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QED and Yang–Mills theory

Quantum electrodynamics and Yang–Mills theory use the same central idea—replace an ordinary derivative by a connection—but the consequences differ sharply. In QED the gauge algebra is Abelian, so the photon carries no electric charge and the covariant ghost determinant is field independent. In Yang–Mills theory the gauge bosons carry the non-Abelian charge, the curvature itself is nonlinear, and gauge, matter, and ghost interactions are tied to one coupling. This lesson develops that comparison far enough to check a perturbative calculation without attempting a survey of the Standard Model.

Required background. Vector fields and gauge redundancy supplies covariant gauge fixing and physical polarizations. Perturbative expansion and Feynman rules supplies the rule-extraction and fermion-sign conventions. Loops and regularization and renormalization and the renormalization group supply the regulator, counterterm, and running-coupling language used below.

Helpful background. Fermions, spin, and anticommutation fixes the Dirac propagator and closed-fermion-loop sign. Symmetry, currents, and Ward identities explains contact terms, while LSZ and tree amplitudes explains why an on-shell polarization-replacement test is stronger than a check on one Green function.

Connections and curvature distinguish the theories

Section titled “Connections and curvature distinguish the theories”

For QED, let qq be the signed charge of a Dirac field and choose

DμQED=μ+iqAμ,Fμν=μAννAμ.D_\mu^{\mathrm{QED}}=\partial_\mu+iqA_\mu, \qquad F_{\mu\nu}=\partial_\mu A_\nu-\partial_\nu A_\mu.

The local transformation

ψeiqλ(x)ψ,AμAμ+μλ\psi\longmapsto e^{-iq\lambda(x)}\psi, \qquad A_\mu\longmapsto A_\mu+\partial_\mu\lambda

makes DμψD_\mu\psi transform like ψ\psi and leaves FμνF_{\mu\nu} invariant. Moreover,

[DμQED,DνQED]=iqFμν.[D_\mu^{\mathrm{QED}},D_\nu^{\mathrm{QED}}] =iqF_{\mu\nu}.

With the (+)(+---) metric, a gauge-fixed QED action is

SQED=d4x[14FμνFμν+ψˉ(iγμDμQEDm)ψ12ξ(μAμ)2].S_{\mathrm{QED}}=\int\mathrm d^4x\left[ -\frac14F_{\mu\nu}F^{\mu\nu} +\bar\psi(i\gamma^\mu D_\mu^{\mathrm{QED}}-m)\psi -\frac1{2\xi}(\partial_\mu A^\mu)^2 \right].

Because iγμDμQED=iγμμqγμAμi\gamma^\mu D_\mu^{\mathrm{QED}} =i\gamma^\mu\partial_\mu-q\gamma^\mu A_\mu, the interaction is qψˉγμψAμ-q\bar\psi\gamma^\mu\psi A_\mu. This sign will determine the vertex below. The action, its current, and its covariant gauge fixing are derived in Schwartz 2014, §§ 13.1–13.3, pp. 224–236.

For Yang–Mills theory, let GG be a compact gauge group and write Aμ=AμaTRaA_\mu=A_\mu^aT_R^a in a unitary representation RR. We use Hermitian generators and the site convention

[TRa,TRb]=ifabcTRc,DμYM=μigAμ,g>0.[T_R^a,T_R^b]=if^{abc}T_R^c, \qquad D_\mu^{\mathrm{YM}}=\partial_\mu-igA_\mu, \qquad g>0.

If ψUψ\psi\mapsto U\psi, covariance requires

AμUAμU1ig(μU)U1.A_\mu\longmapsto UA_\mu U^{-1}-\frac{i}{g}(\partial_\mu U)U^{-1}.

