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N=4 SYM Field Content, Action, and Superconformal Data

Four-dimensional N=4\mathcal N=4 super-Yang–Mills theory packages a gauge connection, six adjoint scalars, and four adjoint Weyl fermions into one multiplet. Sixteen supersymmetries fix every relative interaction, but they do not choose the global gauge group or genuine-line spectrum. This page freezes a local su(N)\mathfrak{su}(N) convention, derives its action from ten dimensions, and records the superconformal data needed by later BPS and duality pages.

Required background. Extended supersymmetry gauge dynamics supplies the N=2\mathcal N=2 and N=1\mathcal N=1 decompositions. Superconformal algebras and the CFT handoff supplies the distinction between Poincaré and conformal supercharges and between shortening data and dynamical CFT data.

Helpful background. Supersymmetric Yang–Mills actions develops the lower-N\mathcal N component and superspace normalizations.

Local fields, trace, and supersymmetry transformations

Section titled “Local fields, trace, and supersymmetry transformations”

For the explicit card, take local gauge algebra su(N)\mathfrak{su}(N) with Hermitian generators

Tr⁡(TaTb)=12δab,\operatorname{Tr}(T^aT^b)=\frac12\delta^{ab},

where Tr⁡\operatorname{Tr} is the fundamental trace. Use the site’s (+−−−)(+---) metric and Hermitian adjoint-valued fields. The connection convention is

F=dA−iA∧A,DμXI=∂μXI−i[Aμ,XI].F=d\mathcal A-i\mathcal A\wedge\mathcal A, \qquad D_\mu X^I=\partial_\mu X^I-i[\mathcal A_\mu,X^I].

The on-shell fields transform under Spin(3,1)×SU(4)RSpin(3,1)\times SU(4)_R as

fieldLorentz representationSU(4)RSU(4)_R representationreal on-shell degrees of freedom per generator
Aμ\mathcal A_\muvector1\mathbf122
λαA\lambda^A_\alphaleft Weyl spinor4\mathbf488 fermionic in total
λˉα˙A\bar\lambda_{\dot\alpha A}right Weyl conjugate4‾\overline{\mathbf4}—
XIX^Iscalar6\mathbf666

Thus the multiplet has eight bosonic and eight fermionic on-shell degrees of freedom for each adjoint generator.

A compact way to display all sixteen supersymmetries is to begin in ten dimensions. Let M,N=0,…,9M,N=0,\ldots,9, let Ψ\Psi be a Majorana–Weyl adjoint spinor, and take

S10=1g102∫d10x Tr⁡ ⁣(−12FMNFMN+iΨˉΓMDMΨ).S_{10} =\frac1{g_{10}^2}\int d^{10}x\, \operatorname{Tr}\!\left( -\frac12F_{MN}F^{MN} +i\bar\Psi\Gamma^M D_M\Psi \right).

One consistent phase convention has

δεAM=iεˉΓMΨ,δεΨ=−12FMNΓMNε.\delta_\varepsilon \mathcal A_M =i\bar\varepsilon\Gamma_M\Psi, \qquad \delta_\varepsilon\Psi =-\frac12F_{MN}\Gamma^{MN}\varepsilon.

After using the fermion equation of motion, two transformations close into a translation plus a gauge transformation. Reversing the phase of Ψ\Psi changes both displayed transformation signs without changing the theory. The ten-dimensional construction and its reduction are given in Brink, Schwarz, and Scherk 1977, §§2–3.

For a formal reduction on a flat six-torus of volume V6V_6, retain only fields independent of the internal coordinates. Integrating those coordinates defines the four-dimensional coupling by

1gYM2=V6g102,or equivalentlygYM2=g102V6,\frac1{g_{\rm YM}^2}=\frac{V_6}{g_{10}^2}, \qquad\text{or equivalently}\qquad g_{\rm YM}^2=\frac{g_{10}^2}{V_6},

in the unrescaled zero-mode convention used here. Then set all internal derivatives to zero and identify

A3+I=XI,I=1,…,6.\mathcal A_{3+I}=X^I, \qquad I=1,\ldots,6.

The mixed and internal components of the ten-dimensional field strength become

Fμ,3+I=DμXI,F3+I,3+J=−i[XI,XJ].F_{\mu,3+I}=D_\mu X^I, \qquad F_{3+I,3+J}=-i[X^I,X^J].

