5×S5\mathrm{AdS}_5\times S^5, N=4\mathcal N=4 SYM has exactly the right symmetry structure.

Gauge group: U(N)U(N) or SU(N)SU(N)?

Section titled “Gauge group: U(N)U(N)U(N) or SU(N)SU(N)SU(N)?”

D3-branes naturally produce a U(N)U(N) gauge theory. At low energies,

U(N)SU(N)×U(1)ZN.U(N)\simeq \frac{SU(N)\times U(1)}{\mathbb Z_N}.

The overall U(1)U(1) describes the free center-of-mass motion of the stack of branes. It decouples from the interacting SU(N)SU(N) sector.

For the interacting AdS/CFT duality, one usually writes

N=4  SU(N)  SYM.\mathcal N=4\; SU(N)\; \text{SYM}.

At large NN, the distinction between U(N)U(N) and SU(N)SU(N) is often subleading for single-trace observables, but conceptually the distinction is useful. The SU(N)SU(N) theory is the interacting CFT of interest; the decoupled U(1)U(1) is not responsible for the curved AdS5×S5\mathrm{AdS}_5\times S^5 bulk.

The elementary fields AμA_\mu, ΦI\Phi^I, and λA\lambda^A are not gauge-invariant local observables. Physical local operators must be gauge invariant.

The simplest local examples are traces:

Tr(ΦI1ΦI2ΦIJ)(x),\operatorname{Tr}(\Phi^{I_1}\Phi^{I_2}\cdots \Phi^{I_J})(x),

or operators containing fermions, field strengths, and covariant derivatives:

Tr ⁣(FμνDρΦIλA)(x).\operatorname{Tr}\!\big(F_{\mu\nu}D_\rho\Phi^I\lambda^A\cdots\big)(x).

In a conformal theory, one should choose linear combinations that diagonalize the dilatation operator. The cleanest AdS/CFT statement is therefore:

single-trace conformal primary operatorsingle-particle bulk state.\text{single-trace conformal primary operator} \quad\longleftrightarrow\quad \text{single-particle bulk state}.

Some basic examples are:

Boundary objectBulk object
stress tensor TμνT_{\mu\nu}graviton in AdS5\mathrm{AdS}_5
R-current JRμJ^\mu_{R}gauge field from S5S^5 isometries
TrF2\operatorname{Tr}F^2dilaton-like mode
TrFF~\operatorname{Tr}F\widetilde Faxion-like mode
half-BPS scalar bilinearsKaluza–Klein supergravity modes on S5S^5
Wilson loopfundamental string worldsheet ending on the boundary

A particularly important family of protected scalar operators is the symmetric traceless combination

OIJ(x)=Tr(ΦIΦJ16δIJΦKΦK)(x),\mathcal O^{IJ}(x) = \operatorname{Tr}\left( \Phi^I\Phi^J-\frac{1}{6}\delta^{IJ}\Phi^K\Phi^K \right)(x),

which has protected dimension

Δ=2.\Delta=2.

These operators live in the 20\mathbf{20'} representation of SO(6)RSO(6)_R and belong to the stress-tensor multiplet. They are among the first nontrivial single-trace operators one meets in the canonical dictionary.

Supersymmetry does not make the theory trivial. It makes some quantities protected.

A protected operator has a scaling dimension or correlation-function coefficient constrained by supersymmetry. For example, many BPS operators have dimensions that do not depend on λ\lambda.

An unprotected operator can acquire a nontrivial anomalous dimension. A famous example is the Konishi operator, schematically

OK=Tr(ΦIΦI).\mathcal O_K = \operatorname{Tr}(\Phi^I\Phi^I).

At weak coupling it is a simple scalar bilinear. At strong coupling its dimension grows, and it is associated not with a light supergravity field but with a massive stringy excitation.

This distinction is crucial. The low-energy supergravity limit does not keep every single-trace operator light. It keeps operators dual to light bulk fields. Generic stringy operators become heavy when λ1\lambda\gg 1.

This is the field-theory meaning of the separation between the supergravity spectrum and the full string spectrum.

