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QED Vertices and Tree Amplitudes

Gauge redundancy is not yet a theory of charged matter. It tells us that the vector potential AμA_\mu contains unphysical components, and it tells us that local phase rotations must be compensated by a connection. The next step is to ask what that connection does in perturbation theory. The answer is QED: replace ordinary derivatives by covariant derivatives, expand the action, and read off the vertices.

This page develops the first tree-level rules for scalar QED and spinor QED. The scalar theory is useful because it makes the structure of minimal coupling visible: the covariant derivative produces not only a one-photon vertex, but also a two-photon contact vertex. The spinor theory is closer to ordinary electron–photon physics: its basic interaction is the current vertex ψˉγμψAμ\bar\psi\gamma^\mu\psi A_\mu, and one-photon exchange already contains the Coulomb force in its nonrelativistic limit.

The conceptual point is sharper than the formulas themselves. Gauge invariance does not merely suggest an interaction. It correlates different diagrams. A photon polarization can be shifted by a multiple of its momentum, and a physical amplitude must not change. At tree level this becomes a concrete algebraic statement: terms proportional to kμk_\mu cancel after using the equations of motion and after including all diagrams required by minimal coupling.

Required background. Vector fields and gauge redundancy supplies the photon propagator, polarization equivalence, and covariant-derivative convention. Dirac-field quantization and propagators supplies external spinors, spin sums, and the fermion propagator.

A bookkeeping choice independent of charge is whether every momentum is drawn incoming to a vertex or physical incoming/outgoing momenta are followed along a matter line. Compact vertices below use the physical-line convention; the all-incoming translation is given afterward. The invariant check is the Ward identity, not the memorized sign of an isolated vertex.

A complex scalar field has a global phase symmetry

ϕ↦eiqαϕ,ϕ∗↦e−iqαϕ∗.\phi\mapsto e^{iq\alpha}\phi, \qquad \phi^*\mapsto e^{-iq\alpha}\phi^*.

If α\alpha is constant, the free Lagrangian

L0=(∂μϕ)∗(∂μϕ)−m2ϕ∗ϕ\mathcal L_0=(\partial_\mu\phi)^*(\partial^\mu\phi)-m^2\phi^*\phi

is invariant. If α=α(x)\alpha=\alpha(x), the derivative of ϕ\phi transforms with an extra term:

∂μϕ↦eiqα(x)(∂μϕ+iq(∂μα)ϕ).\partial_\mu\phi\mapsto e^{iq\alpha(x)} \left(\partial_\mu\phi+iq(\partial_\mu\alpha)\phi\right).

The cure is to introduce AμA_\mu and replace ∂μ\partial_\mu by

Dμϕ=(∂μ−iqAμ)ϕ.D_\mu\phi=(\partial_\mu-iqA_\mu)\phi.

With Aμ↦Aμ+∂μαA_\mu\mapsto A_\mu+\partial_\mu\alpha, one finds

Dμϕ↦eiqα(x)Dμϕ.D_\mu\phi\mapsto e^{iq\alpha(x)}D_\mu\phi.

The gauge-invariant scalar QED Lagrangian is therefore

Lscalar QED=−14FμνFμν+(Dμϕ)∗(Dμϕ)−m2ϕ∗ϕ,Fμν=∂μAν−∂νAμ.\mathcal L_{\mathrm{scalar\ QED}} =-{1\over4}F_{\mu\nu}F^{\mu\nu} +(D_\mu\phi)^*(D^\mu\phi)-m^2\phi^*\phi, \qquad F_{\mu\nu}=\partial_\mu A_\nu-\partial_\nu A_\mu.

Expanding the covariant derivative gives

Lscalar QED=−14FμνFμν+∂μϕ∗∂μϕ−m2ϕ∗ϕ+iqAμ(ϕ∗∂μϕ−(∂μϕ∗)ϕ)+q2AμAμϕ∗ϕ.\mathcal L_{\mathrm{scalar\ QED}} =-{1\over4}F_{\mu\nu}F^{\mu\nu} +\partial_\mu\phi^*\partial^\mu\phi-m^2\phi^*\phi +iqA_\mu\left(\phi^*\partial^\mu\phi-(\partial^\mu\phi^*)\phi\right) +q^2A_\mu A^\mu\phi^*\phi.

There are two interaction terms. The term linear in AμA_\mu gives a one-photon scalar vertex. The term quadratic in AμA_\mu gives a contact vertex with two photons and two scalars. That contact term is often called the seagull vertex because of its shape in diagrams.

For a scalar line with charge flowing from incoming momentum pp to outgoing momentum p′p', and with the photon index μ\mu, the three-point vertex is

+iq(p+p′)μ.+iq(p+p')^\mu.

For two photons with indices μ,ν\mu,\nu, the four-point scalar–scalar–photon–photon vertex is

2iq2ημν.2iq^2\eta^{\mu\nu}.

The factor of 22 comes from the two identical photon fields in AμAμA_\mu A^\mu. It is not optional; without it, Ward identities fail.

A reliable way to check scalar-QED signs is to contract the one-photon vertex with the incoming photon momentum. With k=p′−pk=p'-p and equal-mass scalar legs,

k⋅(p+p′)=p′2−p2=0k\cdot(p+p')=p'^2-p^2=0

on shell. For amplitudes with two external photons, the same cancellation leaves contact terms, and those are precisely canceled by the seagull vertex.

