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Yang–MillsA QFT.ORG PROJECT

Free massive and massless fields

A free field is a reference experiment in which we can solve the spectral question before asking how interactions change it. It distinguishes a mass put into the model from a mass generated by a gauge theory.

Prerequisites: Gaussian measures and Euclidean correlators.
Outcomes: compute a smeared free correlator; locate its spectral threshold; identify infrared and boundary-condition assumptions.

Consider a real free scalar on four-dimensional Euclidean space, with three spatial directions, ℏ=c=1\hbar=c=1, and mass m>0m>0. This is a scalar Gaussian theory, with no gauge group or gauge constraint. Its momentum covariance is (p02+p2+m2)−1(p_0^2+\mathbf p^2+m^2)^{-1}.

Fourier transforming only Euclidean time gives

Cm(t,p)=∫Rdp02πeip0tp02+ωp2=e−ωp∣t∣2ωp,ωp=p2+m2.C_m(t,\mathbf p) =\int_{\mathbb R}\frac{dp_0}{2\pi} \frac{e^{ip_0t}}{p_0^2+\omega_{\mathbf p}^2} =\frac{e^{-\omega_{\mathbf p}|t|}}{2\omega_{\mathbf p}}, \qquad \omega_{\mathbf p}=\sqrt{\mathbf p^2+m^2}.

The last integral follows by closing the contour in the half-plane where the exponential decays. The poles at ±iωp\pm i\omega_{\mathbf p} yield the positive exponential. Free scalar quantization is developed in Tong’s QFT notes, chapter 2; this calculation fixes the conventions used below.

Choose a real Schwartz spatial smearing ff. For the observable Of(t)=∫d3x f(x)ϕ(t,x)O_f(t)=\int d^3x\,f(\mathbf x)\phi(t,\mathbf x),

⟨Of(t)Of(0)⟩=∫d3p(2π)3∣f~(p)∣2e−ωp∣t∣2ωp.\langle O_f(t)O_f(0)\rangle =\int\frac{d^3p}{(2\pi)^3} |\widetilde f(\mathbf p)|^2 \frac{e^{-\omega_{\mathbf p}|t|}}{2\omega_{\mathbf p}}.

Rapid decrease of f~\widetilde f controls large momenta. The observable has zero vacuum mean, so this is already connected.

The threshold need not be an isolated eigenvalue

Section titled “The threshold need not be an isolated eigenvalue”

Every energy in this integral is at least mm. Therefore, for t≥0t\geq0,

0≤Cf(t)≤e−mtCf(0).0\leq C_f(t)\leq e^{-mt}C_f(0).

If f~\widetilde f does not vanish near p=0\mathbf p=0, the spectral measure reaches energies arbitrarily near mm. On infinite space the momentum eigenvectors are not normalizable, so a threshold at mm need not be an isolated Hilbert-space eigenvector. A power multiplying e−mte^{-mt} in a position-space correlator is consistent with a positive threshold.

For the free scalar Fock space, nonvacuum states contain one or more quanta, so their total energy is at least mm. A nonlinear probe can still miss the one-particle sector. Use the already spatially smeared variable above to define Yf(t)=Of(t)2−⟨Of2⟩Y_f(t)=O_f(t)^2-\langle O_f^2\rangle. Gaussian pairing gives

⟨Yf(t)Yf(0)⟩=2Cf(t)2.\langle Y_f(t)Y_f(0)\rangle=2C_f(t)^2.

When f~\widetilde f has support arbitrarily near zero momentum, the two-particle spectral support of this correlator begins at 2m2m. This example squares one well-defined smeared variable; it does not assume a pointwise Euclidean Wick square exists in four dimensions. A channel threshold and the theory’s gap are different objects.

Setting the mass to zero changes the infrared question

Section titled “Setting the mass to zero changes the infrared question”

For the massless scalar in four Euclidean dimensions the covariance 1/p21/p^2 is locally integrable near p=0p=0: the radial measure gives p3dp/p2=p dpp^3dp/p^2=p\,dp. Smeared fields can be defined, and one-particle energies ∣p∣|\mathbf p| approach zero. The infinite-volume theory is gapless.

This statement is dimension dependent. In two Euclidean dimensions, the same infrared integral behaves as dp/pdp/p and diverges for generic test functions with nonzero Fourier transform at zero. A massless scalar there requires a restricted observable class or a treatment of the additive zero mode. One cannot erase this distinction by declaring all free Gaussian fields identical.

On a spatial interval with Dirichlet boundaries, the mode energies are

En(L)=m2+(nπ/L)2,n≥1.E_n(L)=\sqrt{m^2+(n\pi/L)^2},\qquad n\geq1.

For m=0m=0, the first mode is positive at each finite LL but tends to zero as LL grows. For m>0m>0, it tends to mm. Periodic boundaries instead allow a spatial zero mode. At m=0m=0 that mode is not a positive-frequency oscillator; it must be handled separately.

These are exact free-mode statements for the specified boundaries. They are not numerical measurements of a Yang–Mills glueball.

A free scalar has mass m=1m=1 in chosen physical units. A probe couples only to two-particle states with total zero momentum. Its measured long-time decay begins at energy 2. Does the underlying theory have gap 2?

Solution. No. One-particle wave packets have energy arbitrarily near 1, so the nonvacuum spectrum starts there. The selected probe misses that sector. The threshold 2 describes its channel. Changing the probe does not change the Hamiltonian.

The mass parameter was supplied in the covariance. There is no non-Abelian gauge interaction and no dynamical demonstration of dimensional transmutation. The official Yang–Mills target, §§4–5 cannot be satisfied by substituting this free scalar.

Use this example in the gap-and-decay page, operator overlap, and the finite-volume lab. The model is valuable because every assumption can be inspected.