Substitution into −FMNFMN/2-F_{MN}F^{MN}/2 fixes the relative coefficients. In the overall-coupling convention, the bosonic Minkowski action is

Sbos=1gYM2∫d4x Tr⁡ ⁣[−12FμνFμν+DμXIDμXI+12[XI,XJ][XI,XJ]]+θ8π2∫Tr⁡(F∧F).\begin{aligned} S_{\rm bos} ={}&\frac{1}{g_{\rm YM}^{2}}\int d^4x\, \operatorname{Tr}\!\left[ -\frac12 F_{\mu\nu}F^{\mu\nu} +D_\mu X^I D^\mu X^I +\frac12[X^I,X^J][X^I,X^J] \right]\\ &+\frac{\theta}{8\pi^2}\int\operatorname{Tr}(F\wedge F). \end{aligned}

With Tr⁡(TaTb)=δab/2\operatorname{Tr}(T^aT^b)=\delta^{ab}/2, the gauge term is −FμνaFaμν/(4gYM2)-F^a_{\mu\nu}F^{a\mu\nu}/(4g_{\rm YM}^2). This component normalization is the one compatible with the complex coupling below and with the D3-brane relation gYM2=4πgsg_{\rm YM}^2=4\pi g_s derived in the AdS5×S5_5\times S^5 parameter map.

Repeated I,JI,J are summed. Because XIX^I are Hermitian, [XI,XJ][X^I,X^J] is anti-Hermitian and

V(X)=−12gYM2Tr⁡[XI,XJ][XI,XJ]≥0.V(X) =-\frac{1}{2g_{\rm YM}^{2}} \operatorname{Tr}[X^I,X^J][X^I,X^J] \geq0.

The vacuum condition is therefore [XI,XJ]=0[X^I,X^J]=0 for every pair. The fermion kinetic and Yukawa terms descend together from iΨˉΓMDMΨi\bar\Psi\Gamma^M D_M\Psi; the six internal gamma matrices furnish the SU(4)RSU(4)_R-equivariant maps between the 4\mathbf4, 4‾\overline{\mathbf4}, and 6\mathbf6. This derivation is a stronger normalization check than matching the bosonic potential alone, because it fixes the Yukawa couplings as well.

Translating to canonically normalized fields

Section titled “Translating to canonically normalized fields”

Many perturbative calculations place gYMg_{\rm YM} inside the covariant derivative and give the quadratic kinetic terms unit normalization. Define

Aμ=gYMAμcan,XI=gYMXcanI,Ψ=gYMΨcan.\mathcal A_\mu=g_{\rm YM}A_\mu^{\rm can}, \qquad X^I=g_{\rm YM}X_{\rm can}^I, \qquad \Psi=g_{\rm YM}\Psi_{\rm can}.

Then

F(A)=gYM(dAcan−igYMAcan∧Acan),F(\mathcal A)=g_{\rm YM} \left(dA^{\rm can} -ig_{\rm YM}A^{\rm can}\wedge A^{\rm can}\right),

and the quadratic gauge term becomes

−12gYM2Tr⁡F(A)2⟶−12Tr⁡(dAcan)2=−14(dAa,can)2.-\frac{1}{2g_{\rm YM}^2}\operatorname{Tr}F(\mathcal A)^2 \longrightarrow -\frac12\operatorname{Tr}(dA^{\rm can})^2 =-\frac14(dA^{a,{\rm can}})^2.

So cubic and quartic vertices carry gYMg_{\rm YM} and gYM2g_{\rm YM}^2. Two physical quantities provide quick round-trip checks:

Tr⁡R Pexp⁡ ⁣(i∮A)=Tr⁡R Pexp⁡ ⁣(igYM∮Acan),\operatorname{Tr}_{R}\,\mathcal P \exp\!\left(i\oint\mathcal A\right) = \operatorname{Tr}_{R}\,\mathcal P \exp\!\left(ig_{\rm YM}\oint A^{\rm can}\right),

and, at a commuting scalar expectation value,

MW,α2=∑I∣α(XI)∣2=gYM2∑I∣α(XcanI)∣2.M_{W,\alpha}^{2} =\sum_I\lvert\alpha(X^I)\rvert^2 =g_{\rm YM}^{2}\sum_I \lvert\alpha(X_{\rm can}^I)\rvert^2.

Thus a quoted scalar expectation value is not meaningful across conventions until the kinetic normalization is stated.

In N=1\mathcal N=1 language the same multiplet is one vector superfield VV and three adjoint chiral fields Φi\Phi_i. After canonical normalization and a phase choice for the chirals, the superpotential can be written

W=2 gYM Tr⁡(Φ1[Φ2,Φ3]).W=\sqrt2\,g_{\rm YM}\, \operatorname{Tr}\bigl(\Phi_1[\Phi_2,\Phi_3]\bigr).

Anti-Hermitian generators or a different chiral-field phase can move a sign or a factor of ii. The invariant statement is that the superpotential coefficient is not an independent parameter: its magnitude and its relation to the gauge coupling are fixed by the hidden twelve supercharges.