Scalar and spinor QED vertices generated by minimal coupling

Minimal coupling produces different elementary vertices for scalar and spinor matter. Scalar QED has both the one-photon vertex +iq(p+p′)μ+iq(p+p')^\mu and the seagull vertex 2iq2ημν2iq^2\eta^{\mu\nu}. Spinor QED has the current vertex +iqγμ+iq\gamma^\mu, which becomes −ieγμ-ie\gamma^\mu for an electron of charge q=−eq=-e.

For a Dirac field, the gauge-invariant Lagrangian is

Lspinor QED=−14FμνFμν+ψˉ(iγμDμ−m)ψ.\mathcal L_{\mathrm{spinor\ QED}} =-{1\over4}F_{\mu\nu}F^{\mu\nu} +\bar\psi(i\gamma^\mu D_\mu-m)\psi.

For a field of charge qq,

Dμψ=(∂μ−iqAμ)ψ,D_\mu\psi=(\partial_\mu-iqA_\mu)\psi,

so

ψˉ(iγμDμ−m)ψ=ψˉ(iγμ∂μ−m)ψ+qψˉγμψAμ.\bar\psi(i\gamma^\mu D_\mu-m)\psi =\bar\psi(i\gamma^\mu\partial_\mu-m)\psi +q\bar\psi\gamma^\mu\psi A_\mu.

Thus

Lint=qψˉγμψAμ.\mathcal L_{\mathrm{int}}=q\bar\psi\gamma^\mu\psi A_\mu.

For the electron, q=−eq=-e, so

Lint=−eψˉγμψAμ,vertex=−ieγμ.\mathcal L_{\mathrm{int}}=-e\bar\psi\gamma^\mu\psi A_\mu, \qquad \text{vertex}=-ie\gamma^\mu.

The difference between scalar QED and spinor QED is worth pausing over. The scalar kinetic term is quadratic in derivatives, so replacing ∂\partial by DD produces both Aϕ∂ϕA\phi\partial\phi and A2ϕ2A^2\phi^2 interactions. The Dirac kinetic term is first order, so minimal coupling produces only one power of AμA_\mu. There is no elementary two-photon–two-fermion seagull vertex in ordinary spinor QED.

The charge-weighted coefficient of AμA_\mu in the interaction is

jqμ=qψˉγμψ.j_q^\mu=q\bar\psi\gamma^\mu\psi.

Thus Lint=Aμjqμ\mathcal L_{\mathrm{int}}=A_\mu j_q^\mu. For the electron, jqμ=−eψˉγμψj_q^\mu=-e\bar\psi\gamma^\mu\psi, consistently giving the vertex −ieγμ-ie\gamma^\mu. With the previous page’s Maxwell-source convention Lsource=−Jsource ⁣⋅A\mathcal L_{\mathrm{source}}=-J_{\mathrm{source}}\!\cdot A, the source in ∂μFμν=Jsourceν\partial_\mu F^{\mu\nu}=J_{\mathrm{source}}^\nu is instead Jsourceμ=−jqμJ_{\mathrm{source}}^\mu=-j_q^\mu. This last minus sign is a dictionary between two named conventions, not an additional vertex sign.

It is useful to fix what a diagram means before assembling amplitudes. We define M\mathcal M by

⟨f∣S∣i⟩=⟨f∣i⟩+i(2π)4δ(4)(Pf−Pi)Mfi.\langle f|S|i\rangle =\langle f|i\rangle +i(2\pi)^4\delta^{(4)}(P_f-P_i)\mathcal M_{fi}.

Thus the product of propagators, vertices, and external wavefunctions supplied by a connected diagram is iMi\mathcal M. The free internal-line factors are

charged scalar:ip2−m2+iϵ,charged fermion:i(γ⋅p+m)p2−m2+iϵ,photon in Feynman gauge:−iημνk2+iϵ.\begin{aligned} \text{charged scalar:}\quad&{i\over p^2-m^2+i\epsilon},\\ \text{charged fermion:}\quad&{i(\gamma\cdot p+m)\over p^2-m^2+i\epsilon},\\ \text{photon in Feynman gauge:}\quad&{-i\eta_{\mu\nu}\over k^2+i\epsilon}. \end{aligned}

For physical incoming and outgoing momenta pp and p′p' along a matter line, the vertices are

Aμϕ∗ϕ:+iq(p+p′)μ,AμAνϕ∗ϕ:2iq2ημν,Aμψˉψ:+iqγμ.\begin{aligned} A_\mu\phi^*\phi:&\quad +iq(p+p')^\mu,\\ A_\mu A_\nu\phi^*\phi:&\quad 2iq^2\eta^{\mu\nu},\\ A_\mu\bar\psi\psi:&\quad +iq\gamma^\mu. \end{aligned}

In an all-incoming convention, if pϕp_\phi labels the ϕ\phi leg and pϕ∗p_{\phi^*} labels the ϕ∗\phi^* leg, the scalar three-point rule is +iq(pϕ−pϕ∗)μ+iq(p_\phi-p_{\phi^*})^\mu. Since an outgoing scalar of momentum p′p' is represented by an incoming ϕ∗\phi^* momentum −p′-p', this is the same rule as +iq(p+p′)μ+iq(p+p')^\mu. Incoming photons carry εμ\varepsilon_\mu and outgoing photons carry εμ∗\varepsilon_\mu^*; the complex conjugation is not optional for circular polarization.

