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Large N and what a 't Hooft limit holds fixed

Increasing the size of a gauge group does not specify a limit of a physical observable. The coupling might decrease, remain fixed, or grow. A Chern–Simons level might stay at an integer or grow with the rank. Even the same matrix expression can acquire a different limit if its normalization changes.

We will specify these choices and then perform an exact finite-dimensional calculation that distinguishes a limiting answer from its corrections. Ordinary QFT, gauge theory, and Gaussian integration suffice; no supersymmetry or Lie-theory lesson is a prerequisite.

A limit is a sequence of theories and measurements

Section titled “A limit is a sequence of theories and measurements”

For SU(N)SU(N) or U(N)U(N), NN is the dimension of the fundamental color space. Their mathematical ranks are N−1N-1 and NN, respectively. “Large rank” conventionally means taking this color parameter to infinity. It does not change the number of spacetime dimensions or the amount of supersymmetry.

Write a measured quantity as ON(g,mR,…)\mathcal O_N(g,mR,\ldots), where RR is a specified length and mm a mass. A limit requires a sequence of allowed parameters, together with a prescription for comparing observables. Keeping mm fixed while changing RR does not keep mRmR fixed. Changing the representation of a Wilson loop or letting the number of fields in an operator grow with NN likewise changes the problem.

We use the ordinary fundamental trace and its explicitly normalized counterpart:

Tr⁡NIN=N,tr⁡NM=1NTr⁡NM.\operatorname{Tr}_N I_N=N,\qquad \operatorname{tr}_N M=\frac1N\operatorname{Tr}_N M.

Replacing one by the other requires a compensating factor of NN. The optional matrix-valued matter lesson explains their color-index meaning in more detail.

First calculation: keep the Yang–Mills coupling combination fixed

Section titled “First calculation: keep the Yang–Mills coupling combination fixed”

Consider four-dimensional SU(N)SU(N) N=4\mathcal N=4 supersymmetric Yang–Mills theory, with sixteen real Poincaré supercharges and vanishing theta angle. Its supersymmetric interactions are part of the theory’s definition; only the gauge kinetic term is needed for this scaling calculation. Use flat Euclidean space, Hermitian generators Tr⁡N(tatb)=δab/2\operatorname{Tr}_N(t^at^b)=\delta^{ab}/2, and a connection with the coupling absorbed:

Dμ=∂μ−iAμ,Fμν=∂μAν−∂νAμ−i[Aμ,Aν].D_\mu=\partial_\mu-iA_\mu,\qquad F_{\mu\nu}=\partial_\mu A_\nu-\partial_\nu A_\mu-i[A_\mu,A_\nu].

Both AμA_\mu and a derivative have mass dimension one. Define the dimensionless coupling gYMg_{\rm YM} by

Sgauge=12gYM2∫d4x Tr⁡N(FμνFμν).(T15.1)S_{\rm gauge} =\frac1{2g_{\rm YM}^2}\int d^4x\, \operatorname{Tr}_N(F_{\mu\nu}F_{\mu\nu}). \tag{T15.1}

For comparison with canonical components, set Aμ=gYMAμ,canA_\mu=g_{\rm YM}A_{\mu,\rm can}. Then Fμν=gYM(∂μAν,can−∂νAμ,can−igYM[Aμ,can,Aν,can])F_{\mu\nu}=g_{\rm YM}(\partial_\mu A_{\nu,\rm can}-\partial_\nu A_{\mu,\rm can}-ig_{\rm YM}[A_{\mu,\rm can},A_{\nu,\rm can}]). Using the generator norm, (T15.1) has canonical component coefficient 1/41/4. Its cubic and quartic gauge vertices carry gYMg_{\rm YM} and gYM2g_{\rm YM}^2.

