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M5-Branes and Six-Dimensional CFTs

The M5-brane example is the most mysterious member of the original AdS/CFT triad:

D3-branesAdS5/CFT4,M2-branesAdS4/CFT3,M5-branesAdS7/CFT6.\begin{array}{ccl} \text{D3-branes} &\longrightarrow& \mathrm{AdS}_5/\mathrm{CFT}_4,\\ \text{M2-branes} &\longrightarrow& \mathrm{AdS}_4/\mathrm{CFT}_3,\\ \text{M5-branes} &\longrightarrow& \mathrm{AdS}_7/\mathrm{CFT}_6. \end{array}

The M5-brane duality is

M-theory on AdS7×S4the six-dimensional (2,0) SCFT of type AN1.\boxed{ \text{M-theory on }\mathrm{AdS}_7\times S^4 \quad\longleftrightarrow\quad \text{the six-dimensional }(2,0)\text{ SCFT of type }A_{N-1}. }

Here NN is the number of coincident M5-branes, or equivalently the number of four-form flux units through S4S^4. The interacting boundary theory is not a six-dimensional Yang-Mills theory. It has no known ordinary local Lagrangian, contains tensionless string-like excitations at the conformal point, and has degrees of freedom scaling as N3N^3, not N2N^2.

That last fact is the first reason this page belongs in an AdS/CFT course. The D3-brane example might tempt us to equate holography with matrix large-NN counting. M5-branes say: not so fast. The gravitational measure of degrees of freedom is not always N2N^2; for M5-branes it is

LAdS5G7N3.\frac{L_{\mathrm{AdS}}^5}{G_7}\sim N^3.

The second reason is even more important. The six-dimensional (2,0)(2,0) theory is one of the best examples of a quantum field theory whose existence is strongly supported by string/M-theory, supersymmetry, compactification, anomalies, and holography, but whose intrinsic formulation remains highly nontrivial. It is not merely another item in the AdS/CFT zoo; it is a reminder that AdS/CFT often teaches us what quantum field theory itself can be.

A black and gray map of the M5-brane AdS7/CFT6 correspondence. N coincident M5-branes flow in the near-horizon limit to M-theory on AdS7 times S4 with N units of F4 flux. The boundary theory is the six-dimensional (2,0) A_{N-1} SCFT with OSp(8*|4) symmetry and N cubed degrees of freedom. Compactification arrows point to five-dimensional maximally supersymmetric Yang-Mills, four-dimensional N=4 SYM, and class S theories.

The M5-brane correspondence. The near-horizon geometry of NN coincident M5-branes is AdS7×S4\mathrm{AdS}_7\times S^4, with NN units of F4F_4 flux through S4S^4. The dual CFT is the interacting part of the six-dimensional (2,0)(2,0) theory of type AN1A_{N-1}. Its compactifications generate many lower-dimensional theories, including five-dimensional maximally supersymmetric Yang-Mills, four-dimensional N=4\mathcal N=4 SYM, and class-S\mathcal S theories.

The slogan is:

The (2,0) theory is a parent of gauge theories, not merely a strange cousin.\boxed{ \text{The }(2,0)\text{ theory is a parent of gauge theories, not merely a strange cousin.} }

Four-dimensional N=4\mathcal N=4 SYM, its S-duality, five-dimensional maximally supersymmetric Yang-Mills, and broad families of four-dimensional N=2\mathcal N=2 theories are most naturally understood as compactifications of this six-dimensional object.

From M5-branes to AdS7×S4\mathrm{AdS}_7\times S^4

Section titled “From M5-branes to AdS7×S4\mathrm{AdS}_7\times S^4AdS7​×S4”

An M5-brane is a five-dimensional spatial brane in eleven-dimensional M-theory. Its worldvolume has signature 5+15+1, and its transverse space has dimension five. The single M5-brane worldvolume theory contains a free (2,0)(2,0) tensor multiplet:

one chiral two-form B,H=dB,H=6H,\text{one chiral two-form } B, \qquad H=dB, \qquad H=*_{6}H,

plus five scalar fields and fermions fixed by supersymmetry. The five scalars describe transverse fluctuations of the brane and transform as a vector of SO(5)RSO(5)_R, the rotation group of the transverse space.

For NN coincident M5-branes, there is an interacting six-dimensional superconformal theory. The center-of-mass motion gives a decoupled free tensor multiplet; the interacting sector is usually called the AN1A_{N-1} (2,0)(2,0) theory. More generally, (2,0)(2,0) SCFTs are labeled by simply laced Lie algebras of ADE type:

g=AN1,DN,E6,E7,E8.\mathfrak g=A_{N-1},D_N,E_6,E_7,E_8.

