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Shadow Theory

Geometric Realization of Completed Source Relations Descent, Orbit Spaces, Invariant Relations, and Variational Response in Shadow Theory

Variational realization of completed relations

Jeremy RodgersSection 8 of 12Original PDF ↗Publication DOI ↗

Variational realization of completed relations

We now embed the completed relation data into dynamics. The claim to be established is narrow and precise: an invariant relation-dependent action yields, by functional variation, correctly normalized stress-energy, gauge-current, and matter responses, and nothing is postulated by naming it.

Variational setting

Assumption 7.1 (Well-posed variational problem).

The global configuration satisfies the descent conditions of Theorem 3.4 and lies in Cgeo\mathcal{C}_{\mathrm{geo}}. Furthermore, one of the following holds, and which one is part of the declaration of the model:

  1. all variations δg\delta g, δA\delta A, δΦ\delta\Phi have compact support in the interior of MM; or

  2. boundary values of the fields, and for gravity the induced metric on ∂M\partial M, are held fixed, so that boundary contributions vanish identically; or

  3. the gravitational and gauge actions are supplemented by the boundary terms required for a well-posed variational problem. For gravity this is the Gibbons–Hawking–York term 18πGN∮∂MK ∣h∣  d3y\frac{1}{8\pi G_N}\oint_{\partial M} K\,\sqrt{|h|}\;\mathrm{d}^3y [15, 5], with the appropriate subtraction or counterterms in the asymptotic case; for the gauge sector, whatever boundary term the declared B\mathcal{B} requires.

All functional derivatives below are asserted to exist on the declared domain; where SrelS_{\mathrm{rel}} is nonlocal, this existence is a hypothesis on the model, not a theorem.

Definition 7.2 (Relation-dependent total action).

Let r=(rα)α∈Ar=(r_\alpha)_{\alpha\in A} denote the completed invariant relation coordinates, i.e. the components of eAgeoe_A^{\mathrm{geo}}. Consider Stot[g,A,Φ;r]=SEH[g]+SYM[g,A]+Sm[g,A,Φ]+Srel[g,A,Φ;r],(63) S_{\mathrm{tot}}[g,A,\Phi;r] = S_{\mathrm{EH}}[g] +S_{\mathrm{YM}}[g,A] +S_{\mathrm{m}}[g,A,\Phi] +S_{\mathrm{rel}}[g,A,\Phi;r],\tag{63} with (64)SEH[g]=116πGN∫M(R−2Λ) d ⁣vol⁡g    (+ boundary term under \href),(65)SYM[g,A]=−14gYM2∫M⟨Fμν,Fμν⟩ d ⁣vol⁡g,\begin{aligned} \qquad\text{(64)} S_{\mathrm{EH}}[g] &=\frac{1}{16\pi G_N}\int_M \bigl(R-2\Lambda\bigr)\,\mathrm{d}\!\operatorname{vol}_g \;\;(+\text{ boundary term under \href{#V3}{(V3)}}), \\[0.3em] \qquad\text{(65)} S_{\mathrm{YM}}[g,A] &=-\frac{1}{4g_{\mathrm{YM}}^{2}}\int_M \bigl\langle F_{\mu\nu},F^{\mu\nu}\bigr\rangle\,\mathrm{d}\!\operatorname{vol}_g, \end{aligned} and SmS_{\mathrm{m}} a matter action for Φ\Phi [14]. The functional SrelS_{\mathrm{rel}} carries the model-specific dependence on rr. It may be local, boundary-supported, or nonlocal, provided that

  1. it depends on the relation coordinates through a finite or countable dynamical subfamily Adyn⊆AA_{\mathrm{dyn}}\subseteq A, and its Fréchet derivatives with respect to gμνg^{\mu\nu}, AμA_\mu, and the independent matter components exist on the stated domain and are represented by distributional kernels, as set out in Section 7.2; and

  2. it is invariant under the allowed bundle automorphisms and allowed diffeomorphisms, that is, SrelS_{\mathrm{rel}} is constant on the arrows of Ggeo\mathfrak{G}_{\mathrm{geo}}, exactly as the JαJ_\alpha are (Definition 4.1).

