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Derivative Interactions and Contact Terms

A derivative acting on a field contributes ipμ-ip_\mu when that field carries incoming momentum pp in the site Fourier convention. The vertex is obtained by differentiating the written action with respect to its fields, so identical-field multiplicities and the placement of derivatives must be handled before simplifying with momentum conservation. Integration by parts gives equivalent integrated actions under controlled boundary conditions, but derivatives of time-ordered products can also create local delta-function contact terms. In particular, a Hamiltonian interaction containing time derivatives cannot always be replaced blindly by Lint-\mathcal L_{\mathrm{int}}.

Required background. Momentum-Space Feynman Rules fixes the all-momenta-incoming and Fourier conventions.

Helpful background. Coincident Products and Contact Terms explains why local products need a distributional definition; Local versus Integrated Operator Redundancies separates equality after integration from equality of local insertions.

Momentum factors from declared derivatives

Section titled “Momentum factors from declared derivatives”

For

ϕ(x)=ddp(2π)deipxϕ~(p),\phi(x)=\int\frac{\mathrm d^d p}{(2\pi)^d} e^{-ip\cdot x}\widetilde\phi(p),

one has

μϕ(x)ipμϕ~(p).\partial_\mu\phi(x) \longmapsto -ip_\mu\widetilde\phi(p).

Consider two real fields with

Lint=g2χμϕμϕ.\mathcal L_{\mathrm{int}} =-\frac g2\chi\,\partial_\mu\phi\,\partial^\mu\phi.

Let p1,p2p_1,p_2 be the momenta on the two identical ϕ\phi legs and p3p_3 the momentum on χ\chi, all incoming. The two derivatives give (ip1)μ(ip2)μ=p1p2(-ip_1)_\mu(-ip_2)^\mu=-p_1\cdot p_2; multiplication by the g/2-g/2 in the density and by ii from eiSe^{iS} gives igp1p2/2igp_1\cdot p_2/2. The two attachments of the identical ϕ\phi fields cancel the 1/21/2, leaving

Vχϕϕ(p3,p1,p2)=igp1p2,p1+p2+p3=0.\boxed{ V_{\chi\phi\phi}(p_3,p_1,p_2) =ig\,p_1\cdot p_2 }, \qquad p_1+p_2+p_3=0.

The result is symmetric under p1p2p_1\leftrightarrow p_2, as it must be. Its mass dimension also matches the original local operator: the two momenta supply the two derivative dimensions.

The same map appears in the chapter’s action-to-rule figure. Here the important row is the derivative branch and its explicit identical-field check.

The action-to-rule map sends a derivative on a named field to minus i times that field's incoming momentum, while identical attachments cancel only factorials actually present in the action.

Derivative vertices are obtained from the written action before momentum conservation or on-shell identities are used. The displayed χ(ϕ)2\chi(\partial\phi)^2 branch yields igp1p2ig\,p_1\cdot p_2 after the two identical ϕ\phi attachments cancel 1/2!1/2!. Quadratic and polynomial branches are included for comparison. Schematic, not to scale.

Written termIncoming-momentum numeratorCombinatorial check
λϕ4/4!-\lambda\phi^4/4!iλ-i\lambda4!4! identical attachments cancel 4!4!
gχ(ϕ)2/2-g\chi(\partial\phi)^2/2igp1p2ig\,p_1\cdot p_2exchange of the two ϕ\phi legs cancels 2!2!
h(μχ)ϕ1μϕ2-h(\partial_\mu\chi)\phi_1\partial^\mu\phi_2ihpχp2ih\,p_\chi\cdot p_2for distinct ϕ1,ϕ2\phi_1,\phi_2, the derivative belongs only to the ϕ2\phi_2 leg
μKμ(ϕi,ϕi,)\partial_\mu K^\mu(\phi_i,\partial\phi_i,\ldots)vertex proportional to (jpj)μK~μ(\sum_jp_j)_\mu\widetilde K^\muvanishes at a momentum-conserving integrated vertex under the stated boundary assumptions

Integration by parts and total derivatives

Section titled “Integration by parts and total derivatives”

Up to a boundary term,

ddxχ(ϕ)2=ddx[ϕμχμϕ+χϕϕ].\int\mathrm d^d x\, \chi(\partial\phi)^2 =-\int\mathrm d^d x\, \left[ \phi\,\partial_\mu\chi\,\partial^\mu\phi +\chi\phi\,\Box\phi \right].