With the Lorentzian path-integral weight eiSMe^{iS_M} and the topological sign above, Wick rotation gives the bosonic Euclidean action

SE,bos=1gYM2∫d4xE Tr⁡ ⁣[12FμνFμν+DμXIDμXI−12[XI,XJ][XI,XJ]]−iθν,ν=18π2∫Tr⁡(F∧F).\begin{aligned} S_{E,{\rm bos}} ={}&\frac1{g_{\rm YM}^2}\int d^4x_E\, \operatorname{Tr}\!\left[ \frac12F_{\mu\nu}F_{\mu\nu} +D_\mu X^I D_\mu X^I -\frac12[X^I,X^J][X^I,X^J] \right]\\ &-i\theta\nu, \qquad \nu=\frac1{8\pi^2}\int\operatorname{Tr}(F\wedge F). \end{aligned}

Every term in the first line is nonnegative for Hermitian fields. The theta term is imaginary, so SES_E is generally complex even though its real part is bounded below. Euclidean left- and right-handed spinors are independent complex variables; the Lorentzian Majorana conjugation cannot be imposed unchanged. A localization or instanton formula must therefore state its Euclidean reality condition and contour rather than infer them from the Minkowski card.

For the simply connected SU(N)SU(N) theory on a spin four-manifold, the chosen trace gives ν∈Z\nu\in\mathbb Z. The theta angle is then 2π2\pi periodic, and the local complex coupling is

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

For a unit (anti-)self-dual instanton, the real Euclidean action is 8π2/gYM28\pi^2/g_{\rm YM}^2, providing a direct check of the same normalization. These action and instanton conventions are displayed explicitly in Pestun 2012, §2, eq. (2.2), printed p. 9, and §5, printed pp. 36–37, PDF.

This local card is not yet a complete theory object. One must additionally specify a compact global form with Lie algebra su(N)\mathfrak{su}(N), the allowed bundle sectors, a maximal mutually local spectrum of genuine Wilson–’t Hooft lines, and any discrete theta datum. For quotient groups, ν\nu can be fractional on nontrivial bundles; a shift τ↦τ+1\tau\mapsto\tau+1 can then change the discrete datum rather than return to the same global theory. The exact finite charge lattices and their modular transport are developed on line operators, global forms, and discrete theta data; the global-theory orbit figure shows how one local su(2)\mathfrak{su}(2) card splits into three globally distinct nodes.

It is useful to keep the dependency explicit:

local algebra and action  ⟶  global form and genuine lines  ⟶  candidate duality arrow.\text{local algebra and action} \;\longrightarrow\; \text{global form and genuine lines} \;\longrightarrow\; \text{candidate duality arrow}.

The first item does not determine the second, and neither one proves the third.

Superconformal algebra and normalized local data

Section titled “Superconformal algebra and normalized local data”

At the conformal point, the symmetry algebra is psu(2,2∣4)\mathfrak{psu}(2,2|4). Its bosonic subalgebra is

so(4,2)⊕su(4)R,\mathfrak{so}(4,2)\oplus\mathfrak{su}(4)_R,

and it contains sixteen Poincaré supercharges QQ and sixteen conformal supercharges SS. The scalar superconformal primary at the bottom of the stress-tensor multiplet has Δ=2\Delta=2 and transforms in

20′=[0,2,0]\mathbf{20'}=[0,2,0]

of SU(4)RSU(4)_R. In the overall-coupling fields, a convenient unnormalized representative is

O2IJ=1gYM2Tr⁡ ⁣(XIXJ−δIJ6XKXK).\mathcal O_2^{IJ} =\frac1{g_{\rm YM}^2} \operatorname{Tr}\!\left( X^I X^J-\frac{\delta^{IJ}}6X^KX^K \right).

The 1/gYM21/g_{\rm YM}^2 compensates XI=gYMXcanIX^I=g_{\rm YM}X_{\rm can}^I; an additional numerical factor is chosen when its two-point function is set to a particular CFT normalization. Descendants of this multiplet include the stress tensor, supercurrents, SU(4)RSU(4)_R currents, and the exactly marginal operators tangent to the τ\tau conformal manifold. The multiplet and its correlator constraints are analyzed in Dolan and Osborn 2002, §§2–6, while the representation-theoretic classification is fixed in Córdova, Dumitrescu, and Intriligator 2019, §§2.2.4 and 5.1.4.

The Weyl-anomaly coefficients follow from the exact N=1\mathcal N=1 anomaly relations. The gaugino has R=1R=1, while the fermion in each of the three chiral multiplets has R=−1/3R=-1/3. Hence

Tr⁡R=dim⁡g [1+3(−1/3)]=0,\operatorname{Tr}R =\dim\mathfrak g\,[1+3(-1/3)]=0, Tr⁡R3=dim⁡g [1+3(−1/3)3]=89dim⁡g.\operatorname{Tr}R^3 =\dim\mathfrak g\,[1+3(-1/3)^3] =\frac89\dim\mathfrak g.