Condition (R2) is what makes SrelS_{\mathrm{rel}} a functional of the physical orbit, and it is what supplies the Ward identities of Section 8. An SrelS_{\mathrm{rel}} that fails to be Ggeo\mathfrak{G}_{\mathrm{geo}}-invariant does not define a geometric realization of a completed relation.

The functional chain rule for relation functionals

Convention 7.3 (Two regimes for rr, and the correct chain rule).

By Convention 2.11, exactly one of the following applies to each component rαr_\alpha, and the model declares which.

(a) rαr_\alpha is a functional of the fields. Paper 3 permits an arbitrary index set AA, and nothing in Sections 5–6 requires more. A differentiable action, however, needs additional analytic structure, and we impose it only where it is used. We therefore require that SrelS_{\mathrm{rel}} depend on the relation coordinates through a distinguished dynamical subfamily Adyn⊆A,Adyn finite or countable,(66) A_{\mathrm{dyn}}\subseteq A, \qquad A_{\mathrm{dyn}} \text{ finite or countable},\tag{66} so that Srel=Srel[g,A,Φ;(rα)α∈Adyn]S_{\mathrm{rel}}=S_{\mathrm{rel}}[g,A,\Phi;(r_\alpha)_{\alpha\in A_{\mathrm{dyn}}}] and ∂Srel/∂rα=0\partial S_{\mathrm{rel}}/\partial r_\alpha=0 for α∉Adyn\alpha\notin A_{\mathrm{dyn}}. When AdynA_{\mathrm{dyn}} is countably infinite we require in addition that the derivative series in (68) below converge unconditionally in the distributional-dual topology of the relevant space of kernels; when AdynA_{\mathrm{dyn}} is finite this is vacuous. The remaining relation coordinates, indexed by A∖AdynA\setminus A_{\mathrm{dyn}}, continue to serve as completion coordinates in the sense of Sections 5–6; they simply do not enter the action.

Now suppose rα=rα[g,A,Φ]r_\alpha=r_\alpha[g,A,\Phi], α∈Adyn\alpha\in A_{\mathrm{dyn}}, takes values in a Banach (or finite-dimensional) space VαV_\alpha and is Fréchet differentiable on the declared domain. Then rαr_\alpha is in general nonlocal: a Wilson observable integrates around a loop, an integral invariant integrates over MM, a spectral quantity depends on the fields through a global eigenvalue problem. Its variation is accordingly given not by a pointwise partial derivative but by the pairing of distributional kernels with the variations: δrα=∫M ⁣[δrαδgμν(y) δgμν(y)+⟨δrαδAμ(y), δAμ(y)⟩+⟨ ⁣⟨δrαδΦ(y), δΦ(y)⟩ ⁣⟩]−g(y)  d4y,(67) \delta r_\alpha =\int_M\!\Bigl[ \frac{\delta r_\alpha}{\delta g^{\mu\nu}(y)}\,\delta g^{\mu\nu}(y) +\Bigl\langle \frac{\delta r_\alpha}{\delta A_\mu(y)},\,\delta A_\mu(y)\Bigr\rangle +\Bigl\langle\!\Bigl\langle \frac{\delta r_\alpha}{\delta \Phi(y)},\,\delta\Phi(y) \Bigr\rangle\!\Bigr\rangle \Bigr]\sqrt{-g(y)}\;\mathrm{d}^4y ,\tag{67} where δrα/δgμν(y)\delta r_\alpha/\delta g^{\mu\nu}(y) etc. denote the VαV_\alpha-valued distributional kernels representing the derivative, ⟨⋅,⋅⟩\langle\cdot,\cdot\rangle is the Ad⁡\operatorname{Ad}-invariant pairing on g\mathfrak{g}, and ⟨ ⁣⟨⋅,⋅⟩ ⁣⟩\langle\!\langle\cdot,\cdot\rangle\!\rangle is the duality pairing between W∗W^{*} and WW discussed in Section 7.3. (For a Wilson loop rαr_\alpha the kernel δrα/δAμ(y)\delta r_\alpha/\delta A_\mu(y) is supported on the loop and is a distribution, not a function; (67) is exactly the statement that must be used, and a pointwise ∂rα/∂Aμ(y)\partial r_\alpha/\partial A_\mu(y) does not exist.)

