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M2-Branes, ABJM, and AdS4/CFT3

The D3-brane example taught us the cleanest form of AdS/CFT:

N=4 SYM4type IIB string theory on AdS5×S5.\mathcal N=4\ \mathrm{SYM}_4 \quad\longleftrightarrow\quad \text{type IIB string theory on } \mathrm{AdS}_5\times S^5.

M2-branes give the next great example, and it is different in almost every useful way. The boundary theory is three-dimensional rather than four-dimensional, the gravity dual is naturally eleven-dimensional M-theory rather than perturbative string theory, and the number of degrees of freedom scales as N3/2N^{3/2} rather than N2N^2.

The central duality is the ABJM correspondence:

U(N)k×U(N)k N=6 Chern-Simons-matter theoryM-theory on AdS4×S7/Zk.\boxed{ U(N)_k\times U(N)_{-k}\ \mathcal N=6\ \text{Chern-Simons-matter theory} \quad\longleftrightarrow\quad \text{M-theory on }\mathrm{AdS}_4\times S^7/\mathbb Z_k. }

Here kk is an integer Chern-Simons level. The same theory has a second large-NN limit, the planar ‘t Hooft limit,

N,k,λ=Nk fixed,N\to\infty, \qquad k\to\infty, \qquad \lambda=\frac{N}{k}\ \text{fixed},

in which the dual description becomes type IIA string theory on

AdS4×CP3.\boxed{ \mathrm{AdS}_4\times \mathbb{CP}^3. }

This page has three goals. First, it explains why M2-branes lead naturally to a three-dimensional Chern-Simons-matter CFT rather than an ordinary Yang-Mills theory. Second, it derives the geometric dictionary between NN, kk, the M-theory radius, the type IIA coupling, and the curvature scale. Third, it explains the famous N3/2N^{3/2} scaling, one of the sharpest lessons that AdS/CFT teaches beyond the matrix-large-NN intuition of D-branes.

A black and gray map of the ABJM AdS4/CFT3 correspondence. N M2-branes probing C4/Zk flow to ABJM theory with gauge group U(N)k times U(N){-k}. At large N and fixed k the dual is M-theory on AdS4 times S7/Zk. In the planar limit with lambda equals N over k fixed and strong but not too strong, the dual is type IIA string theory on AdS4 times CP3. The figure also highlights F_S3 scaling as k^{1/2} N^{3/2} and the Hopf fibration S1/Zk to S7/Zk to CP3.

The ABJM correspondence has two useful gravity languages. At fixed kk and large NN, the natural bulk theory is eleven-dimensional M-theory on AdS4×S7/Zk\mathrm{AdS}_4\times S^7/\mathbb Z_k. In the planar limit with λ=N/k\lambda=N/k fixed, the Hopf fiber of S7/ZkS^7/\mathbb Z_k becomes the M-theory circle, and the dual becomes type IIA string theory on AdS4×CP3\mathrm{AdS}_4\times \mathbb{CP}^3.

The slogan is:

M2-branes are not just D3-branes in one fewer dimension.\boxed{ \text{M2-branes are not just D3-branes in one fewer dimension.} }

The difference is structural. D3-branes give a four-dimensional Yang-Mills theory with a marginal coupling. M2-branes give a three-dimensional SCFT whose natural weakly described Lagrangian uses Chern-Simons gauge fields, bifundamental matter, and discrete level kk.

Why M2-branes are different from D3-branes

Section titled “Why M2-branes are different from D3-branes”

A single M2-brane in flat eleven-dimensional spacetime has a 2+12+1-dimensional worldvolume and eight transverse scalar fields. For one brane this is simple: the low-energy theory is a free N=8\mathcal N=8 theory of eight scalars and eight fermions. For many coincident M2-branes, however, the interacting theory is much subtler than the D-brane gauge theories discussed earlier.

For Dpp-branes, open strings end on the branes. The massless open-string sector gives a p+1p+1 dimensional supersymmetric Yang-Mills theory, with coupling

[gYM2]=mass3p.[g_{\mathrm{YM}}^2]=\mathrm{mass}^{3-p}.