The commutator now defines a matrix-valued curvature,

[DμYM,DνYM]=igFμν,Fμν=μAννAμig[Aμ,Aν],Fμνa=μAνaνAμa+gfabcAμbAνc.\begin{aligned} [D_\mu^{\mathrm{YM}},D_\nu^{\mathrm{YM}}]&=-igF_{\mu\nu},\\ F_{\mu\nu} &=\partial_\mu A_\nu-\partial_\nu A_\mu-ig[A_\mu,A_\nu],\\ F_{\mu\nu}^a &=\partial_\mu A_\nu^a-\partial_\nu A_\mu^a +g f^{abc}A_\mu^bA_\nu^c. \end{aligned}

Thus FμνUFμνU1F_{\mu\nu}\mapsto UF_{\mu\nu}U^{-1}, and a minimal action with Dirac matter is

Sinv=d4x[14FμνaFaμν+ψˉ(iγμDμYMm)ψ].S_{\mathrm{inv}}=\int\mathrm d^4x\left[ -\frac14F_{\mu\nu}^aF^{a\mu\nu} +\bar\psi(i\gamma^\mu D_\mu^{\mathrm{YM}}-m)\psi \right].

The commutator term in FF is the decisive difference: squaring the curvature forces cubic and quartic gauge interactions. Yang and Mills introduced this nonlinear gauge curvature in Yang and Mills 1954, pp. 191–195; a modern action-level derivation appears in Schwartz 2014, §§ 25.1–25.3, pp. 481–495.

The opposite signs displayed in the two covariant derivatives are conventions, not different physics. Here qq is a signed Abelian charge, whereas gg is positive and the sign is carried by the non-Abelian generator convention. When the generators commute, the identification gTRqgT_R\leftrightarrow -q turns DμYMD_\mu^{\mathrm{YM}} into DμQEDD_\mu^{\mathrm{QED}}. A calculation must transport this sign through the transformation law, curvature, action, and vertices; changing only one line is inconsistent.

Gauge fixing introduces ghosts only when the orbit derivative depends on the field

Section titled “Gauge fixing introduces ghosts only when the orbit derivative depends on the field”

The invariant gauge-field kinetic operator has null directions. In a linear covariant gauge, both theories add

Lgf=12ξ(μAμa)2,\mathcal L_{\mathrm{gf}} =-\frac1{2\xi}(\partial^\mu A_\mu^a)^2,

where the adjoint index is omitted in QED. The free gauge propagator is

Dμνab(p)=iδabp2+i0[ημν(1ξ)pμpνp2+i0].D_{\mu\nu}^{ab}(p) =\frac{-i\delta^{ab}}{p^2+i0} \left[ \eta_{\mu\nu} -(1-\xi)\frac{p_\mu p_\nu}{p^2+i0} \right].

This propagator acts in an enlarged gauge-fixed state space; its numerator is not a sum over physical polarizations.

The Faddeev–Popov determinant measures how the gauge function Ga[A]=μAμaG^a[A]=\partial^\mu A_\mu^a changes along a gauge orbit. In QED, δAμ=μλ\delta A_\mu=\partial_\mu\lambda, so δG=λ\delta G=\Box\lambda. The determinant is independent of AμA_\mu and can be absorbed into the overall normalization.

For Yang–Mills theory,

δAμa=(Dμα)a,(Dμα)a=μαa+gfabcAμbαc,\delta A_\mu^a=(D_\mu\alpha)^a, \qquad (D_\mu\alpha)^a =\partial_\mu\alpha^a+g f^{abc}A_\mu^b\alpha^c,

so δGa=μ(Dμα)a\delta G^a=\partial^\mu(D_\mu\alpha)^a depends on the gauge field. Grassmann fields ca,cˉac^a,\bar c^a exponentiate the determinant. With the same adjoint derivative, the gauge-fixing and ghost terms are

Lgf+gh=12ξ(μAμa)2cˉaμ(Dμc)a.\mathcal L_{\mathrm{gf+gh}} =-\frac1{2\xi}(\partial^\mu A_\mu^a)^2 -\bar c^a\partial^\mu(D_\mu c)^a.

After integrating by parts,

Lgh=(μcˉa)μca+gfabc(μcˉa)Aμbcc.\mathcal L_{\mathrm{gh}} =(\partial^\mu\bar c^a)\partial_\mu c^a +g f^{abc}(\partial^\mu\bar c^a)A_\mu^b c^c.