Then, writing ∂Srel/∂rα∈Vα∗\partial S_{\mathrm{rel}}/\partial r_\alpha\in V_\alpha^{*} for the derivative of SrelS_{\mathrm{rel}} with respect to its VαV_\alpha-argument (a bounded linear functional, and an ordinary partial derivative only when VαV_\alpha is finite-dimensional), the chain rule reads δSrelδgμν(y)=δSrelδgμν(y)∣r  fixed+∑α∈Adyn⟨∂Srel∂rα,  δrαδgμν(y)⟩Vα∗ ⁣,Vα,(68) \frac{\delta S_{\mathrm{rel}}}{\delta g^{\mu\nu}(y)} =\left.\frac{\delta S_{\mathrm{rel}}}{\delta g^{\mu\nu}(y)}\right|_{r\;\mathrm{fixed}} +\sum_{\alpha\in A_{\mathrm{dyn}}} \Bigl\langle \frac{\partial S_{\mathrm{rel}}}{\partial r_\alpha},\; \frac{\delta r_\alpha}{\delta g^{\mu\nu}(y)}\Bigr\rangle_{V_\alpha^*\!,V_\alpha} ,\tag{68} and identically with gμν(y)g^{\mu\nu}(y) replaced by Aμ(y)A_\mu(y) or by the matter components. The sum is over the dynamical subfamily (66), and converges by the unconditional-convergence hypothesis imposed there. Only in the special case where Vα=RV_\alpha=\mathbb{R} and rαr_\alpha is a local scalar field does (68) reduce to an ordinary pointwise partial derivative; in general it does not.

(b) rαr_\alpha labels a fixed topological or boundary sector. Then δrα=0\delta r_\alpha=0 under all variations within the sector, this is what “fixed sector” means, and rαr_\alpha enters the field equations only as a parameter. The second term of (68) is absent.

In neither case is rαr_\alpha varied as an independent dynamical field. A model wishing to promote rαr_\alpha to a field must adjoin it to the configuration tuple, enlarge Cgeo\mathcal{C}_{\mathrm{geo}}, and supply its own kinetic term; that is a different model, and its Euler–Lagrange equation is an additional equation not derived here.

Matter pairings and independent components

Convention 7.4 (Matter variation and the dual pairing).

The representation ρ ⁣:G→GL(W)\rho\colon G\to\mathrm{GL}(W) is not assumed unitary (Convention 2.1), and WW may be complex. Accordingly the matter Euler operator is valued in the dual, and the variational pairing must be specified. We adopt the following, and use it consistently.

(i) Real independent components. Suppose Φ\Phi denotes a collection of real independent field components. This is always achievable: decompose a complex field into its real and imaginary parts, or a section of a complex bundle into its underlying real bundle. Then δS/δΦ\delta S/\delta\Phi is valued in the real dual bundle P×ρ∗W∗P\times_{\rho^{*}}W^{*}, and the pairing ⟨ ⁣⟨⋅,⋅⟩ ⁣⟩ ⁣:W∗×W⟶R\langle\!\langle\cdot,\cdot\rangle\!\rangle\colon W^{*}\times W\longrightarrow\mathbb{R} is the canonical duality pairing. This pairing is GG-invariant for the contragredient action ρ∗(h)=ρ(h−1)T\rho^{*}(h)=\rho(h^{-1})^{\mathsf{T}}, and requires no metric on WW. There is then a single Euler equation EΦ=0\mathcal{E}_\Phi=0.

