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Momentum-Space Correlators and Conformal Ward Identities

Fourier transformation turns conformal Ward identities into differential equations in momenta, but it does not erase distributions supported at coincident points. A correct momentum-space solution therefore specifies its Fourier convention, keeps the overall momentum delta function distinct from the reduced correlator, solves the nonlocal equations, and restores every semilocal, contact, counterterm, and anomaly contribution allowed by the Ward identities. The discussion is Euclidean in general dimension dd; Lorentzian correlators require a stated boundary-value prescription and have different branch cuts.

Required background. Scalar Two- and Three-Point Functions supplies the separated-point position-space correlators. Tempered Distributions and Fourier Calculus supplies distributional Fourier transformation. Helpful background. Fourier Series, Fourier Transforms, and Plancherel Theory fixes the ordinary transform machinery. Contact Terms, Equal-Time Commutators, and Schwinger Terms explains contact contributions to Ward identities.

Fourier conventions and reduced correlators

Section titled “Fourier conventions and reduced correlators”

Use

O~(p)=ddxeipxO(x),O(x)=ddp(2π)deipxO~(p).\widetilde{\mathcal O}(p) =\int d^d x\,e^{-ip\cdot x}\mathcal O(x), \qquad \mathcal O(x)=\int\frac{d^d p}{(2\pi)^d} e^{ip\cdot x}\widetilde{\mathcal O}(p).

Translation invariance gives

i=1nO~i(pi)=(2π)dδ(d) ⁣(i=1npi) ⁣i=1nOi(pi) ⁣.\left\langle\prod_{i=1}^{n}\widetilde{\mathcal O}_i(p_i)\right\rangle =(2\pi)^d\delta^{(d)}\!\left(\sum_{i=1}^{n}p_i\right) \left\langle\!\left\langle \prod_{i=1}^{n}\mathcal O_i(p_i) \right\rangle\!\right\rangle .

Double brackets mean that the momentum-conserving delta distribution has been removed; they do not mean that other distributions or contact terms have been discarded. Set pn=j=1n1pjp_n=-\sum_{j=1}^{n-1}p_j only after differentiating the full distribution or after deriving the reduced Ward operator consistently.

For scalar primaries of dimensions Δi\Delta_i, the homogeneous reduced dilatation equation is

[j=1n1pjμpjμ(i=1nΔi(n1)d)] ⁣O1On ⁣=0.\left[ \sum_{j=1}^{n-1}p_j^\mu\frac{\partial}{\partial p_j^\mu} -\left(\sum_{i=1}^{n}\Delta_i-(n-1)d\right) \right] \left\langle\!\left\langle\mathcal O_1\cdots\mathcal O_n \right\rangle\!\right\rangle=0.

The degree iΔi(n1)d\sum_i\Delta_i-(n-1)d includes the d-d carried by the removed delta distribution. After renormalization, the right-hand side may instead be a local anomaly. With the Fourier convention above, the scalar special-conformal generator is

Kjκ=pjκ2pjαpjα2pjα2pjαpjκ+2(Δjd)pjκ,\mathcal K_j^{\kappa} =p_j^{\kappa}\frac{\partial^2}{\partial p_j^\alpha\partial p_{j\alpha}} -2p_j^\alpha \frac{\partial^2}{\partial p_j^\alpha\partial p_{j\kappa}} +2(\Delta_j-d)\frac{\partial}{\partial p_{j\kappa}},

and the reduced homogeneous equation is

j=1n1Kjκ ⁣O1On ⁣=0.\sum_{j=1}^{n-1}\mathcal K_j^{\kappa} \left\langle\!\left\langle\mathcal O_1\cdots\mathcal O_n \right\rangle\!\right\rangle=0.

Changing the sign in the Fourier exponential changes intermediate factors of ii but not a consistently transformed final equation. Spinning primaries add the momentum-space Lorentz-generator term acting on their indices. The derivation and the reduction to scalar radial equations are given in Bzowski, McFadden, and Skenderis 2014, §§3–4.

A distributional scalar two-point transform

Section titled “A distributional scalar two-point transform”

The position-space power law has the Euclidean Fourier transform

ddxeipx1(x2)Δ=2d2Δπd/2Γ ⁣(d2Δ)Γ(Δ)(p2)Δd/2.\int d^d x\,e^{-ip\cdot x}\frac1{(x^2)^\Delta} =2^{d-2\Delta}\pi^{d/2} \frac{\Gamma\!\left(\frac d2-\Delta\right)}{\Gamma(\Delta)} (p^2)^{\Delta-d/2}.