The AN1A_{N-1} case is the one directly obtained from NN coincident M5-branes in flat space and is the case dual to the simplest AdS7×S4\mathrm{AdS}_7\times S^4 background.

The eleven-dimensional supergravity solution sourced by NN coincident extremal M5-branes takes the form

ds112=H(r)1/3ηαβdxαdxβ+H(r)2/3(dr2+r2dΩ42),α=0,1,,5,ds_{11}^2 = H(r)^{-1/3}\eta_{\alpha\beta}dx^\alpha dx^\beta + H(r)^{2/3}\left(dr^2+r^2d\Omega_4^2\right), \qquad \alpha=0,1,\ldots,5,

with

H(r)=1+R3r3,R3=πNp3.H(r)=1+\frac{R^3}{r^3}, \qquad R^3=\pi N\ell_p^3.

The solution also carries magnetic four-form flux through the transverse S4S^4,

1(2πp)3S4F4=N,\frac{1}{(2\pi\ell_p)^3}\int_{S^4}F_4=N,

up to the standard convention-dependent normalization of F4F_4.

In the near-horizon region rRr\ll R,

H(r)R3r3,H(r)\simeq \frac{R^3}{r^3},

so the metric becomes

ds112=rRηαβdxαdxβ+R2r2dr2+R2dΩ42.ds_{11}^2 = \frac{r}{R}\eta_{\alpha\beta}dx^\alpha dx^\beta + \frac{R^2}{r^2}dr^2 + R^2d\Omega_4^2.

Introduce a Poincare coordinate zz by

r=4R3z2.r=\frac{4R^3}{z^2}.

Then

rRdx1,52+R2r2dr2=4R2z2(dz2+dx1,52).\frac{r}{R}dx_{1,5}^2+\frac{R^2}{r^2}dr^2 = \frac{4R^2}{z^2}\left(dz^2+dx_{1,5}^2\right).

Thus the near-horizon geometry is

AdS7×S4,LAdS=2R,LS4=R.\boxed{ \mathrm{AdS}_7\times S^4, \qquad L_{\mathrm{AdS}}=2R, \qquad L_{S^4}=R. }

Equivalently, if LLAdSL\equiv L_{\mathrm{AdS}}, then

L3=8πNp3,LS4=L2.\boxed{ L^3=8\pi N\ell_p^3, \qquad L_{S^4}=\frac{L}{2}. }

This is the M5-brane analog of the D3-brane derivation of AdS5×S5\mathrm{AdS}_5\times S^5. The structure is the same, but the parameter dependence is different. In type IIB on AdS5×S5\mathrm{AdS}_5\times S^5, the curvature radius is controlled by λ1/4\lambda^{1/4} in string units. In M-theory on AdS7×S4\mathrm{AdS}_7\times S^4, there is no string coupling and no string length. There is only the eleven-dimensional Planck length p\ell_p, and

LpN1/3.\frac{L}{\ell_p}\sim N^{1/3}.

The classical supergravity limit is therefore

N1.N\gg 1.

There is no independent ‘t Hooft coupling to tune.

Why the boundary theory is six-dimensional

Section titled “Why the boundary theory is six-dimensional”

The conformal boundary of AdS7\mathrm{AdS}_7 is six-dimensional. In Poincare coordinates,

dsAdS72=L2z2(dz2+ηαβdxαdxβ),α=0,1,,5,ds_{\mathrm{AdS}_7}^2 = \frac{L^2}{z^2}\left(dz^2+\eta_{\alpha\beta}dx^\alpha dx^\beta\right), \qquad \alpha=0,1,\ldots,5,

and the boundary lies at z=0z=0. The boundary theory therefore lives on R1,5\mathbb R^{1,5}, or after conformal compactification on

R×S5.\mathbb R\times S^5.

The isometry group of AdS7\mathrm{AdS}_7 is

SO(2,6),SO(2,6),

which is precisely the conformal group in six spacetime dimensions. The isometry group of the internal sphere is

SO(5),SO(5),

which becomes the RR-symmetry group of the (2,0)(2,0) SCFT. The full superconformal symmetry is

OSp(84),bosonic subgroup SO(2,6)×SO(5)R.\boxed{ OSp(8^*|4), \qquad \text{bosonic subgroup }SO(2,6)\times SO(5)_R. }

This symmetry match is one of the cleanest pieces of the dictionary:

Bulk objectBoundary object
AdS7\mathrm{AdS}_7 isometries SO(2,6)SO(2,6)six-dimensional conformal symmetry
S4S^4 isometries SO(5)SO(5)SO(5)RSO(5)_R symmetry
NN units of F4F_4 fluxrank/type AN1A_{N-1} data
11d gravitons on AdS7×S4\mathrm{AdS}_7\times S^4stress-tensor multiplet and protected operators
M2-branes ending on the boundarysurface operators / self-dual strings
M5-branes wrapping cycles in S4S^4 or AdSextended defects and wrapped-brane observables

Notice the difference from D3-branes. In four-dimensional N=4\mathcal N=4 SYM, the gauge field is one of the elementary degrees of freedom. In the six-dimensional (2,0)(2,0) theory, the elementary free tensor multiplet contains a two-form potential BB, not a one-form gauge field AA. For the interacting nonabelian theory, even the phrase “elementary field” is dangerous. Many observables are more naturally associated with strings and surfaces than with particles and Wilson lines.

The (2,0)(2,0) tensor multiplet and the interacting theory

Section titled “The (2,0)(2,0)(2,0) tensor multiplet and the interacting theory”

For a single M5-brane, the free (2,0)(2,0) tensor multiplet contains:

FieldInterpretationSO(5)RSO(5)_R representation
BαβB_{\alpha\beta} with H=dB=HH=dB=*Hchiral two-form gauge potentialsinglet
ϕI\phi^I, I=1,,5I=1,\ldots,5transverse fluctuationsvector 5\mathbf 5
fermionssupersymmetric partnersspinor of SO(5)RSO(5)_R

The self-duality condition is crucial:

Hαβγ=13!ϵαβγδϵζHδϵζ.H_{\alpha\beta\gamma} = \frac{1}{3!}\epsilon_{\alpha\beta\gamma\delta\epsilon\zeta} H^{\delta\epsilon\zeta}.

It halves the degrees of freedom of the two-form, much as chirality halves the degrees of freedom of a Weyl fermion. It also makes covariant Lagrangian formulations subtle even for the free theory.

For multiple M5-branes, the interacting theory is not obtained by simply replacing U(1)U(1) by U(N)U(N) in a two-form gauge theory. There is no known ordinary nonabelian two-form gauge theory that captures the full interacting (2,0)(2,0) theory in a manifestly local six-dimensional Lagrangian. The theory is instead characterized by a network of mutually consistent facts:

  • it exists as the low-energy theory of coincident M5-branes;
  • it has OSp(84)OSp(8^*|4) superconformal symmetry;
  • it has ADE classification;
  • compactification on S1S^1 gives five-dimensional maximally supersymmetric Yang-Mills;
  • compactification on T2T^2 gives four-dimensional N=4\mathcal N=4 SYM with S-duality;
  • compactification on Riemann surfaces gives class-S\mathcal S theories;
  • holography predicts large-NN observables from M-theory on AdS7×S4\mathrm{AdS}_7\times S^4.

That is why the (2,0)(2,0) theory is often treated as a definition by its consequences. This sounds unsatisfying at first, but it is powerful. The theory is overconstrained from many sides.

The most famous quantitative statement about NN M5-branes is

number of degrees of freedomN3.\boxed{ \text{number of degrees of freedom} \sim N^3. }

Holographically, the reason is short. Reduce eleven-dimensional supergravity on S4S^4. If LL is the AdS7_7 radius, then the S4S^4 radius is L/2L/2, so

1G7=Vol(SL/24)G11=1G118π23(L2)4.\frac{1}{G_7} = \frac{\mathrm{Vol}(S^4_{L/2})}{G_{11}} = \frac{1}{G_{11}}\frac{8\pi^2}{3}\left(\frac{L}{2}\right)^4.

Using

G11=16π7p9,L3=8πNp3,G_{11}=16\pi^7\ell_p^9, \qquad L^3=8\pi N\ell_p^3,

one obtains

L5G7=163π2N3.\boxed{ \frac{L^5}{G_7}=\frac{16}{3\pi^2}N^3. }

This is the six-dimensional analog of the familiar AdS5_5/CFT4_4 result

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

But the physical meaning is more surprising. In ordinary adjoint matrix theories, N2N^2 suggests fields with two color indices. The (2,0)(2,0) theory has no conventional adjoint Lagrangian, and the N3N^3 scaling is not explained by a simple matrix count. It is instead a robust gravitational fact.

A clean thermodynamic manifestation comes from the planar AdS7_7 black brane:

ds72=L2z2[f(z)dt2+dx52+dz2f(z)],f(z)=1(zzh)6.ds_7^2 = \frac{L^2}{z^2}\left[-f(z)dt^2+d\vec x_5^{\,2}+\frac{dz^2}{f(z)}\right], \qquad f(z)=1-\left(\frac{z}{z_h}\right)^6.