(ii) Complex fields treated holomorphically. If instead Φ\Phi is treated as a complex field with Φ\Phi and Φˉ\bar\Phi varied independently, the usual convention for a charged scalar or a Dirac spinor, then there are two Euler equations, EΦ:=1−gδSδΦˉ=0andEΦ‾:=1−gδSδΦ=0,(69) \mathcal{E}_{\Phi}:=\frac{1}{\sqrt{-g}}\frac{\delta S}{\delta \bar\Phi}=0 \qquad\text{and}\qquad \overline{\mathcal{E}_{\Phi}}:=\frac{1}{\sqrt{-g}}\frac{\delta S}{\delta \Phi}=0 ,\tag{69} which are conjugate to one another when the action is real, and the pairing used in the variation is the sesquilinear one furnished by a ρ\rho-invariant Hermitian form on WW, which exists precisely when ρ\rho is unitary. If ρ\rho is not unitary, no such Hermitian form is available and one must revert to convention (i).

For definiteness, and to avoid carrying two conjugate equations through every formula, in the statements below Φ\Phi denotes real independent field components in the sense of (i), and EΦ\mathcal{E}_\Phi is the corresponding single dual-valued Euler operator. Every result restates verbatim in convention (ii) upon replacing EΦ=0\mathcal{E}_{\Phi}=0 by the conjugate pair (69) and ⟨ ⁣⟨⋅,⋅⟩ ⁣⟩\langle\!\langle\cdot,\cdot\rangle\!\rangle by the invariant Hermitian pairing.

Response tensors, currents, and Euler operators

Definition 7.5 (Responses).

For each nongravitational sector X∈{YM,m,rel}X\in\{\mathrm{YM},\mathrm{m},\mathrm{rel}\} define the stress-energy tensor TμνX  :=  −2−g δSXδgμν,(70) T^{X}_{\mu\nu} \;:=\; -\frac{2}{\sqrt{-g}}\,\frac{\delta S_X}{\delta g^{\mu\nu}} ,\tag{70} the gauge current Jmμ  :=  −1−g δSmδAμ,Jrelμ  :=  −1−g δSrelδAμ,(71) J^{\mu}_{\mathrm{m}} \;:=\; -\frac{1}{\sqrt{-g}}\,\frac{\delta S_{\mathrm{m}}}{\delta A_\mu}, \qquad J^{\mu}_{\mathrm{rel}} \;:=\; -\frac{1}{\sqrt{-g}}\,\frac{\delta S_{\mathrm{rel}}}{\delta A_\mu},\tag{71} each valued in g\mathfrak{g} (with g\mathfrak{g}-indices contracted using ⟨⋅,⋅⟩\langle\cdot,\cdot\rangle), and the matter Euler operators EΦX  :=  1−g δSXδΦ,(72) \mathcal{E}^{X}_{\Phi} \;:=\; \frac{1}{\sqrt{-g}}\,\frac{\delta S_X}{\delta\Phi} ,\tag{72} valued in the dual bundle and paired with δΦ\delta\Phi by ⟨ ⁣⟨⋅,⋅⟩ ⁣⟩\langle\!\langle\cdot,\cdot\rangle\!\rangle as in Convention 7.4(i). For X=relX=\mathrm{rel} the functional derivatives in (70)–(72) are those computed by the chain rule (68), and thus already include the relation-mediated contributions.

Lemma 7.6 (Yang–Mills stress tensor).

With the normalization (65), TμνYM=1gYM2(⟨Fμρ,Fνρ⟩−14 gμν ⟨Fρσ,Fρσ⟩),(73) T^{\mathrm{YM}}_{\mu\nu} =\frac{1}{g_{\mathrm{YM}}^{2}} \left( \bigl\langle F_{\mu\rho},F_{\nu}{}^{\rho}\bigr\rangle -\tfrac14\,g_{\mu\nu}\,\bigl\langle F_{\rho\sigma},F^{\rho\sigma}\bigr\rangle \right),\tag{73} which is symmetric, gauge invariant, and (in four dimensions) trace free.