External wavefunctions and the one-photon current

Section titled “External wavefunctions and the one-photon current”

At tree level, external fields are replaced by on-shell wavefunctions. For a fermion of momentum pp and spin ss,

(γ⋅p−m)us(p)=0,uˉs(p)(γ⋅p−m)=0.(\gamma\cdot p-m)u_s(p)=0, \qquad \bar u_s(p)(\gamma\cdot p-m)=0.

For a photon of momentum kk and polarization εμ(k)\varepsilon_\mu(k),

k2=0,k⋅ε(k)=0,εμ(k)∼εμ(k)+c kμ.k^2=0, \qquad k\cdot\varepsilon(k)=0, \qquad \varepsilon_\mu(k)\sim \varepsilon_\mu(k)+c\,k_\mu.

The last relation says that the representative of the polarization vector is gauge-dependent. A physical amplitude must be unchanged by replacing εμ\varepsilon_\mu by εμ+ckμ\varepsilon_\mu+c k_\mu.

The elementary electron current couples to a photon line through

uˉs′(p′) (−ieγμ) us(p) εμ(k),k=p′−p,\bar u_{s'}(p')\,(-ie\gamma^\mu)\,u_s(p)\,\varepsilon_\mu(k), \qquad k=p'-p,

as a contribution to the diagram value iMi\mathcal M. The current itself is well defined for momentum transfer k=p′−pk=p'-p that need not be lightlike, as in the virtual-photon exchange below. Its Ward check is immediate:

kμuˉs′(p′)γμus(p)=uˉs′(p′)γ⋅(p′−p)us(p).k_\mu\bar u_{s'}(p')\gamma^\mu u_s(p) =\bar u_{s'}(p')\gamma\cdot(p'-p)u_s(p).

Using the Dirac equation on the left and on the right,

uˉs′(p′)γ⋅p′=muˉs′(p′),γ⋅p us(p)=mus(p),\bar u_{s'}(p')\gamma\cdot p' = m\bar u_{s'}(p'), \qquad \gamma\cdot p\,u_s(p)=m u_s(p),

so

kμuˉs′(p′)γμus(p)=0.k_\mu\bar u_{s'}(p')\gamma^\mu u_s(p)=0.

This is the simplest form of current conservation on an external line. It is also the tree-level seed of the Ward–Takahashi identities. It does not describe an allowed isolated emission or absorption of a nonzero real photon by a stable massive electron in empty space. For absorption, p′=p+kp'=p+k with future-directed pp and nonzero future-directed null kk would give

p′2=m2+2p⋅k>m2,p'^2=m^2+2p\cdot k>m^2,

since in the electron rest frame p⋅k=mk0>0p\cdot k=m k^0>0. Emission has the same obstruction with pp and p′p' interchanged. The three-point current therefore serves here as a virtual-photon matrix element or an algebraic Ward check. Physical Compton scattering has two photons and the sum of two diagrams, as developed in the canonical tree-level QED calculation.

Replacing the photon polarization by its momentum annihilates the on-shell electron current

The on-shell electron-current Ward check, with equal electron masses and k=p′−pk=p'-p. Replacing εμ\varepsilon_\mu by kμk_\mu gives zero by the two Dirac equations. The diagram is schematic; it does not imply that an isolated electron can absorb or emit a nonzero real photon. In a physical process the appropriate full current or sum of diagrams must satisfy the Ward identity.

The simplest nontrivial QED amplitude is one-photon exchange. For two distinguishable charged fermions with electron-like vertex −ieγμ-ie\gamma^\mu, the tree contribution is

iM=[uˉ(p1′)(−ieγμ)u(p1)]−iημνq2+iϵ[uˉ(p2′)(−ieγν)u(p2)],q=p1′−p1=p2−p2′.i\mathcal M =\left[\bar u(p_1')(-ie\gamma^\mu)u(p_1)\right] { -i\eta_{\mu\nu}\over q^2+i\epsilon} \left[\bar u(p_2')(-ie\gamma^\nu)u(p_2)\right], \qquad q=p_1'-p_1=p_2-p_2'.

Equivalently,

M=e2[uˉ(p1′)γμu(p1)][uˉ(p2′)γμu(p2)]q2+iϵ,\mathcal M =e^2{\left[\bar u(p_1')\gamma^\mu u(p_1)\right] \left[\bar u(p_2')\gamma_\mu u(p_2)\right] \over q^2+i\epsilon},

for the stated SS-matrix and vertex conventions. More generally the numerator carries the product of the two charges, q1q2q_1q_2. The current–propagator–current structure is

J1μ(q) Dμν(q) J2ν(−q).J_1^\mu(q)\,D_{\mu\nu}(q)\,J_2^\nu(-q).

In a covariant gauge, the extra propagator numerator is proportional to qμqνq_\mu q_\nu. It drops out because the on-shell currents obey qμJ1μ=qνJ2ν=0q_\mu J_1^\mu=q_\nu J_2^\nu=0. This both checks the momentum assignments and proves that the exchange amplitude is independent of the gauge parameter.

One-photon exchange between two charged fermion lines

Tree-level photon exchange has the universal structure current–propagator–current. In Feynman gauge the internal photon contributes −iημν/(q2+iϵ)-i\eta_{\mu\nu}/(q^2+i\epsilon), while each fermion current contributes a spinor bilinear uˉγμu\bar u\gamma^\mu u.