The temperature is

T=64πzh=32πzh,T=\frac{6}{4\pi z_h}=\frac{3}{2\pi z_h},

and the entropy density is

s=14G7(Lzh)5=L54G7(2πT3)5.s = \frac{1}{4G_7}\left(\frac{L}{z_h}\right)^5 = \frac{L^5}{4G_7}\left(\frac{2\pi T}{3}\right)^5.

Using the formula above,

s=128π3729N3T5.\boxed{ s= \frac{128\pi^3}{729}N^3T^5. }

The T5T^5 follows from six-dimensional conformal invariance. The N3N^3 is the nontrivial information.

The same scaling appears in the holographic Weyl anomaly of the six-dimensional theory. In even-dimensional CFTs, the trace of the stress tensor on a curved background has local curvature-anomaly terms. For the M5-brane theory, holographic renormalization gives anomaly coefficients that grow as N3N^3 at large NN.

There are several useful ways to remember this:

M2-branes:FS3N3/2,D3-branes:a,c,s/T3N2,M5-branes:a6d,CT,s/T5N3.\boxed{ \begin{array}{ccl} \text{M2-branes} &:& F_{S^3}\sim N^{3/2},\\ \text{D3-branes} &:& a,c,s/T^3\sim N^2,\\ \text{M5-branes} &:& a_{6d},C_T,s/T^5\sim N^3. \end{array} }

The powers are not arbitrary. They come from flux quantization and dimensional reduction of the gravitational action.

For the M5-brane duality, the parameter controlling the classical bulk approximation is

pLN1/3.\frac{\ell_p}{L}\sim N^{-1/3}.

Thus large NN suppresses eleven-dimensional quantum-gravity corrections and higher-derivative corrections. Schematically,

S11d=1p9d11xgR+1p3C3F4F4+higher-derivative terms.S_{\mathrm{11d}} = \frac{1}{\ell_p^9}\int d^{11}x\sqrt g\,R + \frac{1}{\ell_p^3}\int C_3\wedge F_4\wedge F_4 + \text{higher-derivative terms}.

The familiar eleven-dimensional R4R^4-type higher-derivative terms are suppressed by powers of

(pL)61N2.\left(\frac{\ell_p}{L}\right)^6 \sim \frac{1}{N^2}.

Bulk loops are also suppressed at large NN. In the boundary theory this corresponds to a large-NN expansion, but it is not the usual planar expansion of a four-dimensional matrix gauge theory.

A useful comparison is:

DualityCurvature controlLoop controlClassical bulk limit
D3 / N=4\mathcal N=4 SYML4/α2λL^4/\alpha'^2\sim\lambdagsλ/Ng_s\sim\lambda/NN1N\gg 1, λ1\lambda\gg 1
M2 / ABJM at fixed kkL/pN1/6L/\ell_p\sim N^{1/6}same 11d expansionN1N\gg 1
M5 / (2,0)(2,0)L/pN1/3L/\ell_p\sim N^{1/3}same 11d expansionN1N\gg 1

For M5-branes there is no parameter analogous to the four-dimensional ‘t Hooft coupling. The strongly coupled nature of the boundary theory is built in.

Local operators of the six-dimensional SCFT are organized by OSp(84)OSp(8^*|4) representations. The best-protected sector consists of half-BPS operators. In the AN1A_{N-1} theory, single-particle supergravity modes on S4S^4 map to protected single-trace-like operators with SO(5)RSO(5)_R quantum numbers.

A schematic tower is

OkKK harmonic of degree k on S4,Δ=2k,k=2,3,.\mathcal O_k \quad\longleftrightarrow\quad \text{KK harmonic of degree }k\text{ on }S^4, \qquad \Delta=2k, \qquad k=2,3,\ldots.

The k=2k=2 multiplet contains the stress tensor, the SO(5)RSO(5)_R current, and other protected operators. In the free center-of-mass tensor multiplet one also has k=1k=1 fields, but the interacting AN1A_{N-1} sector begins differently. As always in holography, one should separate the decoupled center-of-mass sector from the interacting large-NN theory.

The most important universal dictionary entries are:

CFT6_6 operator/dataBulk dual
stress tensor TαβT_{\alpha\beta}AdS7_7 graviton
SO(5)RSO(5)_R currentgauge fields from S4S^4 isometries
scalar half-BPS operatorsKaluza-Klein scalar modes on S4S^4
surface operatorsM2-branes ending on boundary surfaces
codimension defectsprobe M2/M5 branes with AdS submanifolds
thermal stateAdS7_7 black brane
CTC_T, anomaly coefficientsL5/G7N3L^5/G_7\sim N^3

This dictionary is less elementary-looking than the D3-brane one because the boundary theory lacks a simple Lagrangian. Nevertheless, the protected spectrum, anomalies, correlator normalizations, and thermodynamics are sharply constrained.

