Skip to content

Interacting Measures, Stability, and Wick Ordering

An interacting Euclidean measure is obtained by weighting a Gaussian random distribution only when the interaction is defined on that distribution space and its exponential is integrable. Wick ordering removes covariance-dependent self-contractions; stability prevents the weight from running to infinity along large-field directions. Neither condition can be replaced by a formal action.

Required background. Gaussian Euclidean fields as measures fixes the reference law and Wick contractions; the constructive program and cutoff removal separates fixed-cutoff normalization from uniform removal.

Helpful background. Osterwalder–Schrader axioms and reflection positivity explains the positivity that a regulator should preserve; Euclidean growth, regularity, and temperedness supplies the distributional setting.

Wick ordering defines the local polynomial

Section titled “Wick ordering defines the local polynomial”

Let ϕκ\phi_\kappa be a mollified massive Gaussian field in two dimensions and let cκ=E[ϕκ(x)2]c_\kappa=\mathbb E[\phi_\kappa(x)^2], which diverges as the ultraviolet scale κ\kappa\to\infty. The covariance-dependent Wick powers are

: ⁣ϕκ2 ⁣:=ϕκ2cκ,: ⁣ϕκ4 ⁣:=ϕκ46cκϕκ2+3cκ2.:\!\phi_\kappa^2\!:=\phi_\kappa^2-c_\kappa, \qquad :\!\phi_\kappa^4\!:=\phi_\kappa^4-6c_\kappa\phi_\kappa^2+3c_\kappa^2.

Their smeared limits exist as random distributions even though the pointwise powers of ϕ\phi do not. Equivalently, they are Hermite polynomials with the variance fixed by the chosen covariance. Changing the reference covariance changes lower-order terms, so the convention must remain fixed or be accompanied by the corresponding finite counterterm.

On a two-dimensional torus TL2\mathbb T_L^2, the regulated quartic law is

dνL,κ(ϕ)=ZL,κ1exp ⁣[λTL2: ⁣ϕκ4 ⁣:Cdx]dμC(ϕ),λ0.d\nu_{L,\kappa}(\phi)=Z_{L,\kappa}^{-1} \exp\!\left[-\lambda\int_{\mathbb T_L^2}:\!\phi_\kappa^4\!:_C dx\right]d\mu_C(\phi), \qquad \lambda\ge0.

For fixed LL, the Wick polynomial converges in every finite Lp(μC)L^p(\mu_C) needed in the standard construction, and a stability estimate bounds its negative tail strongly enough that the exponential is integrable. Thus the ultraviolet limit defines a normalizable finite-volume λϕ24\lambda\phi^4_2 measure. The classic finite-volume and cutoff-removal mechanism is reviewed in Summers 2016, §3.1, pp. 10–12; the original no-cutoff construction is Glimm and Jaffe 1970, pp. 362–401.

For a general even polynomial P(u)=a2nu2n++a0P(u)=a_{2n}u^{2n}+\cdots+a_0, the decisive large-field hypothesis is a2n>0a_{2n}>0. Wick ordering adds lower-degree, cutoff-dependent terms but does not reverse the positive leading behavior. One seeks a bound of the form

Λ: ⁣P(ϕκ) ⁣:CdxAΛRκ(ϕ),\int_\Lambda :\!P(\phi_\kappa)\!:_C dx \ge -A|\Lambda|-R_\kappa(\phi),

where the remainder is controlled in exponential moments uniformly enough for the intended limit. This licenses 0<ZΛ,κ<0<Z_{\Lambda,\kappa}<\infty and uniform moment estimates. It does not by itself prove an infinite-volume limit, clustering, reflection positivity, or non-Gaussianity; those require further arguments.

For the worked torus example, differentiating the finite-cutoff partition function gives

λlogZL,κ=EνL,κTL2: ⁣ϕκ4 ⁣:Cdx.-\frac{\partial}{\partial\lambda}\log Z_{L,\kappa} =\mathbb E_{\nu_{L,\kappa}}\int_{\mathbb T_L^2}:\!\phi_\kappa^4\!:_C dx.