The nonrelativistic limit recovers the Coulomb interaction. For a slowly moving fermion,

uˉ(p′)γ0u(p)≃2m,uˉ(p′)γiu(p)≪2m.\bar u(p')\gamma^0u(p)\simeq 2m, \qquad \bar u(p')\gamma^iu(p)\ll 2m.

The momentum transfer has q0≃0q^0\simeq0, hence

q2=(q0)2−q2≃−q2.q^2=(q^0)^2-\mathbf q^2\simeq-\mathbf q^2.

Therefore the dominant exchange is the temporal current coupled through

1q2.{1\over \mathbf q^2}.

More explicitly, for charges q1q_1 and q2q_2,

MNR≃−4m1m2q1q2q2.\mathcal M_{\mathrm{NR}} \simeq-{4m_1m_2q_1q_2\over\mathbf q^2}.

The relativistic Born-amplitude relation V~(q)=−MNR/(4m1m2)\widetilde V(\mathbf q)=-\mathcal M_{\mathrm{NR}}/(4m_1m_2) then gives

V~(q)=q1q2q2.\widetilde V(\mathbf q)={q_1q_2\over\mathbf q^2}.

Fourier transformation yields the Coulomb potential,

V(r)=q1q24πr.V(r)={q_1q_2\over4\pi r}.

This is a useful sanity check: the same minimal coupling that enforces local gauge invariance also reproduces the familiar long-range electromagnetic force.

Scalar Compton scattering and the seagull term

Section titled “Scalar Compton scattering and the seagull term”

Consider scalar Compton scattering,

ϕ(p)+γ(k,ε)⟶ϕ(p′)+γ(k′,ε′),p+k=p′+k′.\phi(p)+\gamma(k,\varepsilon)\longrightarrow \phi(p')+\gamma(k',\varepsilon'), \qquad p+k=p'+k'.

The scalar QED Lagrangian produces three tree diagrams: two exchange diagrams and one contact diagram. The contact diagram is required by gauge invariance.

Scalar QED Compton scattering diagrams with two exchange graphs and a contact graph

Scalar Compton scattering contains two scalar-exchange diagrams plus the A2ϕ∗ϕA^2\phi^*\phi contact interaction. The three diagrams are not separately gauge invariant; their sum is.

The three contributions have the schematic form

iMs=[+iq(2p+k)μεμ]i(p+k)2−m2+iϵ[+iq(2p′+k′)νεν′∗],i\mathcal M_s =\left[+iq(2p+k)^\mu\varepsilon_\mu\right] {i\over(p+k)^2-m^2+i\epsilon} \left[+iq(2p'+k')^\nu\varepsilon_\nu'^*\right], iMu=[+iq(2p−k′)νεν′∗]i(p−k′)2−m2+iϵ[+iq(2p′−k)μεμ],i\mathcal M_u =\left[+iq(2p-k')^\nu\varepsilon_\nu'^*\right] {i\over(p-k')^2-m^2+i\epsilon} \left[+iq(2p'-k)^\mu\varepsilon_\mu\right],

and

iMcontact=2iq2ημνεμεν′∗.i\mathcal M_{\mathrm{contact}} =2iq^2\eta^{\mu\nu}\varepsilon_\mu\varepsilon_\nu'^*.

The precise placement of signs depends on whether all momenta are drawn incoming or as physical incoming/outgoing momenta. A reliable way to avoid confusion is to keep the scalar charge flow fixed along the line and then translate to the chosen all-incoming convention only at the end. What does not depend on notation is the Ward identity:

M(εμ→kμ)=0,M(εν′∗→kν′)=0.\mathcal M(\varepsilon_\mu\to k_\mu)=0, \qquad \mathcal M(\varepsilon_\nu'^*\to k_\nu')=0.

The cancellation works because, on shell,

k⋅(2p+k)=(p+k)2−p2=(p+k)2−m2,k\cdot(2p+k)=(p+k)^2-p^2=(p+k)^2-m^2,

and similarly for the other scalar-exchange channel. Thus the numerator of an exchange diagram can cancel its scalar propagator. The leftover local terms are canceled by the contact diagram. This is the practical reason why the A2ϕ∗ϕA^2\phi^*\phi term cannot be ignored even when one is mainly interested in one-photon vertices.

For spinor QED,

e(p)+γ(k,ε)→e(p′)+γ(k′,ε′),p+k=p′+k′,e(p)+\gamma(k,\varepsilon)\to e(p')+\gamma(k',\varepsilon'), \qquad p+k=p'+k',

there are two tree diagrams. There is no seagull vertex because the Dirac Lagrangian is first order in derivatives. With the electron-like vertex −ieγμ-ie\gamma^\mu, the amplitude is

iMspinor=(−ie)2uˉ(p′)[(γ⋅ε′∗)i(γ⋅(p+k)+m)(p+k)2−m2+iϵ(γ⋅ε)+(γ⋅ε)i(γ⋅(p−k′)+m)(p−k′)2−m2+iϵ(γ⋅ε′∗)]u(p).i\mathcal M_{\mathrm{spinor}} =(-ie)^2\bar u(p') \left[ (\gamma\cdot\varepsilon'^*){i(\gamma\cdot(p+k)+m)\over (p+k)^2-m^2+i\epsilon}(\gamma\cdot\varepsilon) +(\gamma\cdot\varepsilon){i(\gamma\cdot(p-k')+m)\over (p-k')^2-m^2+i\epsilon}(\gamma\cdot\varepsilon'^*) \right]u(p).