Ghosts therefore interact in Yang–Mills loops even though they are never physical external particles. The determinant construction is due to Faddeev and Popov 1967, pp. 29–30.

An auxiliary field BaB^a makes the organizing BRST symmetry nilpotent off shell. One consistent convention is

sAμa=(Dμc)a,sca=g2fabccbcc,scˉa=Ba,sBa=0,sψ=igcaTRaψ.\begin{aligned} sA_\mu^a&=(D_\mu c)^a, &sc^a&=-\frac g2f^{abc}c^bc^c,\\ s\bar c^a&=B^a, &sB^a&=0,\\ s\psi&=igc^aT_R^a\psi. \end{aligned}

Then Lgf+gh\mathcal L_{\mathrm{gf+gh}} follows by applying ss to cˉa(Aa+ξBa/2)\bar c^a(\partial\cdot A^a+\xi B^a/2) and eliminating BaB^a. The signs in scsc and sψs\psi are fixed by s2=0s^2=0, using both the anticommutation of the ghosts and the Jacobi identity. This is the perturbative BRST construction, not a claim that a linear gauge condition intersects every nonperturbative gauge orbit exactly once Becchi, Rouet, and Stora 1976, pp. 287–321.

Define the linear part of the Yang–Mills curvature by

Fμνa(0)=μAνaνAμa.F_{\mu\nu}^{a(0)} =\partial_\mu A_\nu^a-\partial_\nu A_\mu^a.

Expanding the gauge action gives

LYM=14Fμνa(0)Fa(0)μνg2fabcFμνa(0)AbμAcνg24fabcfadeAμbAνcAdμAeν.\begin{aligned} \mathcal L_{\mathrm{YM}} ={}&-\frac14F_{\mu\nu}^{a(0)}F^{a(0)\mu\nu}\\ &-\frac g2 f^{abc}F_{\mu\nu}^{a(0)}A^{b\mu}A^{c\nu}\\ &-\frac{g^2}{4}f^{abc}f^{ade} A_\mu^bA_\nu^cA^{d\mu}A^{e\nu}. \end{aligned}

The last two lines are the three- and four-gauge interactions. They are not optional additions, and their relative coefficient cannot be adjusted independently. The matter terms and their full vertex factors are

Lintvertex factorQEDqψˉγμψAμiqγμYang-Mills+gψˉγμTRaψAμa+igγμTRa\begin{array}{c|c|c} &\mathcal L_{\mathrm{int}}&\text{vertex factor}\\ \hline \mathrm{QED}&-q\bar\psi\gamma^\mu\psi A_\mu&-iq\gamma^\mu\\ \mathrm{Yang\text{-}Mills} &+g\bar\psi\gamma^\mu T_R^a\psi A_\mu^a &+ig\gamma^\mu T_R^a \end{array}

Use the Fourier transform f~(p)=d4xe+ipxf(x)\widetilde f(p)=\int\mathrm d^4x\,e^{+ip\cdot x}f(x) and take all momenta incoming. For Aμa(p)A_\mu^a(p), Aνb(q)A_\nu^b(q), and Aρc(r)A_\rho^c(r) with p+q+r=0p+q+r=0, the three-gauge vertex factor is

Vμνρabc(p,q,r)=gfabc[(qr)μηνρ+(rp)νηρμ+(pq)ρημν].\begin{aligned} \mathcal V_{\mu\nu\rho}^{abc}(p,q,r) =g f^{abc}\big[{} &(q-r)_\mu\eta_{\nu\rho} +(r-p)_\nu\eta_{\rho\mu}\\ &+(p-q)_\rho\eta_{\mu\nu} \big]. \end{aligned}

The derivative supplies the factor that makes this rule real in the stated Fourier convention; the four-gauge rule instead carries ig2-ig^2 times a sum of three ffff color tensors and metric products. For an incoming antighost momentum qq, the ghost–gauge vertex is

Vμabˉc=gfabcqμ.\mathcal V_\mu^{a\bar b c}=g f^{abc}q_\mu.