Proof. Write SYM=−14gYM2∫M⟨Fμρ,Fνσ⟩gμνgρσ−g d4xS_{\mathrm{YM}}=-\tfrac{1}{4g_{\mathrm{YM}}^2}\int_M \langle F_{\mu\rho},F_{\nu\sigma}\rangle g^{\mu\nu}g^{\rho\sigma}\sqrt{-g}\,\mathrm{d}^4x; the components Fμν=∂μAν−∂νAμ+[Aμ,Aν]F_{\mu\nu}=\partial_\mu A_\nu-\partial_\nu A_\mu+[A_\mu,A_\nu] are independent of gg. Using δ−g=−12−g gμν δgμν\delta\sqrt{-g}=-\tfrac12\sqrt{-g}\,g_{\mu\nu}\,\delta g^{\mu\nu} and varying the two inverse metrics, δSYM=−14gYM2∫M(2⟨Fμρ,Fνρ⟩−12gμν⟨Fρσ,Fρσ⟩)δgμν−g d4x,\delta S_{\mathrm{YM}} =-\frac{1}{4g_{\mathrm{YM}}^2}\int_M \Bigl( 2\langle F_{\mu\rho},F_{\nu}{}^{\rho}\rangle -\tfrac12 g_{\mu\nu}\langle F_{\rho\sigma},F^{\rho\sigma}\rangle \Bigr)\delta g^{\mu\nu}\sqrt{-g}\,\mathrm{d}^4x , and (70) gives (73). Gauge invariance follows from Ad⁡\operatorname{Ad}-invariance of ⟨⋅,⋅⟩\langle\cdot,\cdot\rangle and (23); tracelessness from gμν⟨Fμρ,Fνρ⟩=⟨Fρσ,Fρσ⟩g^{\mu\nu}\langle F_{\mu\rho},F_\nu{}^\rho\rangle=\langle F_{\rho\sigma},F^{\rho\sigma}\rangle and gμνgμν=4g^{\mu\nu}g_{\mu\nu}=4. ◻

Lemma 7.7 (Yang–Mills variation with respect to the connection).

Under Assumption 7.1, δSYM=−1gYM2∫M⟨Fμν, Dμ δAν⟩ d ⁣vol⁡g=  1gYM2∫M⟨DμFμν, δAν⟩ d ⁣vol⁡g,(74) \delta S_{\mathrm{YM}} =-\frac{1}{g_{\mathrm{YM}}^{2}}\int_M \bigl\langle F^{\mu\nu},\,D_\mu\,\delta A_\nu\bigr\rangle\,\mathrm{d}\!\operatorname{vol}_g =\;\frac{1}{g_{\mathrm{YM}}^{2}}\int_M \bigl\langle D_\mu F^{\mu\nu},\,\delta A_\nu\bigr\rangle\,\mathrm{d}\!\operatorname{vol}_g,\tag{74} up to the treated boundary term.

Proof. From Fμν=∂μAν−∂νAμ+[Aμ,Aν]F_{\mu\nu}=\partial_\mu A_\nu-\partial_\nu A_\mu+[A_\mu,A_\nu] one has δFμν=Dμ δAν−Dν δAμ.(75) \delta F_{\mu\nu}=D_\mu\,\delta A_\nu - D_\nu\,\delta A_\mu .\tag{75} Hence, from (65), δSYM=−14gYM2∫M2 ⟨Fμν, δFμν⟩ d ⁣vol⁡g=−12gYM2∫M⟨Fμν, DμδAν−DνδAμ⟩ d ⁣vol⁡g.\delta S_{\mathrm{YM}} =-\frac{1}{4g_{\mathrm{YM}}^{2}}\int_M 2\,\bigl\langle F^{\mu\nu},\,\delta F_{\mu\nu}\bigr\rangle\,\mathrm{d}\!\operatorname{vol}_g =-\frac{1}{2g_{\mathrm{YM}}^{2}}\int_M \bigl\langle F^{\mu\nu},\,D_\mu\delta A_\nu - D_\nu\delta A_\mu\bigr\rangle\,\mathrm{d}\!\operatorname{vol}_g. The two terms in the bracket are equal after relabelling, by the antisymmetry of FμνF^{\mu\nu}: swapping the dummy indices μ↔ν\mu\leftrightarrow\nu in the second term gives −⟨Fνμ,DμδAν⟩=+⟨Fμν,DμδAν⟩-\langle F^{\nu\mu},D_\mu\delta A_\nu\rangle=+\langle F^{\mu\nu},D_\mu\delta A_\nu\rangle. Therefore the bracket contributes twice the first term, the factor 12\tfrac12 cancels, and δSYM=−1gYM2∫M⟨Fμν, DμδAν⟩ d ⁣vol⁡g,\delta S_{\mathrm{YM}} =-\frac{1}{g_{\mathrm{YM}}^{2}}\int_M \bigl\langle F^{\mu\nu},\,D_\mu\delta A_\nu\bigr\rangle\,\mathrm{d}\!\operatorname{vol}_g, which is the first equality in (74). Covariant integration by parts, legitimate because ⟨⋅,⋅⟩\langle\cdot,\cdot\rangle is Ad⁡\operatorname{Ad}-invariant, hence DD-compatible, and because the boundary term vanishes by Assumption 7.1, moves DμD_\mu onto FμνF^{\mu\nu} and flips the sign, giving the second equality. ◻