For D3-branes, gYM2g_{\mathrm{YM}}^2 is dimensionless. That is why the D3-brane system naturally leads to a conformal gauge theory. For D2-branes, by contrast,

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

Three-dimensional Yang-Mills theory is not conformal in the ultraviolet or infrared by simple dimensional analysis. It can nevertheless flow to a strongly coupled infrared fixed point. Physically, this infrared fixed point is the theory of M2-branes, because D2-branes lift to M2-branes when the M-theory circle decompactifies.

The question is then:

Can one write a useful Lagrangian for the interacting multiple-M2-brane fixed point itself?

The answer is yes, but not as an ordinary Yang-Mills theory. In three dimensions there is another natural gauge interaction: the Chern-Simons term

SCS[A]=k4πtr(AdA+2i3AAA).S_{\mathrm{CS}}[A] = \frac{k}{4\pi} \int \mathrm{tr}\left( A\wedge dA+\frac{2i}{3}A\wedge A\wedge A \right).

The coefficient kk is dimensionless and quantized. A pure Chern-Simons gauge field has no local propagating degrees of freedom, so coupling it to matter can produce a scale-invariant interacting theory without introducing a dimensionful Yang-Mills coupling. This is the basic reason ABJM theory is a Chern-Simons-matter theory.

Before introducing the boundary Lagrangian, let us recall the gravity side. The extremal M2-brane solution of eleven-dimensional supergravity has metric

ds112=H(r)2/3ηαβdxαdxβ+H(r)1/3(dr2+r2dΩ72),α=0,1,2,ds_{11}^2 = H(r)^{-2/3}\eta_{\alpha\beta}dx^\alpha dx^\beta + H(r)^{1/3}\left(dr^2+r^2d\Omega_7^2\right), \qquad \alpha=0,1,2,

with harmonic function

H(r)=1+R6r6.H(r)=1+\frac{R^6}{r^6}.

The four-form flux F4F_4 is electrically sourced by the M2-branes. Flux quantization fixes

R6=32π2Np6\boxed{ R^6=32\pi^2 N\ell_p^6 }

for NN M2-branes in flat transverse space R8\mathbb R^8, where p\ell_p is the eleven-dimensional Planck length.

In the near-horizon region rRr\ll R,

H(r)R6r6,H(r)\simeq \frac{R^6}{r^6},

and the metric becomes

ds112=r4R4ηαβdxαdxβ+R2r2dr2+R2dΩ72.ds_{11}^2 = \frac{r^4}{R^4}\eta_{\alpha\beta}dx^\alpha dx^\beta + \frac{R^2}{r^2}dr^2 + R^2d\Omega_7^2.

After a simple radial redefinition and a rescaling of the boundary coordinates, this is

AdS4×S7,LAdS4=R2,LS7=R.\boxed{ \mathrm{AdS}_4\times S^7, \qquad L_{\mathrm{AdS}_4}=\frac{R}{2}, \qquad L_{S^7}=R. }

The factor of 22 between the S7S^7 radius and the AdS4_4 radius is not a convention-free detail that can always be ignored. It matters in precise Kaluza-Klein spectra, flux quantization, and comparisons of protected operator dimensions.

The ABJM generalization replaces the transverse space by an orbifold

R8C4C4/Zk.\mathbb R^8\simeq \mathbb C^4 \quad\longrightarrow\quad \mathbb C^4/\mathbb Z_k.

The near-horizon geometry becomes

AdS4×S7/Zk.\boxed{ \mathrm{AdS}_4\times S^7/\mathbb Z_k. }

Because the internal volume is divided by kk, flux quantization gives

R6=32π2kNp6.\boxed{ R^6=32\pi^2 kN\ell_p^6. }

Thus NN is the flux through S7/ZkS^7/\mathbb Z_k, while kk controls the orbifold action and, after reduction, the size of the M-theory circle.