This identity checks both normalization and the sign of the interaction. Convexity of logZ\log Z follows because its second derivative is the variance of the integrated Wick polynomial. These finite-volume facts survive a limit only under uniform integrability.

The physical status and the precise low-dimensional scope return to rigorous status, construction, and open problems. The theorem constructs a two-dimensional scalar measure; it does not transfer unchanged to d=4d=4, where additional renormalization and the nontrivial continuum-limit problem intervene.

Reverse the sign of the leading coefficient: P(u)=u4P(u)=-u^4. Restricting a finite-dimensional ultraviolet approximation to its constant mode uu makes the density proportional to e+λΛu4e^{+\lambda |\Lambda|u^4} times a Gaussian. The quartic growth dominates the Gaussian decay, so Z=Z=\infty. This failure occurs before any limit.

A less obvious error Wick-orders successive cutoffs with unrelated covariances but keeps the same bare quadratic coefficient. Since

: ⁣ϕ4 ⁣:C=: ⁣ϕ4 ⁣:C6(CC)(0): ⁣ϕ2 ⁣:C+3(CC)(0)2,:\!\phi^4\!:_{C'}=: \!\phi^4\!:_C-6(C'-C)(0):\!\phi^2\!:_C+3(C'-C)(0)^2,

the sequence has silently changed its mass and vacuum-energy counterterms. Apparent convergence can then describe different theories. The independent diagnostic is to translate every approximation to one common Wick convention and verify that the induced lower-order coefficients converge.

The converse also fails: normalizability at each cutoff does not imply a uniform lower bound or a nontrivial continuum measure. A sequence can be perfectly integrable while concentrating at a point or drifting with the regulator.

One should also distinguish vacuum-energy renormalization from observable normalization. Adding a cutoff-dependent constant EκΛE_\kappa|\Lambda| to the action multiplies both the numerator and partition function by the same factor, so normalized correlation functions are unchanged at fixed cutoff. A quadratic counterterm is different: it changes the relative weight of field configurations and hence the two-point function. This gives a practical check on a counterterm calculation. Constants may be fixed by a pressure convention, whereas mass terms must be fixed by a physical or correlation-length condition. Confusing the two can make a finite partition function look correct while sending the renormalized mass to an unintended value. Repeat this comparison after every change of ultraviolet regulator: finite counterterms may change even when the continuum normalization condition does not.

1. Centering check. Show that EμC[: ⁣ϕκ4 ⁣:]=0\mathbb E_{\mu_C}[:\!\phi_\kappa^4\!:]=0 at a fixed point of the regulated field.

Solution

For a centered Gaussian XX of variance cc, EX2=c\mathbb E X^2=c and EX4=3c2\mathbb E X^4=3c^2. Hence 3c26c2+3c2=03c^2-6c^2+3c^2=0.

2. Partition-function convexity. Prove λ2logZL,κ0\partial_\lambda^2\log Z_{L,\kappa}\ge0.

Solution

Let V=: ⁣ϕκ4 ⁣:V=\int:\!\phi_\kappa^4\!: and Z(λ)=EeλVZ(\lambda)=\mathbb E e^{-\lambda V}. Direct differentiation gives (logZ)=Eν[V2]Eν[V]2=Varν(V)0(\log Z)''=\mathbb E_\nu[V^2]-\mathbb E_\nu[V]^2=\operatorname{Var}_\nu(V)\ge0.

  • Glimm, James, and Arthur Jaffe. “A λϕ24\lambda\phi^4_2 Quantum Field Theory Without Cutoffs. II.” Annals of Mathematics 91 (1970): 362–401. DOI.
  • Nelson, Edward. “A Quartic Interaction in Two Dimensions.” In Mathematical Theory of Elementary Particles, 69–73. MIT Press, 1966. Publisher record.
  • Summers, Stephen J. “A Perspective on Constructive Quantum Field Theory.” arXiv:1203.3991, revised 2016. Open PDF.