The coupled field equations

Theorem 7.8 (Coupled field equations).

Under Assumption 7.1 and Conventions 7.3 and 7.4(i), stationarity of StotS_{\mathrm{tot}} under independent variations of gμνg^{\mu\nu}, AμA_\mu, and Φ\Phi is equivalent to the system (76)Gμν+Λgμν=8πGN(TμνYM+Tμνm+Tμνrel),(77)1gYM2 DμFμν=Jmν+Jrelν,(78)EΦm+EΦrel=0,\begin{aligned} \qquad\text{(76)} G_{\mu\nu}+\Lambda g_{\mu\nu} &=8\pi G_N\Bigl( T^{\mathrm{YM}}_{\mu\nu}+T^{\mathrm{m}}_{\mu\nu}+T^{\mathrm{rel}}_{\mu\nu} \Bigr), \\[0.35em] \qquad\text{(77)} \frac{1}{g_{\mathrm{YM}}^{2}}\,D_\mu F^{\mu\nu} &=J^{\nu}_{\mathrm{m}}+J^{\nu}_{\mathrm{rel}}, \\[0.35em] \qquad\text{(78)} \mathcal{E}^{\mathrm{m}}_{\Phi}+\mathcal{E}^{\mathrm{rel}}_{\Phi} &=0, \end{aligned} with representation indices and the pairings ⟨⋅,⋅⟩\langle\cdot,\cdot\rangle and ⟨ ⁣⟨⋅,⋅⟩ ⁣⟩\langle\!\langle\cdot,\cdot\rangle\!\rangle restored as required by GG and ρ\rho.

Proof. Metric variation. The standard variation of (64), after the boundary treatment stipulated in Assumption 7.1 (which is exactly what disposes of the total-derivative term ∫MgμνδRμν−g\int_M g^{\mu\nu}\delta R_{\mu\nu}\sqrt{-g}; under (V3) it is the Gibbons–Hawking–York term that cancels it [15, 5]), gives δSEH=116πGN∫M(Gμν+Λgμν) δgμν d ⁣vol⁡g.(79) \delta S_{\mathrm{EH}} =\frac{1}{16\pi G_N}\int_M \bigl(G_{\mu\nu}+\Lambda g_{\mu\nu}\bigr)\,\delta g^{\mu\nu}\,\mathrm{d}\!\operatorname{vol}_g.\tag{79} By Definition 7.5, δ(SYM+Sm+Srel)∣δg=−12∫M(TμνYM+Tμνm+Tμνrel) δgμν d ⁣vol⁡g,(80) \delta\bigl(S_{\mathrm{YM}}+S_{\mathrm{m}}+S_{\mathrm{rel}}\bigr)\Big|_{\delta g} =-\frac12\int_M \bigl( T^{\mathrm{YM}}_{\mu\nu}+T^{\mathrm{m}}_{\mu\nu}+T^{\mathrm{rel}}_{\mu\nu} \bigr)\,\delta g^{\mu\nu}\,\mathrm{d}\!\operatorname{vol}_g,\tag{80} where δSrel\delta S_{\mathrm{rel}} is computed by the chain rule (68): in regime (a) of Convention 7.3 it includes the relation-mediated kernel contributions, and in regime (b) those are absent. In either case (80) defines its left side via (70) and adds no assumption. Setting δStot=0\delta S_{\mathrm{tot}}=0 for arbitrary symmetric δgμν\delta g^{\mu\nu} (compactly supported, or boundary-vanishing) and applying the fundamental lemma of the calculus of variations gives 116πGN(Gμν+Λgμν)−12(TμνYM+Tμνm+Tμνrel)=0,\frac{1}{16\pi G_N}\bigl(G_{\mu\nu}+\Lambda g_{\mu\nu}\bigr) -\frac12\bigl(T^{\mathrm{YM}}_{\mu\nu}+T^{\mathrm{m}}_{\mu\nu}+T^{\mathrm{rel}}_{\mu\nu}\bigr)=0 , which is (76) with the displayed 8πGN8\pi G_N normalization.