The seven-sphere can be viewed as a circle fibration over complex projective space:

S1S7CP3.S^1\longrightarrow S^7\longrightarrow \mathbb{CP}^3.

The Zk\mathbb Z_k quotient acts along the Hopf fiber, so the circle becomes shorter:

S1/ZkS7/ZkCP3.S^1/\mathbb Z_k\longrightarrow S^7/\mathbb Z_k\longrightarrow \mathbb{CP}^3.

The radius of the M-theory circle is schematically

R11Rk.R_{11}\sim \frac{R}{k}.

If this circle is large in eleven-dimensional Planck units, the proper description is M-theory. If this circle is small, one should reduce to type IIA string theory on the base CP3\mathbb{CP}^3.

Using

Rp(kN)1/6,\frac{R}{\ell_p}\sim (kN)^{1/6},

one finds

R11p(kN)1/6k=(Nk5)1/6.\frac{R_{11}}{\ell_p} \sim \frac{(kN)^{1/6}}{k} = \left(\frac{N}{k^5}\right)^{1/6}.

Therefore:

M-theory regime: Nk5,\boxed{ \text{M-theory regime: } N\gg k^5, }

while

type IIA regime: Nk5.\boxed{ \text{type IIA regime: } N\ll k^5. }

In the type IIA regime it is natural to define the ABJM ‘t Hooft coupling

λ=Nk.\boxed{ \lambda=\frac{N}{k}. }

The string-frame curvature radius and string coupling scale as

L2αλ,gsλ5/4N.\boxed{ \frac{L^2}{\alpha'}\sim \sqrt{\lambda}, \qquad g_s\sim \frac{\lambda^{5/4}}{N}. }

Thus classical type IIA supergravity requires

1λN4/5.\boxed{ 1\ll \lambda\ll N^{4/5}. }

The first inequality suppresses stringy α\alpha' corrections. The second suppresses string loops and keeps the M-theory circle small enough for the IIA reduction.

This is already a major conceptual difference from the D3-brane case. In AdS5_5/CFT4_4, large NN and large λ\lambda lead directly to weakly curved classical type IIB supergravity. In ABJM theory, there are two distinct strong-coupling gravity regimes:

LimitBoundary variablesBulk descriptionExpansion
M-theory limitNN\to\infty, kk fixedM-theory on AdS4×S7/Zk\mathrm{AdS}_4\times S^7/\mathbb Z_k1/N1/N quantum M-theory corrections
Planar string limitN,kN,k\to\infty, λ=N/k\lambda=N/k fixedtype IIA string theory on AdS4×CP3\mathrm{AdS}_4\times \mathbb{CP}^3genus expansion plus α\alpha' corrections
Classical IIA supergravityN1N\gg 1, 1λN4/51\ll\lambda\ll N^{4/5}two-derivative type IIA supergravitysmall gsg_s and small curvature
Weak planar ABJMN,kN,k\to\infty, λ1\lambda\ll 1perturbative Chern-Simons-matterweak planar field theory

ABJM theory is a three-dimensional superconformal Chern-Simons-matter theory with gauge group

U(N)k×U(N)k.\boxed{ U(N)_k\times U(N)_{-k}. }

The two subscripts denote opposite Chern-Simons levels. The opposite signs are essential: a single Chern-Simons term violates parity, but the ABJM theory has a parity symmetry that combines spatial reflection with exchange of the two gauge fields.

The field content can be summarized as follows:

FieldRepresentationRole
AμA_\muadjoint of first U(N)U(N)Chern-Simons gauge field at level kk
A^μ\widehat A_\muadjoint of second U(N)U(N)Chern-Simons gauge field at level k-k
YAY^A, A=1,,4A=1,\ldots,4(N,N)(\mathbf N,\overline{\mathbf N})four complex scalar fields
ψA\psi_A(N,N)(\mathbf N,\overline{\mathbf N})fermionic partners
conjugates(N,N)(\overline{\mathbf N},\mathbf N)complete bifundamental matter multiplets

The matter fields transform under

SU(4)RSO(6)SU(4)_R\simeq SO(6)

for generic kk, and the theory has explicit N=6\mathcal N=6 superconformal symmetry. For k=1,2k=1,2, the supersymmetry is enhanced to N=8\mathcal N=8, and the full R-symmetry becomes

SO(8)R,SO(8)_R,

as expected for M2-branes in flat space or on the mild C4/Z2\mathbb C^4/\mathbb Z_2 orbifold.