A six-dimensional two-form gauge potential naturally couples to a two-dimensional surface, not to a one-dimensional line. For an abelian tensor multiplet, the analog of a Wilson loop is a Wilson surface:

W(Σ)exp(iΣB),W(\Sigma) \sim \exp\left(i\int_{\Sigma}B\right),

where Σ\Sigma is a two-dimensional surface in spacetime. In the interacting theory this formula is only a mnemonic, but the geometry is real: M2-branes can end on M5-branes. The boundary of the M2-brane is a string living on the M5-brane worldvolume. These are the self-dual strings of the (2,0)(2,0) theory.

In the holographic description, a surface operator in the boundary CFT is represented semiclassically by an M2-brane whose worldvolume ends on the prescribed boundary surface:

W(Σ)exp(TM2Volren(M3)),M3=Σ.\langle W(\Sigma)\rangle \sim \exp\left(-T_{\mathrm{M2}}\,\mathrm{Vol}_{\mathrm{ren}}(M_3)\right), \qquad \partial M_3=\Sigma.

Here

TM2=1(2π)2p3.T_{\mathrm{M2}}=\frac{1}{(2\pi)^2\ell_p^3}.

Since

TM2L3N,T_{\mathrm{M2}}L^3\sim N,

surface-operator exponents often scale like NN at leading semiclassical order. Wrapped M5-branes give other extended observables whose scaling can be larger. The detailed classification of defects in the (2,0)(2,0) theory is a rich subject, but the basic lesson is simple:

In six dimensions, the natural nonlocal probes are surfaces and defects, not only Wilson lines.\boxed{ \text{In six dimensions, the natural nonlocal probes are surfaces and defects, not only Wilson lines.} }

This is one reason the (2,0)(2,0) theory looks exotic from a four-dimensional gauge-theory viewpoint.

The (2,0)(2,0) theory becomes more familiar after compactification. In fact, many of our best definitions of its properties come from asking what it becomes on lower-dimensional spaces.

Compactification on S1S^1: five-dimensional maximally supersymmetric Yang-Mills

Section titled “Compactification on S1S^1S1: five-dimensional maximally supersymmetric Yang-Mills”

Compactify one spatial direction on a circle of radius R6R_6:

(2,0) theory on SR615d maximally supersymmetric Yang-Mills at low energy.\text{$(2,0)$ theory on }S^1_{R_6} \quad\leadsto\quad \text{5d maximally supersymmetric Yang-Mills at low energy.}

The five-dimensional gauge coupling has dimension of length:

[g52]=length.[g_5^2]=\text{length}.

The relation is convention-dependent, but schematically

g52R6.\boxed{ g_5^2\sim R_6. }

In a common normalization,

g52=8π2R6.g_5^2=8\pi^2R_6.

Five-dimensional Yang-Mills is perturbatively nonrenormalizable, so it cannot be a complete UV theory by itself. The (2,0)(2,0) theory is its proposed UV completion. A key check is the instanton particle. In five dimensions, an instanton in the spatial R4\mathbb R^4 becomes a particle with mass

Minst=8π2g52.M_{\mathrm{inst}}=\frac{8\pi^2}{g_5^2}.

Using g52=8π2R6g_5^2=8\pi^2R_6, this is

Minst=1R6,M_{\mathrm{inst}}=\frac{1}{R_6},

which is exactly the Kaluza-Klein scale of momentum around the compact circle. Thus the tower of instanton particles knows about the sixth dimension.

Compactification on T2T^2: four-dimensional N=4\mathcal N=4 SYM and S-duality

Section titled “Compactification on T2T^2T2: four-dimensional N=4\mathcal N=4N=4 SYM and S-duality”

Compactify the (2,0)(2,0) theory on a two-torus:

(2,0) theory on T24d N=4 SYM.\text{$(2,0)$ theory on }T^2 \quad\leadsto\quad \text{4d }\mathcal N=4\text{ SYM}.

The complex structure of the torus becomes the complexified Yang-Mills coupling:

τT2τYM=θ2π+4πigYM2.\tau_{T^2} \quad\longleftrightarrow\quad \tau_{\mathrm{YM}} = \frac{\theta}{2\pi}+\frac{4\pi i}{g_{\mathrm{YM}}^2}.