This formula is first defined as a Riesz distribution for 0<ReΔ<d/20<\operatorname{Re}\Delta<d/2 and nonzero Euclidean pp, with the endpoints and the rest of the Δ\Delta-plane reached by analytic continuation. It is not an absolutely convergent ordinary integral on all of Rd\mathbb R^d.

The momentum power has degree 2Δd2\Delta-d, exactly the reduced two-point degree. At

Δ=d2+k,k=0,1,2,,\Delta=\frac d2+k, \qquad k=0,1,2,\ldots,

Γ(d/2Δ)\Gamma(d/2-\Delta) has a pole. After subtracting a local polynomial counterterm, the renormalized nonlocal part is proportional to

(p2)klogp2μ2,(p^2)^k\log\frac{p^2}{\mu^2},

plus a scheme-dependent polynomial in p2p^2. Its scale derivative is local:

μμ[(p2)klogp2μ2]=2(p2)k.\mu\frac{\partial}{\partial\mu} \left[(p^2)^k\log\frac{p^2}{\mu^2}\right] =-2(p^2)^k.

Thus a logarithm and a local scale anomaly are two descriptions of the same renormalized distribution. Deleting the polynomial terms before applying the Ward identity can erase precisely the anomaly one wants to determine.

Scalar three-point functions and triple-K integrals

Section titled “Scalar three-point functions and triple-K integrals”

Rotational invariance makes a scalar reduced three-point function depend on the magnitudes pi=pi2p_i=\sqrt{p_i^2}. Away from exceptional momentum configurations, the special-conformal equations reduce to

(KiKj) ⁣O1(p1)O2(p2)O3(p3) ⁣=0,(K_i-K_j)\left\langle\!\left\langle \mathcal O_1(p_1)\mathcal O_2(p_2)\mathcal O_3(p_3) \right\rangle\!\right\rangle=0,

where

Ki=2pi2+d+12Δipipi.K_i=\frac{\partial^2}{\partial p_i^2} +\frac{d+1-2\Delta_i}{p_i}\frac{\partial}{\partial p_i}.

A solution of the homogeneous primary Ward identities is

 ⁣O1O2O3 ⁣=C123Iα{β1β2β3}(p1,p2,p3),\left\langle\!\left\langle \mathcal O_1\mathcal O_2\mathcal O_3 \right\rangle\!\right\rangle =C_{123}\,I_{\alpha\{\beta_1\beta_2\beta_3\}}(p_1,p_2,p_3),

with

Iα{β1β2β3}=0dxxαi=13piβiKβi(pix),α=d21,βi=Δid2.\begin{aligned} I_{\alpha\{\beta_1\beta_2\beta_3\}} &=\int_0^\infty dx\,x^\alpha \prod_{i=1}^{3}p_i^{\beta_i}K_{\beta_i}(p_i x),\\ \alpha&=\frac d2-1, \qquad \beta_i=\Delta_i-\frac d2. \end{aligned}

Here KνK_\nu is the modified Bessel function, not the conformal generator. The Bessel equation proves (KiKj)I=0(K_i-K_j)I=0. Rescaling every momentum by λ\lambda and then xx/λx\mapsto x/\lambda gives

I(λp1,λp2,λp3)=λΔ1+Δ2+Δ32dI(p1,p2,p3),I(\lambda p_1,\lambda p_2,\lambda p_3) =\lambda^{\Delta_1+\Delta_2+\Delta_3-2d}I(p_1,p_2,p_3),

which matches the reduced dilatation equation and the Fourier transform of the position-space three-point function. This representation, including convergence and renormalization, is derived in Bzowski, McFadden, and Skenderis 2014, §§4.1–4.2.

The integral is singular when, for some independent choices σi{+1,1}\sigma_i\in\{+1,-1\} and some integer k0k\geq0,

α+1+σ1β1+σ2β2+σ3β3=2k.\alpha+1+\sigma_1\beta_1+\sigma_2\beta_2+\sigma_3\beta_3=-2k.

One then regulates dd and the Δi\Delta_i in a symmetry-compatible way, expands the integral, adds local counterterms, and takes the regulator to zero. Different sign patterns encode different endpoint singularities and support types; they must not all be interpreted as an ordinary ultraviolet divergence. At special dimensions, the renormalized answer can contain logarithms and inhomogeneous conformal Ward identities. The systematic current and stress-tensor treatment appears in Bzowski, McFadden, and Skenderis 2018, §§2–4.