A schematic form of the action is

SABJM=SCS[A;k]+SCS[A^;k]+d3xtr(DμYADμYA+iψˉAγμDμψAVsextic+).S_{\mathrm{ABJM}} = S_{\mathrm{CS}}[A;k] + S_{\mathrm{CS}}[\widehat A;-k] + \int d^3x\,\mathrm{tr}\left( -D_\mu Y_A^\dagger D^\mu Y^A +i\bar\psi^A\gamma^\mu D_\mu\psi_A -V_{\mathrm{sextic}}+\cdots \right).

The ellipsis includes Yukawa couplings fixed by supersymmetry. The scalar potential is sextic, not quartic, as required in three dimensions: a scalar has engineering dimension 1/21/2, so a classically marginal scalar potential has degree six.

There is no continuous Yang-Mills coupling. The parameter kk is discrete. The continuous-looking coupling λ=N/k\lambda=N/k appears only in the large-NN planar expansion.

Moduli space and the meaning of C4/Zk\mathbb C^4/\mathbb Z_k

Section titled “Moduli space and the meaning of C4/Zk\mathbb C^4/\mathbb Z_kC4/Zk​”

A decisive check of ABJM theory is its moduli space. The moduli space should describe the positions of NN indistinguishable M2-branes moving in the transverse orbifold C4/Zk\mathbb C^4/\mathbb Z_k:

MN=SymN(C4/Zk).\boxed{ \mathcal M_N = \mathrm{Sym}^N\left(\mathbb C^4/\mathbb Z_k\right). }

Let us first consider N=1N=1. The gauge group is U(1)k×U(1)kU(1)_k\times U(1)_{-k}. The matter fields YAY^A are charged under the relative U(1)U(1) but neutral under the diagonal U(1)U(1). The Chern-Simons terms imply that after gauge identifications the scalar coordinates are subject to

YAe2πi/kYA,A=1,,4.Y^A\sim e^{2\pi i/k}Y^A, \qquad A=1,\ldots,4.

Thus the moduli space is

C4/Zk.\mathbb C^4/\mathbb Z_k.

For general NN, one can diagonalize the scalar matrices on the moduli space. The eigenvalues describe NN branes, and permutation of eigenvalues by the Weyl group gives the symmetric product.

This simple statement hides one of the characteristic subtleties of three-dimensional gauge theory: monopole operators. In three dimensions, local disorder operators can insert magnetic flux through a small two-sphere surrounding the insertion point. In Chern-Simons theory, magnetic flux carries electric charge because the Chern-Simons equation of motion schematically relates charge and flux:

k2πFJ.\frac{k}{2\pi}F \sim \star J.

Therefore monopole operators in ABJM theory are not optional exotic decorations. They are needed for the full operator spectrum, for the correct moduli-space interpretation, and for supersymmetry enhancement at k=1,2k=1,2.

A useful rule of thumb is:

In ABJM, some geometrically obvious bulk quantum numbers are carried by monopole operators.\boxed{ \text{In ABJM, some geometrically obvious bulk quantum numbers are carried by monopole operators.} }

For example, momentum along the M-theory circle is not visible as an ordinary polynomial in the elementary bifundamental fields. It is encoded by monopole sectors.

Symmetries and the AdS4_4/CFT3_3 dictionary

Section titled “Symmetries and the AdS4_44​/CFT3_33​ dictionary”

The bosonic symmetry of a three-dimensional CFT is

SO(2,3),SO(2,3),

which matches the isometry group of AdS4\mathrm{AdS}_4. The internal symmetry of the round S7S^7 is SO(8)SO(8), matching the SO(8)RSO(8)_R symmetry of the N=8\mathcal N=8 M2-brane theory. After orbifolding by Zk\mathbb Z_k, the manifest internal symmetry is reduced to

SU(4)×U(1),SU(4)\times U(1),

matching the generic ABJM global symmetry. In the type IIA description, this is the geometric symmetry of CP3\mathbb{CP}^3 together with the remnant associated to the M-theory circle.