Here

γ⋅ε=γμεμ,γ⋅ε′∗=γμεμ′∗.\gamma\cdot\varepsilon=\gamma^\mu\varepsilon_\mu, \qquad \gamma\cdot\varepsilon'^*=\gamma^\mu\varepsilon'^*_{\mu}.

The two terms are the two possible orderings of photon absorption and emission along the fermion line. Their matrix order matters because gamma matrices do not commute.

Spinor QED tree diagrams for Compton scattering

Spinor Compton scattering contains the two possible orderings of photon insertions along the fermion line. Gauge invariance belongs to the sum of the two diagrams, not to either diagram separately.

The Ward identity again comes from differences of inverse propagators. Strip off the common couplings and factors of ii, and write

Tνμ=uˉ(p′)[γνS0(p+k)γμ+γμS0(p−k′)γν]u(p),T^{\nu\mu} =\bar u(p')\left[ \gamma^\nu S_0(p+k)\gamma^\mu +\gamma^\mu S_0(p-k')\gamma^\nu \right]u(p),

where

S0(r)=γ⋅r+mr2−m2,S0−1(r)=γ⋅r−mS_0(r)={\gamma\cdot r+m\over r^2-m^2}, \qquad S_0^{-1}(r)=\gamma\cdot r-m

on the nonsingular internal momenta. Contract the incoming-photon index with kμk_\mu. In the first ordering use

γ⋅k=S0−1(p+k)−S0−1(p).\gamma\cdot k=S_0^{-1}(p+k)-S_0^{-1}(p).

The second term annihilates u(p)u(p), while the first cancels S0(p+k)S_0(p+k) and leaves uˉ(p′)γνu(p)\bar u(p')\gamma^\nu u(p). For the other ordering, momentum conservation gives

γ⋅k=S0−1(p′)−S0−1(p−k′).\gamma\cdot k=S_0^{-1}(p')-S_0^{-1}(p-k').

The first term annihilates uˉ(p′)\bar u(p') and the second cancels the internal propagator with the opposite sign. Consequently,

kμTνμ=uˉ(p′)γνu(p)−uˉ(p′)γνu(p)=0.k_\mu T^{\nu\mu} =\bar u(p')\gamma^\nu u(p) -\bar u(p')\gamma^\nu u(p)=0.

This telescoping cancellation is the fermionic counterpart of the scalar-QED cancellation among exchange and contact diagrams. Repeating the argument with kν′k'_\nu proves the Ward identity for the outgoing photon.

After writing an amplitude, one often squares it and sums or averages over unobserved spin states. With the standard relativistic normalization,

∑sus(p)uˉs(p)=γ⋅p+m,∑svs(p)vˉs(p)=γ⋅p−m.\sum_s u_s(p)\bar u_s(p)=\gamma\cdot p+m, \qquad \sum_s v_s(p)\bar v_s(p)=\gamma\cdot p-m.

The basic trace identities are

Tr⁡(γμγν)=4ημν,\operatorname{Tr}(\gamma^\mu\gamma^\nu)=4\eta^{\mu\nu},

and

Tr⁡(γμγνγργσ)=4(ημνηρσ−ημρηνσ+ημσηνρ).\operatorname{Tr}(\gamma^\mu\gamma^\nu\gamma^\rho\gamma^\sigma) =4\left( \eta^{\mu\nu}\eta^{\rho\sigma} -\eta^{\mu\rho}\eta^{\nu\sigma} +\eta^{\mu\sigma}\eta^{\nu\rho} \right).

For example, a spin-summed fermion current product becomes

∑s,s′[uˉs′(p′)γμus(p)][uˉs′(p′)γρus(p)]∗=Tr⁡[(γ⋅p′+m)γμ(γ⋅p+m)γρ].\sum_{s,s'} \left[\bar u_{s'}(p')\gamma^\mu u_s(p)\right] \left[\bar u_{s'}(p')\gamma^\rho u_s(p)\right]^* = \operatorname{Tr}\left[(\gamma\cdot p'+m)\gamma^\mu(\gamma\cdot p+m)\gamma^\rho\right].

Evaluating the trace gives

Lμρ(p′,p)=4[p′μpρ+p′ρpμ−ημρ(p′⋅p−m2)].L^{\mu\rho}(p',p) =4\left[p'^\mu p^\rho+p'^\rho p^\mu -\eta^{\mu\rho}(p'\cdot p-m^2)\right].