The ‘t Hooft coupling in this theory is λYM=gYM2N\lambda_{\rm YM}=g_{\rm YM}^2N. Holding it fixed gives the exact rewriting

gYM2=λYMN,Sgauge=N2λYM∫d4x Tr⁡NF2=N22λYM∫d4x tr⁡NF2.(T15.2)g_{\rm YM}^2=\frac{\lambda_{\rm YM}}N,\qquad S_{\rm gauge} =\frac{N}{2\lambda_{\rm YM}}\int d^4x\,\operatorname{Tr}_N F^2 =\frac{N^2}{2\lambda_{\rm YM}}\int d^4x\,\operatorname{tr}_N F^2. \tag{T15.2}

The last two expressions are the same action. They do not imply two competing large-NN scalings.

Although gYM→0g_{\rm YM}\to0, an internal color sum can compensate a power of the coupling: gYM2N=λYMg_{\rm YM}^2N=\lambda_{\rm YM} remains finite. Minahan’s discussion after (5.12) identifies this combination in planar perturbation theory. “Planar” refers to the leading color-contraction organization; its detailed diagrammatic derivation is a further method. A fixed value such as λYM=100\lambda_{\rm YM}=100 is not a weak-coupling limit merely because NN is large.

Holding gYM2=g02>0g_{\rm YM}^2=g_0^2>0 instead gives λYM=Ng02→∞\lambda_{\rm YM}=Ng_0^2\to\infty. That is a different path through theories. For an observable expanded at fixed λYM\lambda_{\rm YM}, taking the coupling large is an additional approximation whose order and error must be specified.

The integer level changes the three-dimensional question

Section titled “The integer level changes the three-dimensional question”

Now consider equal-rank ABJM theory with compact gauge group U(N)k×U(N)−kU(N)_k\times U(N)_{-k}, positive integer kk, and no extra global quotient. This three-dimensional theory has bifundamental matter and Chern–Simons gauge terms, with no defining Maxwell kinetic term. Its generic full supersymmetry has twelve real Poincaré supercharges. At k=1,2k=1,2 the count increases to sixteen; the ABJM definition explains the enhancement and low-rank qualifications. These facts identify the family; no supersymmetry transformation is needed below.

With Hermitian connections a,a^a,\widehat a and the ordinary trace, its Euclidean connection action contains

SCS,E=ik4π∫d3x ϵμνρTr⁡N(aμ∂νaρ−2i3aμaνaρ−a^μ∂νa^ρ+2i3a^μa^νa^ρ).(T15.3)S_{{\rm CS},E} =\frac{ik}{4\pi}\int d^3x\,\epsilon^{\mu\nu\rho} \operatorname{Tr}_N \left(a_\mu\partial_\nu a_\rho-\frac{2i}{3}a_\mu a_\nu a_\rho -\widehat a_\mu\partial_\nu\widehat a_\rho +\frac{2i}{3}\widehat a_\mu\widehat a_\nu\widehat a_\rho\right). \tag{T15.3}

Here ϵ123=+1\epsilon^{123}=+1. The connection has dimension one, so the integrand has dimension three and kk is dimensionless. The compact theory requires the integer level and its global Chern–Simons definition; continuously varying kk at finite NN would leave this declared family. The opposite levels and fundamental-trace convention come from AB, sections 2.1–2.2.

Its useful coupling ratio is λAB=N/k\lambda_{\rm AB}=N/k, not gYM2Ng_{\rm YM}^2N. The two symbols called “‘t Hooft coupling” belong to different theories. AB’s large-NN paragraph describes perturbative weakness when k≫Nk\gg N, rather than when kk is merely a large integer.

Family of limitsHeld fixedWhat changes
Four-dimensional Yang–Mills ‘t Hooft limitλYM>0\lambda_{\rm YM}>0N→∞N\to\infty, gYM2=λYM/Ng_{\rm YM}^2=\lambda_{\rm YM}/N
ABJM ‘t Hooft limitλAB>0\lambda_{\rm AB}>0N,k→∞N,k\to\infty with N/k→λABN/k\to\lambda_{\rm AB}
ABJM fixed-level limitInteger k=k0>0k=k_0>0N→∞N\to\infty, λAB=N/k0→∞\lambda_{\rm AB}=N/k_0\to\infty

FG, (1.3)–(1.4) distinguishes the last two limits explicitly. For rational λAB=p/q>0\lambda_{\rm AB}=p/q>0, choose N=pnN=pn, k=qnk=qn with positive integers nn. For an irrational target, integer ratios can approach it; they cannot equal it at every finite rank.