Central charges and the number of degrees of freedom

Section titled “Central charges and the number of degrees of freedom”

In four-dimensional CFTs, the stress-tensor two-point function and the Weyl anomaly measure the number of degrees of freedom in a precise way. For N=4\mathcal N=4 SYM with gauge algebra su(N)\mathfrak{su}(N), the central charges are

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

in a standard normalization.

At large NN,

acN2.a\sim c\sim N^2.

This is not a decorative fact. It is the boundary version of the bulk relation

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

The larger NN is, the smaller the effective gravitational coupling is in AdS units. Large central charge on the boundary is the first sign that a semiclassical bulk description might exist.

But large central charge alone is not enough. A weakly curved local Einstein-gravity dual also requires a large gap to most higher-spin or stringy single-trace operators. In the canonical example, that large gap appears at strong ‘t Hooft coupling.

The scalar potential vanishes when the six scalar matrices commute:

[ΦI,ΦJ]=0.[\Phi^I,\Phi^J]=0.

Commuting matrices can be diagonalized simultaneously. Their eigenvalues may be interpreted as positions of D3-branes in the six transverse directions:

ΦIdiag(x1I,x2I,,xNI).\Phi^I \sim \operatorname{diag}(x_1^I,x_2^I,\ldots,x_N^I).

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

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

where SNS_N permutes identical branes. For SU(N)SU(N), the center-of-mass direction is removed:

a=1NxaI=0.\sum_{a=1}^N x_a^I=0.

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

x1I=x2I==xNI=0.x_1^I=x_2^I=\cdots=x_N^I=0.

Moving onto the Coulomb branch separates the branes and changes the bulk geometry. That is a different state or vacuum of the same theory, not the maximally symmetric AdS5×S5\mathrm{AdS}_5\times S^5 vacuum.

Why the theory is called “maximally supersymmetric”

Section titled “Why the theory is called “maximally supersymmetric””

In four-dimensional interacting field theory with particles of spin at most one, N=4\mathcal N=4 is the maximum amount of ordinary supersymmetry one can have without introducing gravity. More supersymmetry would force higher spins or gravity-like structures.

This maximal supersymmetry has several consequences:

  • the field content is completely fixed once the gauge group is chosen;
  • the interactions are fixed by the gauge coupling;
  • the beta function vanishes;
  • many operator dimensions and correlation functions are protected;
  • the theory has a powerful superconformal symmetry.

For holography, maximal supersymmetry is both a blessing and a warning. It gives a beautifully controlled example, but it also makes the theory very different from QCD or condensed-matter systems. Many applications of holography deliberately break or reduce these symmetries.

N=4\mathcal N=4 SYM is a gauge theory, but it is not a model of real-world strong interactions.

It is different from QCD in several obvious ways:

  • it is conformal, so the coupling does not run;
  • it has no confinement in its vacuum on R1,3\mathbb R^{1,3};
  • all elementary fields are adjoint-valued;
  • it has six scalars and four Weyl fermions required by supersymmetry;
  • it has exact supersymmetry;
  • it has no fundamental quarks unless extra flavor sectors are added.

So why study it?

Because it is a controlled nonperturbative laboratory. It teaches us how gauge theories can encode gravity, how black holes can be described by ordinary quantum states, how geometry can emerge from matrix degrees of freedom, and how strong-coupling observables can sometimes be computed by classical gravitational methods.

The correct attitude is not “N=4\mathcal N=4 SYM is QCD.” The correct attitude is “N=4\mathcal N=4 SYM is the hydrogen atom of holography”: highly symmetric, not realistic, but structurally illuminating.