The basic dictionary is:

CFT3_3 objectBulk object
Stress tensor TμνT_{\mu\nu}AdS4_4 graviton
SU(4)RSU(4)_R currentsgauge fields from isometries of CP3\mathbb{CP}^3 or S7/ZkS^7/\mathbb Z_k
Chiral primary operatorsKaluza-Klein modes on the internal space
Monopole operatorsstates carrying M-theory circle momentum or wrapped-brane charges
Wilson loopsfundamental strings in IIA, or M2-branes wrapping the M-circle in M-theory
S3S^3 partition function FFEuclidean AdS4_4 on-shell action
Thermal state on R2\mathbb R^2planar AdS4_4 black brane
Supersymmetric black-hole indexBPS AdS4_4 black-hole microstate counting

In a three-dimensional CFT there is no ordinary Weyl anomaly on a closed manifold, so one does not use four-dimensional central charges aa and cc. Two especially useful measures of degrees of freedom are:

CT,FS3=logZS3.C_T, \qquad F_{S^3}=-\log |Z_{S^3}|.

Here CTC_T normalizes the stress-tensor two-point function, and FS3F_{S^3} is the sphere free energy. In holographic CFT3_3 theories both scale like

LAdS2G4.\frac{L_{\mathrm{AdS}}^2}{G_4}.

For ABJM, this gives the famous scaling

FS3CTk1/2N3/2.\boxed{ F_{S^3}\sim C_T\sim k^{1/2}N^{3/2}. }

More precisely, at leading order for ABJM on the round three-sphere,

FS3=π2k3N3/2+O(N1/2)\boxed{ F_{S^3} = \frac{\pi\sqrt{2k}}{3}N^{3/2}+O(N^{1/2}) }

in the M-theory large-NN regime.

This result is not a minor numerical curiosity. It shows that the fundamental degrees of freedom of coincident M2-branes are not counted by adjoint matrices in the same way as D3-branes. The N3/2N^{3/2} law is one of the clearest signatures of M-theoretic holography.

Where the N3/2N^{3/2} scaling comes from

Section titled “Where the N3/2N^{3/2}N3/2 scaling comes from”

Let us derive the scaling from the bulk. The four-dimensional Newton constant is obtained by reducing eleven-dimensional supergravity on S7/ZkS^7/\mathbb Z_k:

1G4Vol(S7/Zk)G11R7kp9.\frac{1}{G_4} \sim \frac{\mathrm{Vol}(S^7/\mathbb Z_k)}{G_{11}} \sim \frac{R^7}{k\ell_p^9}.

The AdS4_4 radius is LRL\sim R, up to the fixed factor 1/21/2. Therefore the dimensionless gravitational strength is

L2G4R9kp9.\frac{L^2}{G_4} \sim \frac{R^9}{k\ell_p^9}.

Using flux quantization,

R6p6kN,\frac{R^6}{\ell_p^6}\sim kN,

we obtain

R9kp9(kN)3/2k=k1/2N3/2.\frac{R^9}{k\ell_p^9} \sim \frac{(kN)^{3/2}}{k} = k^{1/2}N^{3/2}.

Thus

L2G4k1/2N3/2.\boxed{ \frac{L^2}{G_4}\sim k^{1/2}N^{3/2}. }

For k=1k=1, this is simply N3/2N^{3/2}. Compare this with the D3-brane case:

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

The difference is not merely the boundary dimension. It is a difference between the large-NN physics of D-branes and M-branes.