The modular group of the torus,

SL(2,Z),SL(2,\mathbb Z),

acts on τT2\tau_{T^2}. From the four-dimensional viewpoint this is the S-duality group of N=4\mathcal N=4 SYM. This is one of the most elegant explanations of why electric-magnetic duality in four dimensions should be exact: it is geometry in six dimensions.

Compactification on a Riemann surface: class-S\mathcal S theories

Section titled “Compactification on a Riemann surface: class-S\mathcal SS theories”

Compactify the (2,0)(2,0) theory on a Riemann surface CC with a partial topological twist:

(2,0) theory of type g on C4d N=2 class-S theory.\text{$(2,0)$ theory of type }\mathfrak g\text{ on }C \quad\leadsto\quad \text{4d }\mathcal N=2\text{ class-}\mathcal S\text{ theory}.

The complex structure moduli of CC become exactly marginal couplings of the four-dimensional theory. Degeneration limits of CC correspond to weakly coupled gauge-theory frames. Punctures on CC correspond to codimension-two defects of the six-dimensional theory and produce flavor symmetries in four dimensions.

This is far beyond a historical curiosity. It means that many dualities between four-dimensional gauge theories are shadows of the same six-dimensional parent theory viewed through different pair-of-pants decompositions of CC.

What makes the (2,0)(2,0) theory hard?

Section titled “What makes the (2,0)(2,0)(2,0) theory hard?”

The theory is difficult for several intertwined reasons.

First, six-dimensional conformal field theories are highly constrained. A Yang-Mills coupling in six dimensions has negative mass dimension:

[gYM2]=mass2.[g_{\mathrm{YM}}^2]=\mathrm{mass}^{-2}.

So ordinary six-dimensional Yang-Mills is not a fundamental conformal theory. The (2,0)(2,0) theory is not obtained by tuning a six-dimensional gauge coupling to a fixed point in the usual perturbative way.

Second, the basic tensor multiplet contains a chiral two-form. Even abelian chiral pp-form theories have subtleties involving self-duality, partition functions, and anomalies. The interacting nonabelian version is much more subtle.

Third, the theory contains string-like excitations. On the Coulomb branch, separated M5-branes allow M2-branes to stretch between them. Their boundaries are strings in the M5 worldvolume, with tension proportional to the brane separation. At the conformal point, where the branes coincide, these strings become tensionless.

Fourth, many observables are naturally extended rather than local. Surface operators, defects, compactification data, and anomaly polynomials are often better handles than elementary fields.

These difficulties should not be mistaken for vagueness. The theory has sharp protected data, a precise holographic dual at large NN, and numerous compactification checks.

In even-dimensional CFTs, the stress-tensor trace on a curved background has an anomaly:

T αα=iciIiaE6+αJα.\langle T^\alpha_{\ \alpha}\rangle = \sum_i c_i I_i - a E_6 + \nabla_\alpha J^\alpha.

Here E6E_6 is the six-dimensional Euler density, the IiI_i are Weyl invariants, and the last term is scheme-dependent. In the (2,0)(2,0) theory, supersymmetry relates much of this anomaly data. Holographically, the anomaly is extracted by evaluating the renormalized on-shell action of seven-dimensional asymptotically AdS gravity.

The crucial large-NN scaling is

a6dCTN3.\boxed{ a_{6d}\sim C_T\sim N^3. }

More refined formulas include subleading terms and distinguish the interacting AN1A_{N-1} theory from the decoupled center-of-mass tensor multiplet. For the purposes of the present course, the main lesson is that anomaly coefficients are the six-dimensional analogs of central charges. They measure the normalization of stress-tensor correlators and therefore the effective inverse Newton constant of the AdS7_7 dual.

This is the same logic used throughout AdS/CFT:

CFT stress-tensor normalizationbulk gravitational coupling1.\boxed{ \text{CFT stress-tensor normalization} \quad\longleftrightarrow\quad \text{bulk gravitational coupling}^{-1}. }

For M5-branes, this normalization is order N3N^3.

The maximally supersymmetric AdS7×S4\mathrm{AdS}_7\times S^4 solution is the cleanest AdS7_7/CFT6_6 example, but it is not the only context in which six-dimensional SCFTs appear in holography. Less supersymmetric six-dimensional (1,0)(1,0) SCFTs can also have AdS7_7 duals in massive type IIA or M-theory constructions. Those theories involve richer flavor symmetries, brane intersections, orientifolds, and anomaly-matching tests.

However, the maximally supersymmetric (2,0)(2,0) theory remains the basic reference point because:

  • the geometry is simple and explicit;
  • the symmetry is maximal;
  • the N3N^3 scaling is clean;
  • compactifications connect directly to many lower-dimensional dualities;
  • the large-NN supergravity regime is controlled by one parameter, NN.