A sum and an average are different operations. For an unpolarized process, sum over every unobserved final spin or helicity and divide by the number of equally populated initial states:

∣M∣2‾=1∏a∈initialNa∑initial spinsfinal spins∣M∣2,\overline{|\mathcal M|^2} ={1\over\prod_{a\in\mathrm{initial}}N_a} \sum_{\substack{\text{initial spins}\\\text{final spins}}} |\mathcal M|^2,

where Na=2sa+1N_a=2s_a+1 for a massive particle and Na=2N_a=2 for a photon. For one-photon exchange between two incoming spin-one-half particles, the average factor is 1/41/4. Writing the charges as q1,q2q_1,q_2 and the momentum transfer as QQ, one obtains the useful trace form

∣M∣2‾=q12q22(Q2)2L1μνL2,μν,\overline{|\mathcal M|^2} ={q_1^2q_2^2\over(Q^2)^2} L_1^{\mu\nu}L_{2,\mu\nu},

where each averaged current tensor contains its own factor of 1/21/2,

Laμν=12Tr⁡ ⁣[(γ⋅pa′+ma)γμ(γ⋅pa+ma)γν].L_a^{\mu\nu} ={1\over2}\operatorname{Tr}\!\left[ (\gamma\cdot p_a'+m_a)\gamma^\mu (\gamma\cdot p_a+m_a)\gamma^\nu \right].

This separation is a useful defense against a common factor-of-two error: completeness relations perform sums, whereas the prefactor performs the initial-state average.

For photons, polarization sums must be handled with care. In a gauge-invariant amplitude, gauge-dependent pieces proportional to kμk_\mu do not contribute, so one may effectively use

∑λ∈physεμ(λ)(k)εν(λ)(k)∗  ⇝  −ημν\sum_{\lambda\in\mathrm{phys}}\varepsilon_\mu^{(\lambda)}(k) \varepsilon_\nu^{(\lambda)}(k)^* \;\rightsquigarrow\;-\eta_{\mu\nu}

inside a complete gauge-invariant squared amplitude. The arrow is deliberate: the equality is not an identity of physical polarization vectors in an arbitrary gauge; it is a shortcut justified by Ward identities. A good practical test is this: before replacing a physical-polarization sum by −ημν-\eta_{\mu\nu}, verify that the rest of the amplitude vanishes when any external polarization is replaced by its momentum.

A time-ordered Green function does not know in advance which external legs will be interpreted as incoming particles, outgoing particles, incoming antiparticles, or outgoing antiparticles. These interpretations are imposed by LSZ reduction and by the choice of which pole is approached. Moving a charged external leg from one side of a process to the other turns it into an antiparticle and reverses the sign of the momentum in the analytic amplitude.

Schematically,

M(A→B+fˉ(p))⟷M(A+f(−p)→B),\mathcal M\bigl(A\to B+\bar f(p)\bigr) \quad\longleftrightarrow\quad \mathcal M\bigl(A+f(-p)\to B\bigr),

with the spinor wavefunction changed from a vv spinor to a uu spinor, or conversely, depending on the direction of the fermion arrow.

The external-wavefunction dictionary is

external statespinor factorincoming fermionu(p)outgoing fermionuˉ(p)incoming antifermionvˉ(p)outgoing antifermionv(p)\begin{array}{c|c} \text{external state} & \text{spinor factor}\\ \hline \text{incoming fermion} & u(p)\\ \text{outgoing fermion} & \bar u(p)\\ \text{incoming antifermion} & \bar v(p)\\ \text{outgoing antifermion} & v(p) \end{array}

Thus crossing an outgoing antifermion replaces the analytically continued v(p)v(p) by an incoming-fermion u(−p)u(-p) assignment. For processes with several fermions, one must also preserve a fixed ordering of external fermionic operators. Reordering that convention can produce a relative minus sign; it is not captured by the shorthand p→−pp\to-p alone.

Crossing relation as moving an external charged leg across the amplitude

Crossing is the analytic continuation that moves an external leg across the amplitude. Momentum changes sign, and a particle becomes the corresponding antiparticle. Fermion arrows help keep the spinor factors in the correct order.

This is why Feynman rules are usually formulated with all momenta incoming and with continuous fermion-number arrows. Once the momentum and fermion ordering are fixed, the same analytic function describes several physical channels.

Minimal coupling converts a global phase symmetry into a local gauge symmetry by replacing ordinary derivatives with covariant derivatives. For a complex scalar, this produces both a one-photon vertex and a two-photon seagull vertex. For a Dirac field, the first-order kinetic term produces the current interaction ψˉγμψAμ\bar\psi\gamma^\mu\psi A_\mu and hence the familiar photon–fermion vertex.

Tree amplitudes are assembled from external wavefunctions, propagators, vertices, and momentum conservation. Their most important consistency test is gauge invariance: replacing an external photon polarization by its momentum must give zero. For a single on-shell fermion current this follows directly from the Dirac equation. For scalar Compton scattering it follows only after the exchange diagrams and the seagull diagram are added together.

Spin sums turn squared amplitudes into traces of gamma matrices. Crossing then explains why the same analytic expression can describe several reactions: moving a charged external leg across the amplitude changes a particle into an antiparticle and sends p→−pp\to-p. These are the practical tools needed before one-loop QED and power counting enter the course.

Omitting the scalar seagull. The A2ϕ∗ϕA^2\phi^*\phi vertex is required by minimal coupling. Exchange graphs alone do not satisfy the two-photon Ward identities.

Testing gauge invariance diagram by diagram. A single exchange graph need not be gauge invariant. Apply the polarization-to-momentum replacement to the complete set of diagrams at the chosen perturbative order.

Using −ημν-\eta_{\mu\nu} too early. This replacement is justified only inside a gauge-invariant squared amplitude. Gauge-dependent terms vanish after contraction with conserved currents or after the Ward-related diagrams have been summed.

Confusing sums with averages. Completeness relations sum over spin states; they do not divide by the number of initial states. Insert the initial-state average only once, after the amplitude has been squared.