ABJM theory is strongly coupled in the M-theory regime, but supersymmetry makes some exact computations possible. Supersymmetric localization reduces the S3S^3 partition function of ABJM theory to a finite-dimensional matrix model. At large NN, this matrix model reproduces the gravity prediction

FS3=π2k3N3/2+.F_{S^3}=\frac{\pi\sqrt{2k}}{3}N^{3/2}+\cdots.

Even more impressively, the matrix model can be reorganized as a Fermi gas. In that formulation, the large-NN expansion has an Airy-function structure, and certain quantum corrections become calculable with remarkable precision.

The conceptual lesson is important for the whole course:

AdS/CFT can sometimes compute quantum gravity corrections by exact CFT methods.\boxed{ \text{AdS/CFT can sometimes compute quantum gravity corrections by exact CFT methods.} }

In AdS5_5/CFT4_4, the canonical theory N=4\mathcal N=4 SYM has many exact tools, especially integrability and localization. ABJM theory has its own exact toolkit: supersymmetric localization, matrix models, Fermi-gas methods, superconformal indices, topologically twisted indices, and protected Wilson loops. These tools have made AdS4_4/CFT3_3 one of the best laboratories for studying quantum M-theory.

It is useful to compare the canonical examples side by side.

FeatureD3-branesM2-branes / ABJM
Boundary dimensiond=4d=4d=3d=3
Canonical CFTN=4\mathcal N=4 SYMABJM Chern-Simons-matter theory
Gauge structureSU(N)SU(N) or U(N)U(N) Yang-MillsU(N)k×U(N)kU(N)_k\times U(N)_{-k} Chern-Simons
Couplingλ=gYM2N\lambda=g_{\mathrm{YM}}^2Nλ=N/k\lambda=N/k in planar limit
Bulk at strong planar couplingtype IIB on AdS5×S5\mathrm{AdS}_5\times S^5type IIA on AdS4×CP3\mathrm{AdS}_4\times \mathbb{CP}^3
Bulk at fixed discrete parameterstill type IIBM-theory on AdS4×S7/Zk\mathrm{AdS}_4\times S^7/\mathbb Z_k
Degree scalingN2N^2k1/2N3/2k^{1/2}N^{3/2}
Internal symmetrySO(6)RSO(6)_RSU(4)R×U(1)SU(4)_R\times U(1), enhanced to SO(8)RSO(8)_R for k=1,2k=1,2
Exact toolsintegrability, localizationlocalization, Fermi gas, indices, integrability in planar IIA regime

Two morals are worth isolating.

First, AdS/CFT is not synonymous with gauge theory in four dimensions. It is a broader mechanism relating quantum gravity in asymptotically AdS spaces to nongravitational CFTs in one lower dimension.

Second, the classical-gravity limit is not always a string-theory limit. In ABJM at fixed kk, the correct large-NN bulk is eleven-dimensional M-theory. This is why ABJM is often the cleanest example for asking questions about genuinely M-theoretic quantum gravity.

The following diagnostic is useful in practice.

Start from NN and kk. Define

λ=Nk.\lambda=\frac{N}{k}.

Then ask:

  1. Is N1N\gg 1? If not, there is no classical bulk limit.
  2. Is kk fixed or at least Nk5N\gg k^5? Then the natural bulk is eleven-dimensional M-theory.
  3. Is Nk5N\ll k^5? Then the M-theory circle is small, so reduce to type IIA.
  4. In the type IIA regime, is λ1\lambda\gg 1? Then the string-frame curvature is small.
  5. Is λN4/5\lambda\ll N^{4/5}? Then the string coupling is small.

This gives:

Nk5M-theory on AdS4×S7/Zk,1λN4/5classical type IIA on AdS4×CP3,λ1weakly coupled planar ABJM perturbation theory.\boxed{ \begin{array}{ccl} N\gg k^5 &\Rightarrow& \text{M-theory on }\mathrm{AdS}_4\times S^7/\mathbb Z_k,\\ 1\ll \lambda\ll N^{4/5} &\Rightarrow& \text{classical type IIA on }\mathrm{AdS}_4\times\mathbb{CP}^3,\\ \lambda\ll 1 &\Rightarrow& \text{weakly coupled planar ABJM perturbation theory.} \end{array} }

Do not compress this to “large λ\lambda means gravity.” Large λ\lambda by itself does not tell you whether the correct weakly curved description is type IIA or eleven-dimensional M-theory.