The two forms give the same integrated vertex once all terms are retained and momentum conservation is used. More generally, for P=jpjP=\sum_jp_j, a scalar total-divergence interaction μKμ(ϕi,ϕi,)\partial_\mu K^\mu(\phi_i,\partial\phi_i,\ldots) transforms as

μKμiPμK~μ,VK=PμK~μ,\partial_\mu K^\mu \longmapsto-iP_\mu\widetilde K^\mu, \qquad V_{\partial K} =P_\mu\widetilde K^\mu,

where the second expression includes the factor ii from eiSe^{iS} and any couplings or derivative numerators are contained in K~μ\widetilde K^\mu. The vertex vanishes against δ(d)(P)\delta^{(d)}(P). Schwartz demonstrates this momentum-conservation check for total derivatives in perturbative matrix elements Schwartz 2014, § 7.4, p. 100.

The conclusion has limits. It assumes the boundary term vanishes or is canceled, and it concerns the integrated perturbative vertex. A local operator and that operator plus a total derivative are not pointwise identical. Boundaries, defects, operator insertions carrying momentum, and topological sectors can make the discarded term consequential.

Equations of motion require similar care. Replacing ϕ\Box\phi by m2ϕ-m^2\phi is valid only in an appropriate on-shell matrix element or after a controlled field redefinition. It is not an algebraic identity inside an off-shell correlator: acting the inverse kinetic operator on a time-ordered propagator produces a contact distribution.

For the canonical scalar, equal-time commutation gives

[ϕ˙(t,x),ϕ(t,y)]=iδ(d1)(xy).[\dot\phi(t,\mathbf x),\phi(t,\mathbf y)] =-i\delta^{(d-1)}(\mathbf x-\mathbf y).

Differentiating a time-ordered product twice therefore yields

x020T{ϕ(x)ϕ(y)}0=0T{x02ϕ(x)ϕ(y)}0iδ(d)(xy).\partial_{x^0}^2 \langle0|\mathrm T\{\phi(x)\phi(y)\}|0\rangle = \langle0|\mathrm T\{\partial_{x^0}^2\phi(x)\phi(y)\}|0\rangle -i\delta^{(d)}(x-y).

Combining spatial derivatives and the free equation of motion gives the distributional inverse relation

(x+m2)DF(xy)=iδ(d)(xy).(\Box_x+m^2)D_F(x-y) =-i\delta^{(d)}(x-y).

The delta term is not an optional correction: it is what makes DFD_F the inverse of the kinetic operator with the declared normalization. Consequently, moving derivatives through T\mathrm T or using the equations of motion inside a correlator can create local contact contributions.

Why time-derivative interactions need special care

Section titled “Why time-derivative interactions need special care”

For interactions without time derivatives, canonical momenta are unchanged and Hint=LintH_{\mathrm{int}}=-L_{\mathrm{int}}. With time derivatives, the relation between velocities and canonical momenta changes; the Legendre transform can generate additional interaction terms. An operator derivation must include them, together with contact terms from differentiated time ordering.

A one-field toy model makes the issue explicit. If the time-derivative part of the Lagrangian is

Ltime=12(1+gϕ)ϕ˙,2,\mathcal L_{\mathrm{time}} =\frac12(1+g\phi)\dot\phi^{,2},

then π=(1+gϕ)ϕ˙\pi=(1+g\phi)\dot\phi and the corresponding Hamiltonian term is

Htime=π22(1+gϕ)=12π2g2ϕπ2+g22ϕ2π2+O(g3).\mathcal H_{\mathrm{time}} =\frac{\pi^2}{2(1+g\phi)} =\frac12\pi^2-\frac g2\phi\pi^2 +\frac{g^2}{2}\phi^2\pi^2+O(g^3).