The broader AdS7_7/CFT6_6 landscape is important for research, but it is best understood after the M5-brane example is mastered.

Mistake 1: Calling the six-dimensional theory “Yang-Mills”

Section titled “Mistake 1: Calling the six-dimensional theory “Yang-Mills””

The (2,0)(2,0) theory is not six-dimensional Yang-Mills. Five-dimensional maximally supersymmetric Yang-Mills appears after compactification on S1S^1 and is a low-energy description below the Kaluza-Klein scale.

Mistake 2: Forgetting the free center-of-mass tensor multiplet

Section titled “Mistake 2: Forgetting the free center-of-mass tensor multiplet”

The worldvolume theory of NN M5-branes contains a free center-of-mass tensor multiplet plus the interacting AN1A_{N-1} theory. Holographic large-NN statements usually refer to the interacting sector, where the N3N^3 scaling dominates.

Mistake 3: Treating N3N^3 as ordinary matrix counting

Section titled “Mistake 3: Treating N3N^3N3 as ordinary matrix counting”

The N3N^3 scaling is not explained by adjoint fields with two color indices. It is a gravitational result from L5/G7N3L^5/G_7\sim N^3 and is one of the reasons M5-branes are conceptually deeper than ordinary large-NN gauge theories.

Mistake 4: Looking for a tunable ‘t Hooft coupling

Section titled “Mistake 4: Looking for a tunable ‘t Hooft coupling”

There is no analog of λ=gYM2N\lambda=g_{\mathrm{YM}}^2N in the uncompactified (2,0)(2,0) theory. The large-NN classical bulk limit is controlled by L/pN1/3L/\ell_p\sim N^{1/3}.

Mistake 5: Thinking compactification loses information

Section titled “Mistake 5: Thinking compactification loses information”

Compactification is not merely a way to approximate the theory. It is one of the most powerful ways to define and test the theory. The geometry of the compactification manifold becomes duality data of the lower-dimensional theory.

Start from the extremal M5-brane metric

ds112=H1/3dx1,52+H2/3(dr2+r2dΩ42),H=1+R3r3.ds_{11}^2 = H^{-1/3}dx_{1,5}^2 + H^{2/3}\left(dr^2+r^2d\Omega_4^2\right), \qquad H=1+\frac{R^3}{r^3}.

Show that the near-horizon geometry is AdS7×S4\mathrm{AdS}_7\times S^4 and determine the ratio of the two radii.

Solution

In the near-horizon region rRr\ll R,

HR3r3.H\simeq \frac{R^3}{r^3}.

Therefore

H1/3=rR,H2/3=R2r2.H^{-1/3}=\frac{r}{R}, \qquad H^{2/3}=\frac{R^2}{r^2}.

The metric becomes

ds112=rRdx1,52+R2r2dr2+R2dΩ42.ds_{11}^2 = \frac{r}{R}dx_{1,5}^2 + \frac{R^2}{r^2}dr^2 + R^2d\Omega_4^2.

Define

r=4R3z2.r=\frac{4R^3}{z^2}.

Then

rRdx1,52+R2r2dr2=4R2z2(dx1,52+dz2).\frac{r}{R}dx_{1,5}^2+\frac{R^2}{r^2}dr^2 = \frac{4R^2}{z^2}\left(dx_{1,5}^2+dz^2\right).

Thus

ds112=(2R)2dx1,52+dz2z2+R2dΩ42.ds_{11}^2 = (2R)^2\frac{dx_{1,5}^2+dz^2}{z^2} + R^2d\Omega_4^2.

So

LAdS7=2R,LS4=R.L_{\mathrm{AdS}_7}=2R, \qquad L_{S^4}=R.

Exercise 2: Why L5/G7N3L^5/G_7\sim N^3

Section titled “Exercise 2: Why L5/G7∼N3L^5/G_7\sim N^3L5/G7​∼N3”

Assume

L3=8πNp3,G11=16π7p9,Vol(SL/24)=8π23(L2)4.L^3=8\pi N\ell_p^3, \qquad G_{11}=16\pi^7\ell_p^9, \qquad \mathrm{Vol}(S^4_{L/2})=\frac{8\pi^2}{3}\left(\frac{L}{2}\right)^4.

Show that

L5G7N3.\frac{L^5}{G_7}\propto N^3.
Solution

Dimensional reduction gives

1G7=Vol(SL/24)G11.\frac{1}{G_7}=\frac{\mathrm{Vol}(S^4_{L/2})}{G_{11}}.