Reversing the oriented ghost contraction or moving the derivative to a different leg changes the rule. A closed ghost loop has the usual additional minus sign of a closed Grassmann loop. Complete momentum-space conventions and the four-gauge tensor are developed in Srednicki 2007, § 72, pp. 424–426 and on Yang–Mills color algebra and perturbative vertices.

The comparison is now structural:

FeatureQEDYang–Mills theory
Gauge algebraCommuting[Ta,Tb]=ifabcTc[T^a,T^b]=if^{abc}T^c
Gauge self-interactionNoneThree- and four-gauge vertices
Covariant ghostField-independent determinant; decouplesInteracting adjoint Grassmann field
Matter vertexCharge qqMatrix TRaT_R^a and coupling gg
Quantum identityWard–TakahashiSlavnov–Taylor

Color algebra reduces before momentum integration

Section titled “Color algebra reduces before momentum integration”

For each compact simple factor, define

trR(TRaTRb)=T(R)δab,TRaTRa=C2(R)1R,\operatorname{tr}_R(T_R^aT_R^b)=T(R)\delta^{ab}, \qquad T_R^aT_R^a=C_2(R)\mathbf1_R,

and

facdfbcd=CAδab.f^{acd}f^{bcd}=C_A\delta^{ab}.

Taking a trace of the Casimir relation gives the dimension check

dRC2(R)=dAT(R).d_R C_2(R)=d_A T(R).

For the fundamental representation of SU(N)SU(N) with T(F)=1/2T(F)=1/2,

dF=N,dA=N21,CF=N212N,CA=N.d_F=N, \qquad d_A=N^2-1, \qquad C_F=\frac{N^2-1}{2N}, \qquad C_A=N.

Two useful reductions are

TRbTRaTRb=(C2(R)12CA)TRa,fabefcde+fbcefade+fcaefbde=0.T_R^bT_R^aT_R^b =\left(C_2(R)-\frac12C_A\right)T_R^a, \qquad f^{abe}f^{cde}+f^{bce}f^{ade}+f^{cae}f^{bde}=0.

The second equation is Jacobi. For a color tensor with all external legs treated as incoming, gauge invariance also implies color conservation,

(iTia)C=0,\left(\sum_i\mathbf T_i^a\right)\mathcal C=0,

where an incoming antifundamental carries (Ta)T-(T^a)^T. Reduce these tensors before substituting numerical SU(N)SU(N) values; T(R)T(R), C2(R)C_2(R), and CAC_A answer different contractions.

The Abelian limit means that all generators commute, so fabc0f^{abc}\to0 and CA0C_A\to0. It is not the substitution N=1N=1 in formulas for SU(N)SU(N). In this limit the pure-gauge and ghost vertices vanish, the representation matrices become ordinary charges, and the nonlinear BRST and Slavnov–Taylor structures reduce to their Abelian forms.

Ward and Slavnov–Taylor identities test the complete result

Section titled “Ward and Slavnov–Taylor identities test the complete result”

Let S(p)S(p) be the full QED fermion propagator and let Γμ(p+k,p)\Gamma^\mu(p+k,p) denote the coupling-stripped one-particle-irreducible photon vertex. The Ward–Takahashi identity is

kμΓμ(p+k,p)=S1(p+k)S1(p).k_\mu\Gamma^\mu(p+k,p) =S^{-1}(p+k)-S^{-1}(p).

At tree level, Γμ=γμ\Gamma^\mu=\gamma^\mu. Between equal-mass on-shell spinors the right-hand side vanishes. Consequently a complete amplitude with an external photon must obey

M=εμ(k)Mμ,kμMμ=0.\mathcal M=\varepsilon_\mu(k)\mathcal M^\mu, \qquad k_\mu\mathcal M^\mu=0.

This makes the amplitude invariant under εμεμ+αkμ\varepsilon_\mu\mapsto\varepsilon_\mu+\alpha k_\mu and removes the longitudinal part of an internal photon propagator between conserved currents. Off shell, however, the contraction is a difference of inverse propagators, not zero. The original on-shell identity and its off-shell extension are Ward 1950, p. 182 and Takahashi 1957, pp. 371–375.