The first interaction term agrees with Lint-\mathcal L_{\mathrm{int}} only after the lowest-order relation π=ϕ˙\pi=\dot\phi is used, and the order-g2g^2 contact interaction has no counterpart in that naive replacement. In a covariant Lagrangian calculation, differentiated time ordering and the momentum-integration measure reorganize the same local information.

The Lagrangian path integral often repackages these contributions into covariant rules, but only after the momentum variables and any field-dependent measure have been handled correctly. Weinberg derives the Lagrangian path integral from the Hamiltonian and states the conditions under which the ordinary Lagrangian appears Weinberg 1995, § 9.3, pp. 389–394; his subsequent rule derivation shows how differentiated contractions give momentum numerators Weinberg 1995, § 9.4, pp. 395–398. Srednicki gives an explicit warning that time derivatives require a conjugate-momentum source in the operator treatment Srednicki 2007, § 9, p. 82.

Thus the safe procedure is not “replace every derivative by momentum” in isolation. It is:

  1. declare whether the derivation is canonical or Lagrangian;
  2. derive canonical momenta if time derivatives occur;
  3. keep the contact terms implied by ordered distributions;
  4. include the measure or determinant produced when momenta are integrated out; and
  5. compare a simple correlator or amplitude between the two formulations.

A local monomial such as cϕ2χ2/4-c\phi^2\chi^2/4 produces a four-leg contact vertex even though it contains no propagator. Derivative contact vertices are equally local: their polynomial momentum numerator does not turn them into exchange diagrams. Conversely, canceling a propagator denominator with a factor such as p2m2p^2-m^2 can collapse part of a graph to a contact distribution. The distinction is analytic: a genuine exchange contribution has an uncanceled propagator pole, while a contact term is polynomial in momenta at that stage.

This diagnostic is useful under integration by parts and field redefinitions. Different action representatives can redistribute polynomial contact pieces and exchange numerators while leaving a properly defined on-shell amplitude unchanged. Off-shell Green functions need not be identical.

Assigning the derivative momentum to the wrong leg. A derivative acts on its named field. Momentum conservation may rewrite the result only after the unsimplified vertex has been derived.

Using equations of motion inside a time-ordered product without contact terms. The inverse kinetic operator acting on DFD_F yields iδ(d)-i\delta^{(d)}, not zero.

Assuming Hint=LintH_{\mathrm{int}}=-L_{\mathrm{int}} with time derivatives. The canonical momentum and Legendre transform change. Derive them or use a justified Lagrangian path-integral formulation.

Derive the χϕϕ\chi\phi\phi vertex above, integrate the interaction by parts, and derive it again without imposing on-shell equations.

Solution

The original term gives igp1p2igp_1\cdot p_2. After integration by parts, differentiate which of the two identical ϕ\phi fields occupies each slot. The term +(g/2)ϕμχμϕ+(g/2)\phi\,\partial_\mu\chi\,\partial^\mu\phi contributes

ig2p3(p1+p2),-\frac{ig}{2}\,p_3\cdot(p_1+p_2),

while +(g/2)χϕϕ+(g/2)\chi\phi\Box\phi contributes

ig2(p12+p22).-\frac{ig}{2}(p_1^2+p_2^2).

Using p3=(p1+p2)p_3=-(p_1+p_2), their sum is

ig2[(p1+p2)2p12p22]=igp1p2,\frac{ig}{2}\big[(p_1+p_2)^2-p_1^2-p_2^2\big] =igp_1\cdot p_2,

with no use of pi2=mi2p_i^2=m_i^2.

  • Schwartz, Matthew D. Quantum Field Theory and the Standard Model. Cambridge: Cambridge University Press, 2014. DOI.
  • Srednicki, Mark. Quantum Field Theory. Cambridge: Cambridge University Press, 2007. DOI.
  • Weinberg, Steven. The Quantum Theory of Fields, Volume I: Foundations. Cambridge: Cambridge University Press, 1995. First edition; 2005 paperback, 2012 printing consulted. DOI.