Tensor decomposition must retain longitudinal terms

Section titled “Tensor decomposition must retain longitudinal terms”

For a current or stress tensor, rotations permit a transverse decomposition using, for p20p^2\neq0,

πμν(p)=δμνpμpνp2.\pi_{\mu\nu}(p)=\delta_{\mu\nu}-\frac{p_\mu p_\nu}{p^2}.

The transverse form factors satisfy the primary conformal equations, while longitudinal and trace pieces are fixed by conservation and trace Ward identities. But a current insertion generally obeys

pμ ⁣Jμ(p)O1(p1)On(pn) ⁣=contact terms from the transformations of the insertions,p^\mu\left\langle\!\left\langle J_\mu(p) \mathcal O_1(p_1)\cdots\mathcal O_n(p_n) \right\rangle\!\right\rangle =\text{contact terms from the transformations of the insertions},

not zero. Projecting every leg transversely before recording this equation loses those terms. A safe order is: derive the full distributional Ward identities, solve their longitudinal and trace parts, decompose the remaining transverse tensor, and only then solve its form-factor equations.

At p2=0p^2=0, at zero momentum, or on collinear boundaries of the Euclidean momentum triangle, πμν\pi_{\mu\nu} or a chosen tensor basis becomes singular or loses rank. Statements derived for generic momenta require a separate distributional limit there. In Lorentzian signature the continuation of (p2)ν(p^2)^\nu and the triple-K representation depends on whether the target is Wightman, time-ordered, retarded, or another correlator; an i0i0 prescription and sheet must be specified.

Position-space support determines what may be changed without altering a separated-point correlator.

Momentum-space termPosition-space supportWhat fixes it
Polynomial in all external momentaAll insertions coincident (ultralocal)Local counterterms and scheme choice
Polynomial in one momentum times a nonanalytic lower-point functionA proper subset of insertions coincident (semilocal)Ward identities and lower-point normalization
Nonanalytic dependence on all independent invariantsSeparated points (nonlocal)CFT three-point data and boundary conditions
Scale derivative of a logarithmic termLocal or semilocal anomalyCounterterm residue and consistency conditions

Tensor decompositions can make an anomaly appear as a factor such as 1/p21/p^2 in an individual form factor. Such an anomaly pole can be forced by a local Ward identity because the tensor basis itself contains powers of momentum. Its residue and allowed contact terms are meaningful; the pole alone does not establish a propagating massless particle. One must reconstruct the full correlator and examine its spectral and Lorentzian boundary conditions before making that interpretation.

The position–momentum match is therefore threefold: the nonlocal momentum dependence must transform back to the separated-point power law; polynomial ambiguities must transform to derivatives of delta functions; and scale or conformal anomalies must match the variation of local counterterms. Agreement of only the homogeneity degree is necessary but not sufficient.

Derive the scaling degree of Iα{β1β2β3}I_{\alpha\{\beta_1\beta_2\beta_3\}} directly and specialize to the conformal values of α\alpha and βi\beta_i.

Solution

Under piλpip_i\mapsto\lambda p_i, set y=λxy=\lambda x. The three factors piβip_i^{\beta_i} contribute λiβi\lambda^{\sum_i\beta_i}, while dxxαdx\,x^\alpha contributes λα1\lambda^{-\alpha-1}. Hence I(λpi)=λiβiα1I(pi)I(\lambda p_i)=\lambda^{\sum_i\beta_i-\alpha-1}I(p_i). With βi=Δid/2\beta_i=\Delta_i-d/2 and α=d/21\alpha=d/2-1, the exponent is iΔi2d\sum_i\Delta_i-2d, exactly the degree of a reduced three-point function.

For separated Euclidean points, Scalar Two- and Three-Point Functions gives the position-space answer that the nonlocal terms must reproduce. For four-point spectral decompositions and crossing, return to Crossing Equations and Positivity; contact and anomaly polynomials are not additional exchanged conformal blocks.

  • Bzowski, A., McFadden, P., and Skenderis, K. (2014). “Implications of Conformal Invariance in Momentum Space.” Journal of High Energy Physics 03 (2014), 111. doi:10.1007/JHEP03(2014)111. Open version.
  • Bzowski, A., McFadden, P., and Skenderis, K. (2018). “Renormalised CFT 3-point Functions of Scalars, Currents and Stress Tensors.” Journal of High Energy Physics 11 (2018), 159. doi:10.1007/JHEP11(2018)159. Open version.