There is also a direct action-coefficient check. Replacing the ordinary trace in (T15.3) by tr⁡N\operatorname{tr}_N changes its prefactor to ikN/(4π)ikN/(4\pi). This coefficient grows as NN at fixed kk, and as N2N^2 at fixed N/kN/k. The configurations and their fluctuations have not yet been integrated. Consequently this coefficient comparison alone does not determine the free-energy power: typical fields and the measure also depend on the limit.

The mass dimensions offer another safeguard. In four dimensions gYM2g_{\rm YM}^2 is dimensionless. A three-dimensional Yang–Mills coupling instead has [g32]=1[g_3^2]=1, so its dimensionless color-enhanced parameter at energy EE would be g32N/Eg_3^2N/E. Neither quantity can replace ABJM’s dimensionless integer level.

Worked finite-rank check: a normalized trace fluctuates less

Section titled “Worked finite-rank check: a normalized trace fluctuates less”

To see what a finite-rank correction means without assuming a field-theory solution, define a Gaussian model on all Hermitian NN-by-NN matrices:

ZN(s)=∫dV(M) e−N2sTr⁡NM2,ON=1NTr⁡NM2,s>0.(T15.4)Z_N(s)=\int dV(M)\, e^{-\frac{N}{2s}\operatorname{Tr}_N M^2}, \qquad O_N=\frac1N\operatorname{Tr}_N M^2,\qquad s>0. \tag{T15.4}

All entries and ss are dimensionless. The measure is induced by dsM2=Tr⁡N(dM dM)ds_M^2=\operatorname{Tr}_N(dM\,dM). This is a defined finite-dimensional model, not an asserted localization formula for either field theory.

Choose an orthonormal Hermitian matrix basis EAE_A with Tr⁡N(EAEB)=δAB\operatorname{Tr}_N(E_AE_B)=\delta_{AB}. There are d=N2d=N^2 real coefficients in M=∑AxAEAM=\sum_Ax_AE_A, and Tr⁡M2=∑AxA2\operatorname{Tr}M^2=\sum_Ax_A^2, dV=∏AdxAdV=\prod_A dx_A. Thus

ZN(s)=(2πsN)N2/2.Z_N(s)=\left(\frac{2\pi s}{N}\right)^{N^2/2}.

Every xAx_A has variance s/Ns/N. More usefully, integrate with a source for the whole observable:

GN(t)=⟨e−tON⟩=∏A=1N2∫RdxA e−[N/(2s)+t/N]xA2∫RdxA e−NxA2/(2s)=(1+2stN2)−N2/2,t>−N22s.(T15.5)\begin{aligned} G_N(t)&=\left\langle e^{-tO_N}\right\rangle\\ &=\prod_{A=1}^{N^2} \frac{\int_{\mathbb R}dx_A\, e^{-[N/(2s)+t/N]x_A^2}} {\int_{\mathbb R}dx_A\,e^{-Nx_A^2/(2s)}}\\ &=\left(1+\frac{2st}{N^2}\right)^{-N^2/2}, \qquad t>-\frac{N^2}{2s}. \end{aligned} \tag{T15.5}

For this sign of the source, −∂tlog⁡GN(0)-\partial_t\log G_N(0) is the mean and ∂t2log⁡GN(0)\partial_t^2\log G_N(0) the variance. Therefore

⟨ON⟩=s,Var⁡(ON)=2s2N2,⟨ON2⟩=s2(1+2N2).(T15.6)\boxed{ \langle O_N\rangle=s,\qquad \operatorname{Var}(O_N)=\frac{2s^2}{N^2},\qquad \langle O_N^2\rangle=s^2\left(1+\frac2{N^2}\right). } \tag{T15.6}

The variance is the connected part ⟨ON2⟩−⟨ON⟩2\langle O_N^2\rangle-\langle O_N\rangle^2. It vanishes at fixed ss, while the relative standard deviation is 2/N\sqrt2/N. For s=3/2s=3/2:

NNExact meanExact variance
223/23/29/89/8
443/23/29/329/32
883/23/29/1289/128

This example demonstrates factorization for this particular observable. It does not prove factorization for every operator in an interacting gauge theory. No eigenvalue Jacobian or diagrammatic topology was needed; the matrix-integral lesson explains the alternative eigenvalue coordinates.