The field-theory data of N=4\mathcal N=4 SYM map to bulk data as follows:

N=4\mathcal N=4 SYM dataType IIB on AdS5×S5\mathrm{AdS}_5\times S^5 data
color rank NNNN units of five-form flux through S5S^5
N2N^2 degrees of freedomL3/G5N2L^3/G_5\sim N^2
’t Hooft coupling λ=gYM2N\lambda=g_{\mathrm{YM}}^2Ncurvature radius in string units, L4/α2λL^4/\alpha'^2\sim\lambda
complex coupling τYM\tau_{\mathrm{YM}}type IIB axio-dilaton C0+ieϕC_0+ie^{-\phi}
conformal symmetry SO(2,4)SO(2,4)isometry of AdS5\mathrm{AdS}_5
R-symmetry SO(6)RSO(6)_Risometry of S5S^5
single-trace primariessingle-particle bulk/string states
multi-trace operatorsmultiparticle bulk states
stress tensor TμνT_{\mu\nu}graviton
R-current JRμJ^\mu_Rgauge field from the compact space

This table is the reason N=4\mathcal N=4 SYM is the central example in a foundations course. Almost every later holographic dictionary entry is a generalization of one of these rows.

N=4\mathcal N=4 means N=4N=4 colors.”

Section titled ““N=4\mathcal N=4N=4 means N=4N=4N=4 colors.””

No. N=4\mathcal N=4 counts supersymmetry. The color rank is the NN in SU(N)SU(N). The large-NN limit concerns the color rank, not the number of supersymmetries.

“The elementary fields are the observables.”

Section titled ““The elementary fields are the observables.””

Not as local gauge-invariant operators. The elementary fields are useful variables in the Lagrangian, but local physical operators must be gauge invariant, such as traces of products of fields.

No. N=4\mathcal N=4 SYM is conformal for every value of gYMg_{\mathrm{YM}}, but it is generally interacting. Scaling dimensions of unprotected operators depend nontrivially on λ\lambda.

“Supersymmetry means everything is protected.”

Section titled ““Supersymmetry means everything is protected.””

No. Supersymmetry protects special operators, especially BPS operators. Generic operators have anomalous dimensions.

“The gravity limit is weak field-theory coupling.”

Section titled ““The gravity limit is weak field-theory coupling.””

No. Classical weakly curved gravity corresponds to strong ‘t Hooft coupling:

λ1.\lambda\gg 1.

Weak field-theory perturbation theory corresponds to λ1\lambda\ll 1, where the bulk string theory is highly curved in string units.

“The S5S^5 is an extra arbitrary decoration.”

Section titled ““The S5S^5S5 is an extra arbitrary decoration.””

No. The S5S^5 is required by the R-symmetry and by the D3-brane construction. Its isometry group SO(6)SO(6) matches the SO(6)RSO(6)_R symmetry rotating the six scalars.

“The U(1)U(1) from D3-branes should be part of the interacting dual.”

Section titled ““The U(1)U(1)U(1) from D3-branes should be part of the interacting dual.””

The overall U(1)U(1) is free and describes center-of-mass motion of the brane stack. The interacting holographic CFT is usually the SU(N)SU(N) sector.

Exercise 1: Count the adjoint degrees of freedom

Section titled “Exercise 1: Count the adjoint degrees of freedom”

For gauge group SU(N)SU(N), the adjoint representation has dimension N21N^2-1. Explain why the number of elementary field components in N=4\mathcal N=4 SYM scales like N2N^2 at large NN.

Solution

Each elementary field is adjoint-valued:

X(x)=Xa(x)Ta,a=1,,N21.X(x)=X^a(x)T^a, \qquad a=1,\ldots,N^2-1.

Thus every species of field carries N21N^2-1 color components. Since the number of species is fixed as NN changes, the total number of elementary field components scales as

N21N2.N^2-1\sim N^2.

This is the field-theory origin of the holographic scaling

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

Exercise 2: Why is gYMg_{\mathrm{YM}} dimensionless in four dimensions?

Section titled “Exercise 2: Why is gYMg_{\mathrm{YM}}gYM​ dimensionless in four dimensions?”

Use the Yang–Mills kinetic term

1gYM2d4xTrFμνFμν\frac{1}{g_{\mathrm{YM}}^2}\int d^4x\, \operatorname{Tr}F_{\mu\nu}F^{\mu\nu}

to determine the engineering dimension of gYMg_{\mathrm{YM}} in d=4d=4.

Solution

In units with =c=1\hbar=c=1, the action is dimensionless and

[d4x]=4.[d^4x]=-4.