In Yang–Mills theory, the nonlinear gauge transformation and the interacting determinant prevent one simple linear identity from controlling every vertex. A BRST change of variables gives the functional Slavnov–Taylor equation, schematically

S(Γ)=0,\mathcal S(\Gamma)=0,

where Γ\Gamma includes sources for the nonlinear BRST variations. Differentiating this equation relates gauge, ghost, and matter propagators and vertices. It implies the same on-shell polarization-replacement test for a complete perturbative amplitude,

εμa(k)MaμkμMaμ=0,\varepsilon_\mu^a(k)\mathcal M^{a\mu} \longrightarrow k_\mu\mathcal M^{a\mu}=0,

but it does not imply that an arbitrary off-shell gauge-vertex contraction vanishes. The necessary ghost functions and inverse propagators appear in the off-shell identity. The generalized identities were derived independently in Taylor 1971, pp. 436–444 and Slavnov 1972, pp. 99–104.

Covariant quantization therefore separates internal bookkeeping from physical states. Ghosts, timelike modes, and longitudinal modes occur inside diagrams, but physical perturbative states are BRST cohomology classes: Qphys=0Q|\mathrm{phys}\rangle=0 with states differing by QχQ|\chi\rangle identified. When the Slavnov–Taylor identity is anomaly free, the scattering operator descends to this quotient and unphysical contributions cancel Kugo and Ojima 1978, pp. 459–462. Positivity and gauge-parameter independence belong to physical matrix elements, not to each gauge-fixed propagator, diagram, or cut.

Renormalization must preserve the constrained interaction pattern

Section titled “Renormalization must preserve the constrained interaction pattern”

Write the Yang–Mills bare quantities as

A0=ZA1/2A,c0=Zc1/2c,ψ0=Zψ1/2ψ,g0=μϵZgg.A_0=Z_A^{1/2}A, \qquad c_0=Z_c^{1/2}c, \qquad \psi_0=Z_\psi^{1/2}\psi, \qquad g_0=\mu^\epsilon Z_g g.

The Slavnov–Taylor identity requires the complete multiplicative factors of the interaction terms to be compatible with one ZgZ_g:

Z3A=ZgZA3/2,Z4A=Zg2ZA2,ZcˉcA=ZgZcZA1/2,ZψˉψA=ZgZψZA1/2.\begin{aligned} Z_{3A}&=Z_gZ_A^{3/2}, &Z_{4A}&=Z_g^2Z_A^2,\\ Z_{\bar c cA}&=Z_gZ_cZ_A^{1/2}, &Z_{\bar\psi\psi A}&=Z_gZ_\psi Z_A^{1/2}. \end{aligned}

Thus extracting ZgZ_g from two different vertices must agree after the appropriate wave-function factors are divided out. A symmetry-breaking regulator may require finite restoring counterterms; an uncanceled gauge anomaly prevents restoration. The corresponding Abelian statement is the QED relation Z1=Z2Z_1=Z_2, which follows from the Ward–Takahashi identity and leaves charge renormalization tied to photon vacuum polarization. These constraints and their perturbative use are developed in Srednicki 2007, § 74, pp. 435–442.

One-loop running provides a useful normalization and sign check. For Dirac QED species with qf=eQfq_f=eQ_f,

β(e)=μdedμ=e312π2fQf2+O(e5).\beta(e) =\mu\frac{\mathrm de}{\mathrm d\mu} =\frac{e^3}{12\pi^2}\sum_f Q_f^2+O(e^5).

For Yang–Mills theory with Dirac fermions in representations RfR_f,

β(g)=g316π2[113CA43fT(Rf)]+O(g5).\beta(g) =-\frac{g^3}{16\pi^2} \left[ \frac{11}{3}C_A -\frac{4}{3}\sum_f T(R_f) \right] +O(g^5).

