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Einstein-Proca theory couples general relativity to a massive vector field governed by the Proca action. Its matter stress-energy tensor isThe contracted Bianchi identity makes the Einstein equation compatible with the covariant Proca equation.

Use natural units and the Minkowski metric $g_{\mu \nu }=\mathrm{diag}(1,-1,-1,-1)$. A massive spin-one particle has three physical particle polarizations, whereas a massless gauge boson has two. Giving a vector a mass must account for this extra longitudinal state while preserving a positive physical state space, controlled high-energy scattering and, if a fundamental perturbative theory is sought, renormalizability.

At the free-field level there is no inconsistency. The Proca actiongives the Proca equation ${\partial }_{\nu }{F}^{\nu \mu }+m^2{A}^{\mu }=0$. Taking its divergence gives $m^2{\partial }_{\mu }{A}^{\mu }=0$, and then $(\square +m^2)A^{\mu }=0$. For $m>0$ the divergence constraint removes one of the four components, leaving three positive-norm physical modes. The time component is constrained, rather than an independent negative-norm propagating oscillator. The mass term does, however, change under $A_{\mu }\mapsto A_{\mu }+{\partial }_{\mu }\omega$, so the ordinary massless gauge invariance is no longer manifest.

The difficulty becomes acute for generic interactions. Inverting the quadratic operator gives the Proca propagatorThe longitudinal part approaches order $1/m^2$ at large momentum, rather than falling as $1/k^2$. Thus the usual ultraviolet power counting deteriorates. There is a parallel external-state problem: for $p^{\mu }=(E,\mathbf{p})$,Longitudinal external legs can generate powers of $E/m$ in a scattering amplitude. These are the high-energy obstruction for a hard vector mass. Conserved Abelian currents can remove dangerous contractions, so one should not conclude that every massive-vector interaction is impossible.

For a massive non-Abelian vector with gauge-like cubic and quartic couplings, cancellations among diagrams remove the largest powers, but without a suitable additional sector longitudinal scattering still grows like $s/v^2$, where $v$ is the symmetry-breaking scale. A partial-wave coefficient is then of order $s/(16\pi v^2)$. Partial-wave unitarity requires its real part to remain bounded, so perturbation theory fails at energies of order the electroweak scale times a modest loop factor, around the TeV scale for electroweak vectors. This is a limit on the perturbative description, not a proof that a low-energy massive-vector effective field theory is inconsistent.

The Higgs mechanism supplies a weakly coupled completion. For an Abelian example, take a complex scalar field withLocally write $\varphi =(v+h)e^{i\chi /v}/\sqrt{2}$. Its gauge-covariant kinetic term becomesThe combination is invariant under $A_{\mu }\mapsto A_{\mu }+{\partial }_{\mu }\omega$, $\chi \mapsto \chi +gv\omega$. In unitary gauge $\chi =0$, it contains $m^2{A}_{\mu }{A}^{\mu }/2$ with $m=gv$, as well as the correlated $hAA$ and $hhAA$ interactions. The two original gauge polarizations and two real scalar components become three massive-vector polarizations and one radial Higgs boson. The would-be Goldstone boson supplies the longitudinal state. This counting explains why the Goldstone theorem for spontaneously broken global symmetries does not imply an extra physical massless particle here. Local gauge symmetry is a redundancy; choosing a Higgs background after gauge fixing does not explicitly break the gauge invariance of the action.

The extra scalar interactions also repair high-energy scattering. By the Goldstone-boson equivalence theorem, the leading longitudinal-vector amplitude can be computed using the would-be Goldstone bosons. For a charged-to-neutral channel in the linear scalar model, the scalar contact and radial-exchange terms giveThis Higgs cancellation in longitudinal vector scattering removes the uncontrolled $s/v^2$ growth. It also shows why a very large scalar self-coupling would itself make perturbation theory unreliable; introducing a scalar is not a license to ignore partial-wave unitarity.

Although the unitary gauge propagator looks like the badly behaved Proca propagator, renormalizability is conveniently established in an R-xi gauge. Using Cartesian scalar fluctuations, the quadratic mixing is $-m{A}_{\mu }{\partial }^{\mu }\chi$. The gauge-fixing term $-(\partial \cdot A+\xi m\chi {)}^2/(2\xi )$ cancels it and givesAt fixed finite $\xi$ this falls as $1/k^2$. The would-be scalar modes and Faddeev-Popov ghosts remain in intermediate calculations. Gauge identities, organized through BRST symmetry, make unphysical states cancel from physical amplitudes and constrain counterterms to the gauge-invariant renormalizable form. With a renormalizable scalar sector and cancellation of gauge anomalies, spontaneously broken gauge theory is renormalizable and unitary on its physical states; the bosonic construction is demonstrated in the original massive Yang-Mills renormalizability proof. The ultraviolet limit and $\xi \to \infty$ limit do not commute, so the unitary-gauge numerator alone is not a valid disproof of this result.

