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Relational and Gauge-Invariant Gravitational Observables

A coordinate value such as h00(t,x)h_{00}(t,\boldsymbol x) is not a gravitational observable until the event, frame, and measuring apparatus are specified without relying on the gauge labels being tested. Perturbative relational observables do this by using dynamical clock and rod fields, asymptotic structures, or invariantly defined geometric events. Their construction is order dependent and must be transformed together with the EFT field basis.

Required background. Background-Field Quantization, Gauge Fixing, and Ghosts supplies gauge transformations; Gauge-Invariant Response Kernels supplies invariant linear response; and Local Covariance, Isometries, and Background Embeddings supplies the local-covariant setting.

Helpful background. Gauge, BRST, and BV Interfaces on Curved Backgrounds supplies the interacting gauge complex, while Matching Amplitudes to Background Observables supplies the field-basis dictionary.

Let four scalar matter fields XAX^A, A=0,1,2,3A=0,1,2,3, have background values X0A(x)X_0^A(x) with nonsingular Jacobian in a region:

JAμ=μX0A,eAμJBμ=δAB.J^A{}_\mu=\partial_\mu X_0^A, \qquad e_A{}^\mu J^B{}_\mu=\delta_A{}^B.

Write XA=X0A+κχAX^A=X_0^A+\kappa\chi^A and a scalar geometric quantity A=A0+κδA\mathcal A=\mathcal A_0+\kappa\,\delta\mathcal A, where κ\kappa is a perturbative bookkeeper. The event xμ(X)x^\mu(X) is defined by inverting the four reference fields. To first order,

xμ(X)=x0μ(X)κeAμχA,x^\mu(X) =x_0^\mu(X)-\kappa e_A{}^\mu\chi^A,

so the relational perturbation at fixed reference values is

δArel(X)=δAχAeAμμA0.\delta\mathcal A_{\mathrm{rel}}(X) =\delta\mathcal A -\chi^A e_A{}^\mu\partial_\mu\mathcal A_0.

Choose the active gauge convention

δξ(δA)=ξμμA0,δξχA=ξμμX0A.\delta_\xi(\delta\mathcal A) =\xi^\mu\partial_\mu\mathcal A_0, \qquad \delta_\xi\chi^A =\xi^\mu\partial_\mu X_0^A.

The two terms in δArel\delta\mathcal A_{\mathrm{rel}} then cancel exactly. This proof also exposes the domain: the reference-field Jacobian must be invertible, the same gauge sign must be used throughout, and the construction is valid only through the retained perturbative order. Dittrich develops complete observables from clock variables in Dittrich 2006, §§3–5, pp. 6162–6177.

One clock XX and a chosen flow KμK^\mu would give

δAX=δAδXKμμX0KννA0.\delta\mathcal A_X =\delta\mathcal A -\frac{\delta X}{K^\mu\nabla_\mu X_0} K^\nu\nabla_\nu\mathcal A_0.

That expression is invariant only against gauge displacements along KμK^\mu, or under an explicit gradient-alignment restriction. A generic spacetime diffeomorphism requires enough clock and rod fields to resolve all relevant directions.

The structure map carries a gauge-fixed calculation into this relational completion before making a physical claim.

Four scalar clock and rod fields invert coordinate labels and combine with a curvature perturbation to produce a gauge-invariant relational observable

Reference-field fluctuations shift the event at which a geometric scalar is evaluated, cancelling the gauge shift of the raw perturbation when the reference map is nonsingular. The map is schematic and not to scale.

First application: curvature at a matter-clock event

Section titled “First application: curvature at a matter-clock event”

Take A[g]\mathcal A[g] to be a curvature scalar or a tidal scalar formed from the Riemann tensor and a matter-defined tetrad. Compute its renormalized one-loop perturbation in two metric gauges:

δA(2)=δA(1)+LξA0,χ(2)A=χ(1)A+LξX0A.\delta\mathcal A^{(2)} =\delta\mathcal A^{(1)} +\mathcal L_\xi\mathcal A_0, \qquad \chi_{(2)}^A =\chi_{(1)}^A +\mathcal L_\xi X_0^A.

Substitution gives

δArel(2)δArel(1)=ξμμA0ξμμX0AeAννA0=0.\delta\mathcal A_{\mathrm{rel}}^{(2)} -\delta\mathcal A_{\mathrm{rel}}^{(1)} =\xi^\mu\partial_\mu\mathcal A_0 -\xi^\mu\partial_\mu X_0^A e_A{}^\nu\partial_\nu\mathcal A_0 =0.

This is more than an algebraic cancellation. The clock and rod two-point functions, their counterterms, and correlations with the metric must be included at the same loop order. Treating XAX^A as labels in one gauge but as fluctuating matter in another changes the experiment.

Now perform a local metric redefinition,

gμν=gμν+aRμν+bRgμν.g_{\mu\nu}'=g_{\mu\nu} +aR_{\mu\nu}+bRg_{\mu\nu}.

The coordinate expression for A[g]\mathcal A[g], the action of the reference fields, and contact terms all change. Define the primed observable by matching the same apparatus response, not by simply replacing gg with gg' in one formula. The two descriptions then agree through the matched EFT order; an unmatched raw curvature component need not. In locally covariant perturbative gravity, scalar reference fields provide a concrete way to build such diffeomorphism-invariant functionals Brunetti, Fredenhagen, and Rejzner 2016, §§3–4, pp. 752–768.

In asymptotically flat settings, scattering amplitudes and asymptotic charges can be invariant outputs once their dressing, boundary conditions, and infrared prescription are specified. On a background with distinguished worldlines, clock ratios, radar distance, geodesic deviation, and tetrad-projected curvature are operational alternatives. None licenses a strictly local gauge-invariant metric operator at an arbitrary coordinate point.

Relational observables are not automatically ultraviolet finite. Coincident composite fields still require renormalization, and the reference fields introduce their own fluctuations and possible degeneracies. Nor are they globally complete: caustics or repeated clock values can make X01X_0^{-1} multivalued.

Compute h00(x)h_{00}(x) in two gauges at the same numerical coordinate xx. Agreement can be accidental and disagreement can be pure gauge; neither has invariant meaning because the two labels need not denote the same physical event. Repeating the comparison at fixed XAX^A and in the transported matter frame is decisive. Any remaining gauge dependence must be smaller than the declared truncation error or signals an incomplete gauge, counterterm, or reference-field calculation.

The chapter comparison table requires the gauge convention, reference fields or boundary dressing, invertibility domain, renormalization prescription, field basis, perturbative order, and measured output. A nonperturbative algebra of quantum-gravitational observables and holographic reconstruction lie outside this page.

The failure map highlights singular clock maps and comparisons at fixed coordinate rather than fixed event.

Comparing metric components at the same coordinate across gauges fails, while evaluation at the same matter-defined event cancels the gauge displacement

Gauge invariance requires the event and frame to transform with the fields; a singular reference map or an untransformed observable dictionary invalidates the comparison. The map is schematic and not to scale.

  • Brunetti, R., K. Fredenhagen, and K. Rejzner. “Quantum Gravity from the Point of View of Locally Covariant Quantum Field Theory.” Communications in Mathematical Physics 345, 741–779 (2016). doi:10.1007/s00220-016-2676-x. Open PDF
  • Dittrich, B. “Partial and Complete Observables for Hamiltonian Constrained Systems.” Classical and Quantum Gravity 23, 6155–6184 (2006). doi:10.1088/0264-9381/23/22/006. Open PDF