When the algebra is Abelian, CA=0C_A=0 and T(Rf)=Qf2T(R_f)=Q_f^2, so the second formula reproduces the positive QED coefficient. This cross-check requires the ghost contribution in the non-Abelian gauge-sector sum. The coefficients, their gauge-parameter cancellation, and the one-loop domain are derived in Srednicki 2007, § 78, pp. 465–471 and Schwartz 2014, §§ 26.4–26.6, pp. 517–528.

These beta functions assume four-dimensional perturbation theory and a mass-independent description above the relevant thresholds. Thresholds require matching, higher coefficients depend more strongly on the renormalization scheme, and a running coupling is not itself an observable. A negative leading Yang–Mills beta function establishes weak ultraviolet coupling when the bracket is positive; it does not by itself prove confinement or a mass gap.

Before trusting a gauge-theory calculation

Section titled “Before trusting a gauge-theory calculation”

Use the following checks on the complete result, not on a conveniently chosen diagram:

  1. Theory data: state the gauge group, global representation content needed for the calculation, generator normalization, signed charges, and Fourier convention.
  2. Action signs: recompute [Dμ,Dν][D_\mu,D_\nu] and expand ψˉiγμDμψ\bar\psi i\gamma^\mu D_\mu\psi. The curvature and matter vertices must follow from the same DμD_\mu.
  3. Gauge fixing: record ξ\xi, the gauge propagator, the Faddeev–Popov operator, and whether ghosts interact.
  4. Diagram content: include every graph at the stated order, including closed fermion and ghost loops with their Grassmann signs.
  5. Algebra: reduce Lorentz and color contractions symbolically; test Jacobi, Casimir identities, dimensions, and the Abelian limit.
  6. Physical states and identities: apply the Ward or Slavnov–Taylor contraction to the complete amplitude and keep ghosts and auxiliary polarizations out of the external state set.
  7. Renormalization: state the regulator and scheme, compare coupling renormalization from independent vertices, remove the regulator at fixed input, and label the perturbative and infrared limits of the conclusion.

A disagreement should be traced back to one of these declared ingredients. Adjusting an isolated sign until one identity happens to vanish can conceal a second inconsistency elsewhere.

This lesson treats unbroken, perturbative QED and Yang–Mills theory in linear covariant gauges around the usual vacuum. It does not derive the Higgs mechanism, electroweak mixing, chiral gauge-anomaly cancellation, the Standard Model matter content, or QCD factorization. Those require additional fields and assumptions rather than more terms appended to the formulas above.

Several limitations are already present inside this scope. Linear covariant gauge fixing is local in field space and does not resolve Gribov copies globally. Perturbative colored gauge bosons are useful short-distance external states, but confinement prevents interpreting them as nonperturbative asymptotic particles in QCD. In massless QED, ordinary charged-particle LSZ amplitudes have infrared difficulties and must ultimately be replaced by suitable inclusive or dressed observables. BRST cohomology and Slavnov–Taylor identities also assume compatible boundary conditions and no gauge anomaly. Ultraviolet renormalizability settles none of these infrared or global questions.

  1. Starting from the two covariant derivatives used on this page, derive both commutators and both matter-vertex signs. Then show how the commuting limit of the Yang–Mills convention becomes the QED convention.

    Solution

    In QED, multiplication by AμA_\mu commutes, so acting on a test field gives

    [μ+iqAμ,ν+iqAν]=iq(μAννAμ)=iqFμν.[\partial_\mu+iqA_\mu,\partial_\nu+iqA_\nu] =iq(\partial_\mu A_\nu-\partial_\nu A_\mu) =iqF_{\mu\nu}.

    The matter kinetic term expands as

    ψˉiγμ(μ+iqAμ)ψ=ψˉiγμμψqψˉγμAμψ.\bar\psi i\gamma^\mu(\partial_\mu+iqA_\mu)\psi =\bar\psi i\gamma^\mu\partial_\mu\psi -q\bar\psi\gamma^\mu A_\mu\psi.

    Multiplication by ii in the perturbative expansion eiSe^{iS} therefore gives the vertex iqγμ-iq\gamma^\mu.