Mixing charge signs with momentum-flow signs. The convention Dμ=∂μ−iqAμD_\mu=\partial_\mu-iqA_\mu gives a fermion vertex +iqγμ+iq\gamma^\mu; for q=−eq=-e this is −ieγμ-ie\gamma^\mu. The all-incoming convention changes the scalar momentum labels, not the underlying Ward identity.

Treating crossing as only p→−pp\to-p. A crossed fermion also changes between uu and vv wavefunctions, and a fixed ordering of external fermions must be maintained. Any relative Fermi sign comes from that ordering, not from an arbitrary sign attached to crossing.

Derive the scalar QED three-point and four-point vertices from

L=(Dμϕ)∗(Dμϕ)−m2ϕ∗ϕ,Dμ=∂μ−iqAμ.\mathcal L=(D_\mu\phi)^*(D^\mu\phi)-m^2\phi^*\phi, \qquad D_\mu=\partial_\mu-iqA_\mu.

Use the convention that the scalar enters with momentum pp and leaves with momentum p′p'.

Solution

Expanding the covariant derivative gives

(Dμϕ)∗(Dμϕ)=(∂μϕ∗+iqAμϕ∗)(∂μϕ−iqAμϕ).(D_\mu\phi)^*(D^\mu\phi) =(\partial_\mu\phi^*+iqA_\mu\phi^*) (\partial^\mu\phi-iqA^\mu\phi).

Thus

(Dμϕ)∗(Dμϕ)=∂μϕ∗∂μϕ+iqAμ(ϕ∗∂μϕ−(∂μϕ∗)ϕ)+q2AμAμϕ∗ϕ.(D_\mu\phi)^*(D^\mu\phi) =\partial_\mu\phi^*\partial^\mu\phi +iqA_\mu\left(\phi^*\partial^\mu\phi-(\partial^\mu\phi^*)\phi\right) +q^2A_\mu A^\mu\phi^*\phi.

The term linear in AμA_\mu gives the one-photon vertex. With the standard scalar-line momentum assignment, the two derivative terms combine into (p+p′)μ(p+p')^\mu. Including the factor of ii from iSintiS_{\mathrm{int}}, the vertex is

+iq(p+p′)μ.+iq(p+p')^\mu.

The quadratic term gives a vertex with two photon fields. Differentiating twice with respect to AμA_\mu and AνA_\nu gives a factor 2ημν2\eta^{\mu\nu}, and the factor of ii from iSintiS_{\mathrm{int}} gives

2iq2ημν.2iq^2\eta^{\mu\nu}.

Show that the on-shell fermion current

Jμ=uˉ(p′)γμu(p)J^\mu=\bar u(p')\gamma^\mu u(p)

obeys

(p′−p)μJμ=0.(p'-p)_\mu J^\mu=0.
Solution

Let k=p′−pk=p'-p. Then

kμJμ=uˉ(p′)γ⋅(p′−p)u(p)=uˉ(p′)γ⋅p′ u(p)−uˉ(p′)γ⋅p u(p).k_\mu J^\mu =\bar u(p')\gamma\cdot(p'-p)u(p) =\bar u(p')\gamma\cdot p'\,u(p)-\bar u(p')\gamma\cdot p\,u(p).

The Dirac equations are

(γ⋅p−m)u(p)=0,uˉ(p′)(γ⋅p′−m)=0.(\gamma\cdot p-m)u(p)=0, \qquad \bar u(p')(\gamma\cdot p'-m)=0.

Therefore

uˉ(p′)γ⋅p′=muˉ(p′),γ⋅p u(p)=mu(p).\bar u(p')\gamma\cdot p'=m\bar u(p'), \qquad \gamma\cdot p\,u(p)=m u(p).

Substituting,

kμJμ=muˉ(p′)u(p)−muˉ(p′)u(p)=0.k_\mu J^\mu =m\bar u(p')u(p)-m\bar u(p')u(p)=0.

This is the tree-level Ward identity for a photon attached to an external on-shell fermion line.

Using the trace identities in the text, prove that

Tr⁡[(γ⋅p′+m)γμ(γ⋅p+m)γρ]=4[p′μpρ+p′ρpμ−ημρ(p′⋅p−m2)].\operatorname{Tr}\left[(\gamma\cdot p'+m)\gamma^\mu(\gamma\cdot p+m)\gamma^\rho\right] =4\left[p'^\mu p^\rho+p'^\rho p^\mu -\eta^{\mu\rho}(p'\cdot p-m^2)\right].
Solution

Expand the trace:

Tr⁡[(γ⋅p′+m)γμ(γ⋅p+m)γρ]=pα′pβTr⁡(γαγμγβγρ)+m2Tr⁡(γμγρ),\operatorname{Tr}\left[(\gamma\cdot p'+m)\gamma^\mu(\gamma\cdot p+m)\gamma^\rho\right] = p'_\alpha p_\beta \operatorname{Tr}(\gamma^\alpha\gamma^\mu\gamma^\beta\gamma^\rho) +m^2\operatorname{Tr}(\gamma^\mu\gamma^\rho),

because the terms with three gamma matrices have zero trace. Now use

Tr⁡(γαγμγβγρ)=4(ηαμηβρ−ηαβημρ+ηαρημβ)\operatorname{Tr}(\gamma^\alpha\gamma^\mu\gamma^\beta\gamma^\rho) =4\left(\eta^{\alpha\mu}\eta^{\beta\rho} -\eta^{\alpha\beta}\eta^{\mu\rho} +\eta^{\alpha\rho}\eta^{\mu\beta}\right)

and

Tr⁡(γμγρ)=4ημρ.\operatorname{Tr}(\gamma^\mu\gamma^\rho)=4\eta^{\mu\rho}.