Using

a=332(3Tr⁡R3−Tr⁡R),c=132(9Tr⁡R3−5Tr⁡R),a=\frac{3}{32} \left(3\operatorname{Tr}R^3-\operatorname{Tr}R\right), \qquad c=\frac{1}{32} \left(9\operatorname{Tr}R^3-5\operatorname{Tr}R\right),

gives

a=c=14dim⁡g=N2−14for g=su(N).a=c=\frac14\dim\mathfrak g =\frac{N^2-1}{4} \qquad\text{for }\mathfrak g=\mathfrak{su}(N).

The anomaly relations are derived in Anselmi et al. 1998, §§2–3. Because aa and cc are local anomalies, they depend on the Lie algebra but not on the global form. Partition functions with background flux and genuine-line sectors can still distinguish global theories with the same aa and cc.

The displayed action is an electric-frame Lagrangian. It does not make magnetic lines local, choose a nonperturbative regulator preserving every desired structure, or prove S-duality. It also does not protect every operator. The Konishi multiplet is long, and its scaling dimension varies with τ\tau.

Nor does the flat-space card determine every curved-background counterterm or non-spin refinement. On a general four-manifold, fermion structure, global form, one-form backgrounds, quadratic refinements, and discrete theta phases must be supplied before a partition function is defined.

Mixing the two field normalizations. Writing D=d−igAD=d-igA while retaining an overall 1/g21/g^2 action double-counts the coupling. Translate the fields, Wilson line, and scalar expectation value together.

Reading a positive potential from its displayed sign alone. For Hermitian scalars the commutator is anti-Hermitian. The Lorentzian Lagrangian contains +[X,X]2/2+[X,X]^2/2, while the potential energy contains its negative.

Treating τ\tau as the whole theory. The same local τ\tau and Lie algebra can accompany different global forms, genuine lines, and discrete theta data.

1. Recover the scalar terms from ten dimensions

Section titled “1. Recover the scalar terms from ten dimensions”

Use FμI=DμXIF_{\mu I}=D_\mu X^I and FIJ=−i[XI,XJ]F_{IJ}=-i[X^I,X^J] to explain the relative factors 11 and 1/21/2 in the four-dimensional bosonic action.

Solution

In FMNFMNF_{MN}F^{MN}, the mixed components occur twice, as (μ,I)(\mu,I) and (I,μ)(I,\mu), so the ten-dimensional coefficient −1/2-1/2 becomes a scalar kinetic coefficient of magnitude 11. The internal pair is already summed over ordered I,JI,J and retains magnitude 1/21/2. Because FIJ=−i[XI,XJ]F_{IJ}=-i[X^I,X^J], the extra factor (−i)2=−1(-i)^2=-1, together with the internal metric signs, yields the displayed Lorentzian commutator term and a nonnegative potential energy.

Starting with A=gYMAcan\mathcal A=g_{\rm YM}A^{\rm can} and X=gYMXcanX=g_{\rm YM}X_{\rm can}, verify both the Wilson-loop exponent and the W-boson mass formula.

Solution

Substitution gives i∮A=igYM∮Acani\oint\mathcal A=ig_{\rm YM}\oint A^{\rm can}, so the two Wilson-loop expressions agree. Likewise α(X)=gYMα(Xcan)\alpha(X)=g_{\rm YM}\alpha(X_{\rm can}), and squaring and summing over II gives MW,α2=gYM2∑I∣α(XcanI)∣2M_{W,\alpha}^2=g_{\rm YM}^2\sum_I|\alpha(X_{\rm can}^I)|^2. Both checks fail if only the gauge field or only the scalar is rescaled.

3. Reproduce the Weyl-anomaly coefficients

Section titled “3. Reproduce the Weyl-anomaly coefficients”

Insert the displayed values of Tr⁡R\operatorname{Tr}R and Tr⁡R3\operatorname{Tr}R^3 into the anomaly relations and specialize to SU(N)SU(N).

Solution

Since Tr⁡R=0\operatorname{Tr}R=0,

a=93289dim⁡g=14dim⁡g,c=93289dim⁡g=14dim⁡g.a=\frac{9}{32}\frac89\dim\mathfrak g =\frac14\dim\mathfrak g, \qquad c=\frac{9}{32}\frac89\dim\mathfrak g =\frac14\dim\mathfrak g.

For su(N)\mathfrak{su}(N), dim⁡g=N2−1\dim\mathfrak g=N^2-1, so a=c=(N2−1)/4a=c=(N^2-1)/4.

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