    In Yang–Mills theory, matrix multiplication matters:

    [μigAμ,νigAν]=ig(μAννAμ)g2[Aμ,Aν]=igFμν.\begin{aligned} [\partial_\mu-igA_\mu,\partial_\nu-igA_\nu] ={}&-ig(\partial_\mu A_\nu-\partial_\nu A_\mu)\\ &-g^2[A_\mu,A_\nu]\\ ={}&-igF_{\mu\nu}. \end{aligned}

    Since [Aμ,Aν]=ifabcAμaAνbTc[A_\mu,A_\nu]=i f^{abc}A_\mu^aA_\nu^bT^c, this gives Fμνa=μAνaνAμa+gfabcAμbAνcF_{\mu\nu}^a=\partial_\mu A_\nu^a-\partial_\nu A_\mu^a +g f^{abc}A_\mu^bA_\nu^c. The matter term is

    ψˉiγμ(μigAμ)ψ=ψˉiγμμψ+gψˉγμAμaTRaψ,\bar\psi i\gamma^\mu(\partial_\mu-igA_\mu)\psi =\bar\psi i\gamma^\mu\partial_\mu\psi +g\bar\psi\gamma^\mu A_\mu^aT_R^a\psi,

    hence the vertex is +igγμTRa+ig\gamma^\mu T_R^a. If the generators commute, set gTR=qgT_R=-q. Then μigAμTR=μ+iqAμ\partial_\mu-igA_\mu T_R=\partial_\mu+iqA_\mu, and the vertex becomes iqγμ-iq\gamma^\mu. Every sign has crossed the bridge together.

  2. Derive the Faddeev–Popov operator in Lorenz gauge for QED and Yang–Mills theory. Explain precisely why only the non-Abelian ghost interacts.

    Solution

    With G[A]=AG[A]=\partial\cdot A, the QED variation is

    δλG=μμλ=λ.\delta_\lambda G =\partial^\mu\partial_\mu\lambda =\Box\lambda.

    Thus one may take M=\mathcal M=-\Box. It contains no AμA_\mu, so detM\det\mathcal M is the same for every field configuration and cancels in normalized correlators. Introducing Abelian ghosts would only produce a free determinant with no coupling to photons.

    For Yang–Mills theory,

    δαGa=μ(Dμα)a,Mab[A]=μDμab[A].\delta_\alpha G^a =\partial^\mu(D_\mu\alpha)^a, \qquad \mathcal M^{ab}[A] =-\partial^\mu D_\mu^{ab}[A].

    Because Dμab=δabμ+gfacbAμcD_\mu^{ab}=\delta^{ab}\partial_\mu+g f^{acb}A_\mu^c in the declared index ordering, M[A]\mathcal M[A] depends on AA. Exponentiating its determinant gives

    cˉaμ(Dμc)a(μcˉa)μca+gfabc(μcˉa)Aμbcc,-\bar c^a\partial^\mu(D_\mu c)^a \doteq (\partial^\mu\bar c^a)\partial_\mu c^a +g f^{abc}(\partial^\mu\bar c^a)A_\mu^b c^c,

    where \doteq denotes equality after discarding the boundary term. The second term is the ghost–gauge interaction. Setting fabc=0f^{abc}=0 removes it and recovers the QED result.

  3. Let k=ppk=p'-p and let u(p)u(p) and u(p)u(p') be on-shell spinors of the same mass. Prove the tree-level QED Ward contraction and use it to remove the gauge-parameter-dependent part of a photon exchange.

    Solution

    The Dirac equations are

    (p ⁣ ⁣ ⁣/m)u(p)=0,uˉ(p)(p ⁣ ⁣ ⁣/m)=0.(p\!\!\!/-m)u(p)=0, \qquad \bar u(p')(p'\!\!\!/-m)=0.