The gauge field has engineering dimension

[Aμ]=1,[A_\mu]=1,

so the field strength has dimension

[Fμν]=2.[F_{\mu\nu}]=2.

Therefore

[FμνFμν]=4.[F_{\mu\nu}F^{\mu\nu}]=4.

The integral

d4xFμνFμν\int d^4x\, F_{\mu\nu}F^{\mu\nu}

is dimensionless, so gYMg_{\mathrm{YM}} is also dimensionless in four dimensions.

This argument only shows classical scale invariance. In a generic four-dimensional gauge theory, quantum effects can still generate a beta function. The special fact about N=4\mathcal N=4 SYM is that the beta function vanishes exactly.

Exercise 3: Match SO(6)RSO(6)_R to the bulk sphere

Section titled “Exercise 3: Match SO(6)RSO(6)_RSO(6)R​ to the bulk sphere”

Why is the equality

SO(6)RIsom(S5)SO(6)_R \simeq \operatorname{Isom}(S^5)

natural from the D3-brane viewpoint?

Solution

A D3-brane fills four spacetime directions and has six transverse directions in ten-dimensional flat space. The six scalar fields ΦI\Phi^I, I=1,,6I=1,\ldots,6, describe fluctuations of the brane in these transverse directions.

Rotations of the transverse R6\mathbb R^6 form the group SO(6)SO(6). In the worldvolume theory, this becomes the R-symmetry group rotating the six scalars:

ΦIRIJΦJ,RSO(6).\Phi^I \to R^I{}_J \Phi^J, \qquad R\in SO(6).

In the near-horizon geometry, the angular directions of the transverse R6\mathbb R^6 become an S5S^5. The isometry group of S5S^5 is also SO(6)SO(6). Thus the same transverse rotation symmetry appears as SO(6)RSO(6)_R in the CFT and as Isom(S5)\operatorname{Isom}(S^5) in the bulk.

Exercise 4: Identify the classical gravity regime

Section titled “Exercise 4: Identify the classical gravity regime”

Suppose the canonical parameter map is written as

L4α2=λ,gsλN.\frac{L^4}{\alpha'^2}=\lambda, \qquad g_s\sim \frac{\lambda}{N}.

What conditions suppress stringy curvature corrections and string loop corrections?

Solution

Stringy curvature corrections are suppressed when the AdS radius is large compared with the string length:

L2α.L^2\gg \alpha'.

Using

L4α2=λ,\frac{L^4}{\alpha'^2}=\lambda,

this requires

λ1.\lambda\gg 1.

String loop corrections are suppressed when the string coupling is small. Since

gsλN,g_s\sim \frac{\lambda}{N},

one sufficient condition is

Nλ.N\gg \lambda.

In the usual holographic classical-gravity regime, one takes NN very large and λ\lambda large, while keeping quantum-loop and α\alpha' corrections small. A common shorthand is

N1,λ1,N\gg 1, \qquad \lambda\gg 1,

with the understanding that the precise suppression of string loops also depends on how λ/N\lambda/N behaves.

Exercise 5: Why are single traces natural?

Section titled “Exercise 5: Why are single traces natural?”

Let XX be an adjoint scalar of SU(N)SU(N), so under a gauge transformation

XUXU1.X\to UXU^{-1}.

Show that Tr(XJ)\operatorname{Tr}(X^J) is gauge invariant.

Solution

Under the gauge transformation,

XJ(UXU1)(UXU1)(UXU1)=UXJU1.X^J\to (UXU^{-1})(UXU^{-1})\cdots(UXU^{-1})=UX^JU^{-1}.

Taking the trace gives

Tr(XJ)Tr(UXJU1).\operatorname{Tr}(X^J)\to \operatorname{Tr}(UX^JU^{-1}).

Using cyclicity of the trace,

Tr(UXJU1)=Tr(XJU1U)=Tr(XJ).\operatorname{Tr}(UX^JU^{-1})=\operatorname{Tr}(X^JU^{-1}U)=\operatorname{Tr}(X^J).

Thus Tr(XJ)\operatorname{Tr}(X^J) is gauge invariant. This is the basic reason single-trace operators are natural local operators in adjoint matrix gauge theories.