Thus

L5G7=L5Vol(SL/24)G11=L51G118π23(L2)4.\frac{L^5}{G_7} = L^5\frac{\mathrm{Vol}(S^4_{L/2})}{G_{11}} = L^5\frac{1}{G_{11}}\frac{8\pi^2}{3}\left(\frac{L}{2}\right)^4.

This is proportional to

L9p9.\frac{L^9}{\ell_p^9}.

Since

L3Np3,L^3\propto N\ell_p^3,

we have

L9N3p9.L^9\propto N^3\ell_p^9.

Therefore

L5G7N3.\frac{L^5}{G_7}\propto N^3.

Keeping the stated conventions gives

L5G7=163π2N3.\frac{L^5}{G_7}=\frac{16}{3\pi^2}N^3.

Exercise 3: Entropy density of the M5 plasma

Section titled “Exercise 3: Entropy density of the M5 plasma”

For the planar AdS7_7 black brane,

ds72=L2z2[f(z)dt2+dx52+dz2f(z)],f(z)=1(zzh)6,ds_7^2 = \frac{L^2}{z^2}\left[-f(z)dt^2+d\vec x_5^{\,2}+\frac{dz^2}{f(z)}\right], \qquad f(z)=1-\left(\frac{z}{z_h}\right)^6,

show that the entropy density scales as

sN3T5.s\sim N^3T^5.
Solution

The Hawking temperature of the AdSd+1_{d+1} black brane is

T=d4πzh.T=\frac{d}{4\pi z_h}.

Here d=6d=6, so

T=32πzh,1zh=2πT3.T=\frac{3}{2\pi z_h}, \qquad \frac{1}{z_h}=\frac{2\pi T}{3}.

The horizon area density is

(Lzh)5.\left(\frac{L}{z_h}\right)^5.

Therefore

s=14G7(Lzh)5=L54G7(2πT3)5.s = \frac{1}{4G_7}\left(\frac{L}{z_h}\right)^5 = \frac{L^5}{4G_7}\left(\frac{2\pi T}{3}\right)^5.

Since L5/G7N3L^5/G_7\sim N^3,

sN3T5.s\sim N^3T^5.

With the conventions of Exercise 2,

s=128π3729N3T5.s=\frac{128\pi^3}{729}N^3T^5.

Exercise 4: Instantons as Kaluza-Klein modes

Section titled “Exercise 4: Instantons as Kaluza-Klein modes”

Compactify the (2,0)(2,0) theory on a circle of radius R6R_6. Suppose the low-energy five-dimensional Yang-Mills coupling is normalized as

g52=8π2R6.g_5^2=8\pi^2R_6.

Show that the five-dimensional instanton-particle mass equals the Kaluza-Klein mass of one unit of momentum around the circle.

Solution

In five-dimensional maximally supersymmetric Yang-Mills, an instanton in the four spatial directions is a particle. Its mass is

Minst=8π2g52.M_{\mathrm{inst}}=\frac{8\pi^2}{g_5^2}.

Using

g52=8π2R6,g_5^2=8\pi^2R_6,

we find

Minst=1R6.M_{\mathrm{inst}}=\frac{1}{R_6}.

A Kaluza-Klein excitation with one unit of momentum around a circle of radius R6R_6 also has mass

MKK=1R6.M_{\mathrm{KK}}=\frac{1}{R_6}.

Thus instanton number in five dimensions is identified with momentum around the compact sixth dimension.

Exercise 5: Why S-duality becomes geometry

Section titled “Exercise 5: Why S-duality becomes geometry”

Explain why compactifying the (2,0)(2,0) theory on a two-torus gives a natural origin for the SL(2,Z)SL(2,\mathbb Z) duality of four-dimensional N=4\mathcal N=4 SYM.

Solution

The two-torus has a mapping class group

SL(2,Z),SL(2,\mathbb Z),

which acts on its complex structure τT2\tau_{T^2}. Compactification of the (2,0)(2,0) theory on T2T^2 gives four-dimensional N=4\mathcal N=4 SYM, and the torus complex structure maps to the complexified gauge coupling,

τT2τYM=θ2π+4πigYM2.\tau_{T^2} \longleftrightarrow \tau_{\mathrm{YM}} = \frac{\theta}{2\pi}+\frac{4\pi i}{g_{\mathrm{YM}}^2}.

Therefore the geometric modular transformations of T2T^2 act as duality transformations on τYM\tau_{\mathrm{YM}}. The electric-magnetic S-duality of four-dimensional N=4\mathcal N=4 SYM is reinterpreted as ordinary geometry of the compactification torus.