    Therefore

    kμuˉ(p)γμu(p)=uˉ(p)(p ⁣ ⁣ ⁣/p ⁣ ⁣ ⁣/)u(p)=muˉ(p)u(p)muˉ(p)u(p)=0.\begin{aligned} k_\mu\bar u(p')\gamma^\mu u(p) &=\bar u(p')(p'\!\!\!/-p\!\!\!/)u(p)\\ &=m\bar u(p')u(p)-m\bar u(p')u(p)=0. \end{aligned}

    This is the tree-level, on-shell limit of kμΓμ=S1(p)S1(p)k_\mu\Gamma^\mu=S^{-1}(p')-S^{-1}(p). If two conserved currents exchange a photon, the gauge-dependent propagator term is proportional to

    Jμ(k)kμkνJν(k).J^\mu(k)k_\mu k_\nu J'^\nu(-k).

    Each factor vanishes by current conservation, so the exchange is independent of ξ\xi. This conclusion applies after the complete conserved currents have been assembled; an individual diagram or an off-shell vertex need not vanish under the same contraction.

  4. For the SU(N)SU(N) fundamental representation with tr(TaTb)=δab/2\operatorname{tr}(T^aT^b)=\delta^{ab}/2, derive CFC_F and reduce TbTaTbT^bT^aT^b.

    Solution

    By definition, TaTa=CF1NT^aT^a=C_F\mathbf1_N, with the adjoint index summed. Taking the trace gives

    NCF=a=1N21tr(TaTa)=N212,NC_F =\sum_{a=1}^{N^2-1}\operatorname{tr}(T^aT^a) =\frac{N^2-1}{2},

    hence

    CF=N212N.C_F=\frac{N^2-1}{2N}.

    Next use the adjoint Casimir through the double commutator,

    [Tb,[Tb,Ta]]=CATa.[T^b,[T^b,T^a]]=C_A T^a.

    Expanding the left-hand side and using TbTb=CF1T^bT^b=C_F\mathbf1 gives

    2CFTa2TbTaTb=CATa.2C_FT^a-2T^bT^aT^b=C_AT^a.

    Therefore

    TbTaTb=(CF12CA)Ta.T^bT^aT^b =\left(C_F-\frac12C_A\right)T^a.

    For SU(N)SU(N), CA=NC_A=N, so the coefficient is

    N212NN2=12N.\frac{N^2-1}{2N}-\frac N2=-\frac1{2N}.

    The negative result is a useful test that CFC_F and CAC_A have not been confused.

  5. Suppose a renormalized Yang–Mills calculation determines the three-gauge and ghost–gauge vertex factors Z3AZ_{3A} and ZcˉcAZ_{\bar c cA}, together with ZAZ_A and ZcZ_c. Give two extractions of ZgZ_g and state what a disagreement means.

    Solution

    The Slavnov–Taylor-compatible factorizations are

    Z3A=ZgZA3/2,ZcˉcA=ZgZcZA1/2.Z_{3A}=Z_gZ_A^{3/2}, \qquad Z_{\bar c cA}=Z_gZ_cZ_A^{1/2}.

    Hence

    Zg(3A)=Z3AZA3/2,Zg(cˉcA)=ZcˉcAZc1ZA1/2.Z_g^{(3A)}=Z_{3A}Z_A^{-3/2}, \qquad Z_g^{(\bar c cA)} =Z_{\bar c cA}Z_c^{-1}Z_A^{-1/2}.

    They must agree through the calculated order after all diagrams, subdivergence counterterms, and finite symmetry-restoring terms required by the chosen regulator have been included. A disagreement is not evidence for two independent gauge couplings. It indicates missing diagrams—often a ghost contribution—an inconsistent color or sign convention, an incomplete subtraction, or an anomalous symmetry breaking. Only the last possibility can remain after every allowed local counterterm is exhausted.

Continue from gauge structure to controlled predictions

Section titled “Continue from gauge structure to controlled predictions”

You are ready to continue when you can derive both curvatures from their covariant derivatives, explain why the non-Abelian ghost interacts, reconstruct the vertex signs from the action, reduce the basic color factors, apply the correct on-shell or off-shell identity, and compare coupling renormalization across independent vertices without overextending the perturbative conclusion.

Continue to effective field theory and matching to organize physics across separated scales, then to infrared-safe observables and synthesis to turn massless gauge-theory amplitudes into defensible predictions. For a deeper theory-specific treatment, enter the QED chapter or the Yang–Mills chapter.

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