At fixed s,ts,t, expanding the exact logarithm gives

log⁡GN(t)=−st+s2t2N2−4s3t33N4+O(N−6).(T15.7)\log G_N(t) =-st+\frac{s^2t^2}{N^2} -\frac{4s^3t^3}{3N^4}+O(N^{-6}). \tag{T15.7}

The exact formula and the truncated expansion are different statements. For t≥0t\geq0 and 2st/N2≤12st/N^2\leq1, the alternating logarithm series bounds the error after the N−2N^{-2} term by 4s3t3/(3N4)4s^3t^3/(3N^4). This is an actual error criterion, not merely the instruction to choose a “large” rank.

If instead s=Nhs=Nh with fixed h>0h>0, the same exact formulas give ⟨ON⟩=Nh\langle O_N\rangle=Nh and Var⁡(ON)=2h2\operatorname{Var}(O_N)=2h^2. Relative fluctuations still shrink, but the observable does not approach a finite mean. Its normalization and the parameter path both matter.

A sourced asymptotic statement has a domain

Section titled “A sourced asymptotic statement has a domain”

An exact finite-NN formula includes all rank dependence within its stated model. A large-NN expansion approximates a specified sequence. A strong-coupling expansion concerns a coupling parameter and need not include finite-rank corrections. An approximation may require both conditions, separately.

For one physical benchmark, the undeformed supersymmetric round-sphere partition function of the stated ABJM theory has

FS3(N,k)≡−log⁡ZS3(N,k)∼π2k3 N3/2,N→∞,k>0 fixed.(T15.8)F_{S^3}(N,k)\equiv-\log Z_{S^3}(N,k) \sim \frac{\pi\sqrt{2k}}3\,N^{3/2}, \qquad N\to\infty,\quad k>0\ \text{fixed}. \tag{T15.8}

This is the sourced leading result, not a derivation from (T15.3). FG, (4.27) and the following qualification give the fixed-level regime. Their free energy has the opposite sign, as also seen from their inverse transform and saddle exponent in (3.14)–(3.16).

Algebraically substituting k=N/λABk=N/\lambda_{\rm AB} into the displayed leading expression produces π2 N2/(3λAB)\pi\sqrt2\,N^2/(3\sqrt{\lambda_{\rm AB}}). That substitution alone establishes no approximation at fixed λAB\lambda_{\rm AB}: the omitted remainder was controlled at fixed kk. A uniform estimate would have to remain valid over the growing range of levels being used. Exercise 3 shows how the inference can fail even for elementary positive functions.

The same care applies to changing an observable with rank. Minahan explicitly warns after (5.7) that the color expansion changes when the number of fields in a traced operator grows sufficiently large (PDF p. 12). A fixed-operator calculation is not automatically uniform in operator size.

Repeat the Gaussian calculation on traceless Hermitian matrices XX, with the same induced metric and the same coefficient N/(2s)N/(2s). Find the exact mean and variance of Tr⁡X2/N\operatorname{Tr}X^2/N. Explain why the leading limit can agree with (T15.6) even though the finite-rank models differ.

Hint 1

There are N2−1N^2-1 orthonormal real directions. Alternatively write M=x0IN/N+XM=x_0I_N/\sqrt N+X.

Hint 2

The identity direction is orthogonal to every traceless matrix. Its Gaussian variable has variance s/Ns/N.

Solution

Replace the exponent N2/2N^2/2 in (T15.5) by (N2−1)/2(N^2-1)/2, leaving 2st/N22st/N^2 unchanged. Differentiating gives

⟨ON⟩traceless=s(1−1N2),Var⁡traceless(ON)=2s2N2(1−1N2).\langle O_N\rangle_{\rm traceless} =s\left(1-\frac1{N^2}\right),\qquad \operatorname{Var}_{\rm traceless}(O_N) =\frac{2s^2}{N^2}\left(1-\frac1{N^2}\right).