In the Standard Model, a Higgs doublet breaks the manifest electroweak group from $SU(2{)}_L\times U(1{)}_Y$ to $U(1{)}_{\mathrm{em}}$. The scalar kinetic term yieldsThree scalar directions supply the longitudinal polarizations of $W^{\pm }$ and $Z$, while the unbroken electromagnetic generator leaves the photon massless. The radial Higgs boson remains physical.

There is an important Abelian alternative. The Stueckelberg mechanism introduces a scalar with ${\mathcal{L}}_{\mathrm{mass}}=(m{A}_{\mu }-{\partial }_{\mu }\chi {)}^2/2$, invariant under $A\mapsto A+\partial \omega$, $\chi \mapsto \chi +m\omega$. With suitable conserved-current couplings this can describe a renormalizable massive Abelian gauge theory without a radial Higgs particle. A naive non-Abelian analogue involves a nonlinear group-valued scalar and derivative interactions suppressed by inverse powers of the symmetry-breaking scale; it is generally an effective field theory, not a power-counting-renormalizable substitute. Strongly coupled or composite sectors can provide other completions. A free vector mass is consistent; the central problem is obtaining the longitudinal state and its interactions in a theory with controlled ultraviolet behavior and physical unitarity.

There are two closely related objects to distinguish. Inverting the quadratic Proca action gives the usual covariant Proca propagator. After integration by parts, its kernel isThe matrix inverse with the Feynman i-epsilon prescription givesMultiplication by $K^{ab}$ gives $i{\delta }_b^a$ in the distributional limit. The numerator agrees with the polarization sum for a massive vector boson at the poles, but is not a transverse linear projection at arbitrary four-momentum.

For the literal canonical time-ordered product of $A_a$ and $A_b$, the nondynamical component $A_0$ produces the Proca time-ordering contact term. In the chosen time coordinate the full answer isTo see the local term directly, the three physical polarization vectors give ${\sum }_{\lambda }{ϵ}_{\lambda 0}^2=|\mathbf{q}{|}^2/m^2$. The canonical $00$ two-point correlation function therefore has Fourier transformBy contrast, ${\eta }_{00}+q_0^2/m^2=|\mathbf{q}{|}^2/m^2-(q^2+m^2)/m^2$, so the covariant expression contains an additional $i/m^2$. The mixed and spatial components have no additional contact term. ThusIf $T$ is used to mean covariant time ordering, commonly denoted $T^{\ast }$, the conventional answer is instead just ${\Delta }^{\mathrm{cov}}$. Both conventions have the same propagating poles and agree away from coincidence; explicitly separating them respects the printed definition as an ordinary time-ordered product.

For the torsion-free Levi-Civita connection, cyclically summing the displayed coordinate expression and using ${\Gamma }^a{}_{bc}={\Gamma }^a{}_{cb}$ gives the algebraic first Bianchi identityApply the Jacobi identity to three covariant-derivative commutators, or differentiate the coordinate formula in normal coordinates. The third-derivative terms and the derivatives of quadratic connection terms cancel cyclically, giving the differential second Bianchi identityContracting the first and third curvature indices and then contracting once more yieldsor the contracted Bianchi identity

For the metric variation $h_{ab}=\delta g_{ab}$,while the two double-divergence terms in the supplied metric variation of scalar curvature become a boundary term after integration by parts for tensor fields. The Einstein-Hilbert action therefore contributes $G_{ab}+\Lambda g_{ab}$. Varying the Proca action with respect to the metric gives the Proca stress-energy tensor, and the full Einstein-Proca theory equation is

Since $\delta F_{ab}=2{\nabla }_{[a}\delta A_{b]}$, variation with respect to $A_b$ and one integration by parts give the covariant Proca equationTaking its covariant divergence givesbecause the resulting contractions pair the symmetric Ricci tensor with the antisymmetric electromagnetic field tensor. Since $m\ne 0$, the Lorenz constraint in Proca theory follows:Moreover, $F=dA$ and $d^2=0$, so the Electromagnetic Bianchi identity is

Finally, use that identity to differentiate the matter tensor. The result groups naturally asBoth terms vanish by the Proca equation and its Lorenz constraint in Proca theory. Thus ${\nabla }^a{T}_{ab}=0$, exactly as required by the contracted Bianchi identity applied to the Einstein field equations. The vector equation is therefore consistent with the gravitational equation.

The quadratic Proca action isIts momentum-space kinetic operator isInverting it on transverse and longitudinal projectors gives the Proca propagator

Under $A_{\mu }\mapsto A_{\mu }+{\partial }_{\mu }\alpha$, the field strength is unchanged, but the mass term in the Proca action changes bywhich is not generally a total derivative. The mass therefore breaks gauge invariance.

The Euler-Lagrange field equation isTaking its divergence and using the antisymmetry of $F^{\mu \nu }$ gives $m^2{\partial }_{\nu }{A}^{\nu }=0$. Since $m>0$, the Lorenz constraint in Proca theory follows. Substitution back into the field equation then gives

The Proca stress-energy tensor is the metric variation of the matter part of the Proca action. It consists of the electromagnetic stress-energy tensor plus the quadratic mass contribution $m^2(A_a{A}_b-g_{ab}{A}^2/2)$.