Mistake 1: Treating ABJM as ordinary Yang-Mills. The ABJM gauge fields are Chern-Simons gauge fields. There is no Maxwell kinetic term in the conformal theory. Adding a Yang-Mills term is an irrelevant deformation that can be useful as a regulator or as a route from D2-branes, but it is not part of the fixed-point definition.

Mistake 2: Forgetting that kk is quantized. The Chern-Simons level is an integer. The parameter λ=N/k\lambda=N/k becomes continuously useful only in a large-NN limit.

Mistake 3: Assuming all large-NN holographic CFTs have N2N^2 degrees of freedom. Matrix gauge theories often have N2N^2 scaling, but M2-branes have N3/2N^{3/2} scaling. M5-branes, discussed next, have N3N^3 scaling.

Mistake 4: Confusing the M-theory and type IIA limits. The fixed-kk large-NN regime is not planar string theory. It is an eleven-dimensional regime.

Mistake 5: Ignoring monopole operators. Many important ABJM states and symmetries are invisible if one only writes polynomial traces of elementary fields. Monopole sectors are central to the theory.

Mistake 6: Dropping the radius factor LS7=2LAdSL_{S^7}=2L_{\mathrm{AdS}}. For qualitative discussions this often does no harm. For spectra and precision matching, it matters.

Exercise 1: Why Chern-Simons, not Yang-Mills?

Section titled “Exercise 1: Why Chern-Simons, not Yang-Mills?”

In three dimensions, determine the mass dimension of gYM2g_{\mathrm{YM}}^2 in a Yang-Mills action

SYM=14gYM2d3xtrFμνFμν.S_{\mathrm{YM}} = \frac{1}{4g_{\mathrm{YM}}^2} \int d^3x\, \mathrm{tr}\,F_{\mu\nu}F^{\mu\nu}.

Explain why this makes Yang-Mills theory unsuitable as the fundamental conformal interaction of M2-branes.

Solution

The action is dimensionless and d3xd^3x has mass dimension 3-3. In dd dimensions, [gYM2]=mass4d[g_{\mathrm{YM}}^2]=\mathrm{mass}^{4-d}. Therefore in d=3d=3,

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

The Yang-Mills coupling is dimensionful, so it introduces a scale. Three-dimensional Yang-Mills theory can flow to a nontrivial infrared fixed point, but the Yang-Mills term itself is not a marginal conformal interaction. A Chern-Simons term has dimensionless quantized level kk, so Chern-Simons-matter theory is the natural Lagrangian framework for a three-dimensional gauge-theoretic SCFT.

Exercise 2: The near-horizon M2-brane geometry

Section titled “Exercise 2: The near-horizon M2-brane geometry”

Starting from

ds112=H2/3ηαβdxαdxβ+H1/3(dr2+r2dΩ72),H=R6r6,ds_{11}^2 = H^{-2/3}\eta_{\alpha\beta}dx^\alpha dx^\beta + H^{1/3}\left(dr^2+r^2d\Omega_7^2\right), \qquad H=\frac{R^6}{r^6},

show that the near-horizon metric is AdS4×S7\mathrm{AdS}_4\times S^7 with LAdS4=R/2L_{\mathrm{AdS}_4}=R/2.

Solution

Substituting H=R6/r6H=R^6/r^6 gives

H2/3=r4R4,H1/3=R2r2.H^{-2/3}=\frac{r^4}{R^4}, \qquad H^{1/3}=\frac{R^2}{r^2}.

Thus

ds112=r4R4ηαβdxαdxβ+R2r2dr2+R2dΩ72.ds_{11}^2 = \frac{r^4}{R^4}\eta_{\alpha\beta}dx^\alpha dx^\beta +\frac{R^2}{r^2}dr^2 +R^2d\Omega_7^2.