Therefore

pα′pβTr⁡(γαγμγβγρ)=4(p′μpρ−(p′⋅p)ημρ+p′ρpμ),p'_\alpha p_\beta \operatorname{Tr}(\gamma^\alpha\gamma^\mu\gamma^\beta\gamma^\rho) =4\left(p'^\mu p^\rho-(p'\cdot p)\eta^{\mu\rho}+p'^\rho p^\mu\right),

and the mass term adds 4m2ημρ4m^2\eta^{\mu\rho}. Combining terms gives

4[p′μpρ+p′ρpμ−ημρ(p′⋅p−m2)].4\left[p'^\mu p^\rho+p'^\rho p^\mu -\eta^{\mu\rho}(p'\cdot p-m^2)\right].

In scalar QED, explain why the seagull graph is required for gauge invariance of scalar Compton scattering. You do not need to compute the full amplitude; show how replacing one polarization vector by its momentum cancels a scalar propagator.

Solution

Consider the part of the ss-channel diagram where the incoming photon of momentum kk attaches to an incoming on-shell scalar of momentum pp. The vertex contains

+iq(2p+k)μεμ.+iq(2p+k)^\mu\varepsilon_\mu.

Replace εμ\varepsilon_\mu by kμk_\mu. Then

k⋅(2p+k)=2p⋅k+k2.k\cdot(2p+k)=2p\cdot k+k^2.

Since the external photon is on shell, k2=0k^2=0, and since the scalar is on shell, p2=m2p^2=m^2. Hence

2p⋅k+k2=(p+k)2−p2=(p+k)2−m2.2p\cdot k+k^2=(p+k)^2-p^2=(p+k)^2-m^2.

This is the inverse of the scalar propagator in that channel. Thus the Ward variation of the exchange diagram collapses the internal scalar propagator and leaves a local term. The corresponding variation of the other exchange diagram leaves another local term. These local remnants are canceled by the variation of the contact diagram from

q2AμAμϕ∗ϕ.q^2A_\mu A^\mu\phi^*\phi.

Therefore the exchange diagrams alone are not gauge invariant; the complete minimal-coupling set is.

Two distinguishable spin-one-half particles of charges q1,q2q_1,q_2 scatter by one-photon exchange. Starting from

M=q1q2Q2[uˉ(p1′)γμu(p1)][uˉ(p2′)γμu(p2)],\mathcal M={q_1q_2\over Q^2} \left[\bar u(p_1')\gamma^\mu u(p_1)\right] \left[\bar u(p_2')\gamma_\mu u(p_2)\right],

write the unpolarized squared amplitude as a product of two traces. Identify the initial-state average.

Solution

There are two spin states for each incoming particle, so the initial-state average is 1/(2⋅2)=1/41/(2\cdot2)=1/4. Summing final spins and using the completeness relations gives

∣M∣2‾=q12q22(Q2)214Tr⁡ ⁣[(γ⋅p1′+m1)γμ(γ⋅p1+m1)γν]×Tr⁡ ⁣[(γ⋅p2′+m2)γμ(γ⋅p2+m2)γν].\begin{aligned} \overline{|\mathcal M|^2} ={q_1^2q_2^2\over(Q^2)^2}{1\over4} &\operatorname{Tr}\!\left[ (\gamma\cdot p_1'+m_1)\gamma^\mu (\gamma\cdot p_1+m_1)\gamma^\nu \right]\\ \times{}&\operatorname{Tr}\!\left[ (\gamma\cdot p_2'+m_2)\gamma_\mu (\gamma\cdot p_2+m_2)\gamma_\nu \right]. \end{aligned}

Equivalently, absorb one factor of 1/21/2 into each current tensor. No average is taken over final spins unless the measurement explicitly prepares an incoherent ensemble of final states; unobserved final spins are summed.

  • Coleman, Sidney. Lectures of Sidney Coleman on Quantum Field Theory. Edited by Bryan Gin-ge Chen, David Derbes, David Griffiths, Brian Hill, Richard Sohn, and Yuan-Sen Ting. World Scientific, 2019. The electrodynamics chapters develop minimal coupling and low-order spinor-QED calculations.
  • Schwartz, Matthew D. Quantum Field Theory and the Standard Model. Cambridge University Press, 2014. The chapters on QED scattering and gauge invariance give detailed tree-amplitude and Ward-identity derivations.
  • Srednicki, Mark. Quantum Field Theory. Cambridge University Press, 2007. The scalar- and spinor-electrodynamics chapters derive the vertices, spin sums, and Ward identities used here.
  • Weinberg, Steven. The Quantum Theory of Fields, Volume I: Foundations. Cambridge University Press, 1995. Chapters 6 and 8 develop scattering rules, electrodynamics, and gauge invariance.
  • Zee, A. Quantum Field Theory in a Nutshell. 2nd ed., Princeton University Press, 2010. The discussions of electron scattering and diagrammatic gauge invariance emphasize the physical Ward checks.

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