Independently, orthogonality gives ON(M)=ON(X)+x02/NO_N(M)=O_N(X)+x_0^2/N, with independent variables. The removed mean is s/N2s/N^2 and the removed variance is 2s2/N42s^2/N^4, exactly reproducing both differences. At N=2N=2 and s=3/2s=3/2, the traceless mean is 9/89/8 and variance 27/3227/32.

Both models approach mean ss at fixed ss, but their finite-rank answers are unequal. This is a comparison of Hermitian vector-space integrals, not a statement that the global gauge theories SU(N)SU(N) and U(N)U(N) are identical.

2. Choose allowed levels before taking the limit

Section titled “2. Choose allowed levels before taking the limit”

Give an integer sequence with λAB=3/2\lambda_{\rm AB}=3/2 exactly. Give one approaching λAB=2\lambda_{\rm AB}=\sqrt2, with an error bound. Finally classify (N,k)=(n3,n2)(N,k)=(n^3,n^2): is it either standard limit, and how do λAB\lambda_{\rm AB} and the normalized-trace coefficient kN/(4π)kN/(4\pi) scale?

Hint 1

For the rational target, multiply its numerator and denominator by the same positive integer. For the irrational target use the defining inequality for the floor function.

Hint 2

The condition k→∞k\to\infty alone does not fix N/kN/k. Keep the two growth rates.

Solution

Choose (N,k)=(3n,2n)(N,k)=(3n,2n) for the first target. For the second take k=nk=n, N=⌊2 n⌋N=\lfloor\sqrt2\,n\rfloor. Then

0≤2−Nk<1n.0\leq \sqrt2-\frac Nk<\frac1n.

Every member has integer positive level, while its ratio approaches the desired irrational value. Exact equality at finite integers is impossible.

For (n3,n2)(n^3,n^2), the ratio is λAB=n\lambda_{\rm AB}=n and the coefficient is n5/(4π)n^5/(4\pi). Both rank and level grow, but neither kk nor N/kN/k stays fixed. It is a third scaling path, entering large effective coupling even though 1/k→01/k\to0. The power n5n^5 belongs to this action coefficient; it does not compute the free energy.

Consider the explicitly defined positive function

A(N,k)=Ck N3/2(1+kN),C>0.\mathcal A(N,k) =C\sqrt k\,N^{3/2}\left(1+\frac{k}{N}\right), \qquad C>0.

Show that it has the same leading fixed-kk scaling as its first factor. Along an allowed sequence with N/k=λ0>0N/k=\lambda_0>0 fixed, find its ratio to that factor. Does large NN remove the relative error? What additional limit would remove it?

Hint 1

Use the relative remainder k/Nk/N, rather than the absolute difference of two growing quantities.

Hint 2

Substitute the entire exact function along the new sequence, not only its first factor.

Solution

At any fixed kk, the ratio is 1+k/N→11+k/N\to1, so A∼Ck N3/2\mathcal A\sim C\sqrt k\,N^{3/2}. Along a fixed rational λ0\lambda_0 sequence,

A=Cλ0N2(1+1λ0).\mathcal A =\frac{C}{\sqrt{\lambda_0}}N^2 \left(1+\frac1{\lambda_0}\right).

The fractional discrepancy from the substituted first factor is 1/λ01/\lambda_0, independent of NN. For λ0=3/2\lambda_0=3/2, it is 2/32/3, however large the ranks become. Sending λ0→∞\lambda_0\to\infty afterwards removes it. An integer sequence approaching an irrational λ0\lambda_0 has the same limiting ratio.

This constructed function is not an ABJM prediction. It proves that knowledge of a fixed-level leading term alone is insufficient to justify a fixed-ratio approximation. Additional control of the physical remainder would be needed.

A useful large-rank statement now includes the theory, its allowed parameter sequence, the normalized observable, and the approximation’s domain. Those choices must remain visible when color diagrams or eigenvalue methods supply the next calculation.