Let

y=r2R2.y=\frac{r^2}{R^2}.

Then

R2r2dr2=R24dy2y2,\frac{R^2}{r^2}dr^2 = \frac{R^2}{4}\frac{dy^2}{y^2},

and the first term is y2ηαβdxαdxβy^2\eta_{\alpha\beta}dx^\alpha dx^\beta, up to a constant rescaling of the boundary coordinates. Therefore the four-dimensional part is Poincaré AdS4_4 with radius R/2R/2, while the internal sphere has radius RR.

Exercise 3: The N3/2N^{3/2} scaling from flux quantization

Section titled “Exercise 3: The N3/2N^{3/2}N3/2 scaling from flux quantization”

Use

R6kNp6,1G4R7kp9,LR,R^6\sim kN\ell_p^6, \qquad \frac{1}{G_4}\sim \frac{R^7}{k\ell_p^9}, \qquad L\sim R,

to show that

L2G4k1/2N3/2.\frac{L^2}{G_4}\sim k^{1/2}N^{3/2}.
Solution

The four-dimensional gravitational strength scales as

L2G4R2R7kp9=R9kp9.\frac{L^2}{G_4} \sim \frac{R^2R^7}{k\ell_p^9} = \frac{R^9}{k\ell_p^9}.

From flux quantization,

Rp(kN)1/6.\frac{R}{\ell_p}\sim (kN)^{1/6}.

Therefore

R9kp9(kN)9/6k=(kN)3/2k=k1/2N3/2.\frac{R^9}{k\ell_p^9} \sim \frac{(kN)^{9/6}}{k} = \frac{(kN)^{3/2}}{k} = k^{1/2}N^{3/2}.

Since holographic CFT3_3 observables such as FS3F_{S^3} and CTC_T scale as L2/G4L^2/G_4, they scale as k1/2N3/2k^{1/2}N^{3/2}.

For each pair (N,k)(N,k), determine whether the natural strong-coupling bulk description is M-theory or type IIA, assuming NN is large.

  1. N=108N=10^8, k=1k=1.
  2. N=108N=10^8, k=103k=10^3.
  3. N=108N=10^8, k=107k=10^7.
Solution

The key comparison is NN versus k5k^5.

  1. For k=1k=1, k5=1k^5=1, so Nk5N\gg k^5. This is the M-theory regime.
  2. For k=103k=10^3, k5=1015k^5=10^{15}, so Nk5N\ll k^5. The M-theory circle is small, so the natural description is type IIA. Since λ=N/k=105\lambda=N/k=10^5 and N4/5=106.4N^{4/5}=10^{6.4}, the inequalities 1λN4/51\ll\lambda\ll N^{4/5} are satisfied. This is a clean classical type IIA supergravity regime.
  3. For k=107k=10^7, k5=1035k^5=10^{35}, so the circle is very small, but λ=N/k=10\lambda=N/k=10. This may be in the type IIA string regime with small string coupling, but the curvature is only moderately small. It is not as clean a classical supergravity limit as case 2.

Explain why the moduli space of the U(1)k×U(1)kU(1)_k\times U(1)_{-k} ABJM theory is C4/Zk\mathbb C^4/\mathbb Z_k rather than simply C4\mathbb C^4.

Solution

The four complex scalars YAY^A are coordinates on C4\mathbb C^4 before gauge identifications. In the U(1)k×U(1)kU(1)_k\times U(1)_{-k} theory, the diagonal U(1)U(1) decouples from the matter, while the relative U(1)U(1) acts by a common phase rotation on the YAY^A. Because of the Chern-Simons level kk, the residual gauge identification is a discrete phase rotation

YAe2πi/kYA.Y^A\sim e^{2\pi i/k}Y^A.

Therefore the physical moduli space is

C4/Zk.\mathbb C^4/\mathbb Z_k.

For NN branes one then obtains the symmetric product SymN(C4/Zk)\mathrm{Sym}^N(\mathbb C^4/\mathbb Z_k).