Gauge variation. By Lemma 7.7, δSYM∣δA=1gYM2∫M⟨DμFμν, δAν⟩ d ⁣vol⁡g,\delta S_{\mathrm{YM}}\big|_{\delta A} =\frac{1}{g_{\mathrm{YM}}^{2}}\int_M \bigl\langle D_\mu F^{\mu\nu},\,\delta A_\nu\bigr\rangle\,\mathrm{d}\!\operatorname{vol}_g, while by the definitions (71), δ(Sm+Srel)∣δA=−∫M⟨Jmν+Jrelν, δAν⟩ d ⁣vol⁡g.\delta\bigl(S_{\mathrm{m}}+S_{\mathrm{rel}}\bigr)\big|_{\delta A} =-\int_M\bigl\langle J^{\nu}_{\mathrm{m}}+J^{\nu}_{\mathrm{rel}},\, \delta A_\nu\bigr\rangle\,\mathrm{d}\!\operatorname{vol}_g. Setting the sum of the two to zero for arbitrary δAν\delta A_\nu, and using the nondegeneracy of ⟨⋅,⋅⟩\langle\cdot,\cdot\rangle, gives (77).

Matter variation. SEHS_{\mathrm{EH}} and SYMS_{\mathrm{YM}} are independent of Φ\Phi, so by (72) δΦStot=∫M⟨ ⁣⟨ EΦm+EΦrel,  δΦ ⟩ ⁣⟩ d ⁣vol⁡g\delta_\Phi S_{\mathrm{tot}} =\int_M \langle\!\langle\,\mathcal{E}^{\mathrm{m}}_\Phi+\mathcal{E}^{\mathrm{rel}}_\Phi,\; \delta\Phi\,\rangle\!\rangle\,\mathrm{d}\!\operatorname{vol}_g; arbitrariness of the real independent components δΦ\delta\Phi and nondegeneracy of the duality pairing give (78). Under Convention 7.4(ii) this is replaced by the conjugate pair (69).

The three variations are independent, so stationarity of StotS_{\mathrm{tot}} is equivalent to the simultaneous validity of (76)–(78). ◻

Remark 49 (What has and has not been derived).

The tensor TμνrelT^{\mathrm{rel}}_{\mu\nu} is not an independent postulate. By (70) and the chain rule (68) it is the metric functional derivative of a specified Ggeo\mathfrak{G}_{\mathrm{geo}}-invariant action satisfying (R1)–(R2). Different source completions, and different couplings of the same completion, produce different TμνrelT^{\mathrm{rel}}_{\mu\nu}, JrelμJ^{\mu}_{\mathrm{rel}}, EΦrel\mathcal{E}^{\mathrm{rel}}_{\Phi}. Theorem 7.8 asserts only the structure of the response, that a completed relation enters Tier-1 dynamics through functional variation of an invariant action, with the normalizations displayed, and asserts nothing about the magnitude, sign, or empirical existence of any such term. No new interaction is proposed, and no empirical claim is made.

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