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Compact Einstein–Hilbert variation and SI coupling

Statement

Let (M,g,N,o) be as in Oriented Lorentzian fields, observers and coordinate conventions. Write R:=S=gabRic⁡ab:M→R for the smooth scalar curvature of The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors, with Ric⁡bd=Rabad and Gab=Ric⁡ab−12Rgab in that supplier's curvature convention. For a compactly supported metric variation, write qab=δgab, hab=δgab=−gacgbdqcd, w=∣det⁡(gab)∣, and Va=gbdδΓadb−gabδΓddb, where δΓabc=12gad(∇bhcd+∇chbd−∇dhbc); curvature and Einstein tensors are as in The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors. The local density identity is

δ((R−2Λ)w)=w(Gab+Λgab)qab+∂a(wVa).

Fix constants c>0, GN>0, μ0>0, and Λ∈R. Regard these as formal coefficients; their physical interpretation and units are not assumptions of this mathematical lemma. For smooth metric variations with compact support in the interior, at fixed bundle connection and fixed matter fields, consider the action difference

Stot=c316πGN∫M(R−2Λ) volg−14μ0c∫MFabFab volg+Sm,

where noncompact action values are used only through compactly supported differences, F is the curvature of a fixed smooth bundle connection, and Sm has Hilbert tensor Tm in the convention of The Hilbert stress-energy tensor of a metric-dependent action. Let TEM be the electromagnetic Hilbert tensor supplied by the compact Maxwell variation of Compact potential and metric variation of the Maxwell action, and set κE:=8πGN/c4. Then for every compactly supported inverse-metric variation qab=δgab,

δStot=c316πGN∫M(Gab+Λgab−κE(TabEM+Tabm))qab volg.

Consequently, stationarity under all such metric variations is equivalent to

Gab+Λgab=κE(TabEM+Tabm).

Any tensor fields satisfying this equation necessarily have ∇a(TabEM+Tabm)=0 because Λ is constant. This is a compatibility condition, not a claim that the coupled field equations have a solution or that matter and Maxwell equations follow from metric stationarity.

For dimensional bookkeeping in length coordinates one may assign [R]=[Λ]=m−2, [c]=m s−1, [GN]=m3 kg−1 s−2, [μ0]=H m−1, [Fab]=Wb m−2, and [Tm]=[TEM]=J m−3. Then every action term has units J s and κET has units m−2. These are formal assignments only; the lemma assumes no measured parameter value or physical field law.

Facts & Assumptions

Given: A smooth oriented time-oriented Lorentzian four-manifold with fixed signature, constants c,GN,μ0>0, constant Λ, a fixed smooth connection sector and matter configuration, and compactly supported inverse-metric variations.

[F1]

With R=S as defined in the Statement, for a smooth fixed-signature Lorentzian metric family, the local Einstein–Hilbert density satisfies ∂s(w(s)R(s))∣s=0=wGabqab+∂a(wVa), with the inverse variation and tensor δΓ given in clauses (a)–(d) of First variation of the Einstein-Hilbert density under compactly supported metric variations, and of the timelike length functional. Its clause (e) proves the compact action formula when the support is inside one chart. The extension to arbitrary compact support is proved below, rather than attributed to that chart-only clause. [F2] also supplies the global compact divergence and finite-chart differentiation arguments proved in the preliminary localization argument of Compact potential and metric variation of the Maxwell action.

[F2]

The planned M03 Maxwell metric variation is δgSEM=−12c∫MTabEMqabvolg, with TabEM=μ0−1(FacFbc−14gabFcdFcd), for fixed lower F and compact inverse-metric variations. (Compact potential and metric variation of the Maxwell action)

[F3]

The matter Hilbert tensor satisfies δgSm=−12c∫MTabmqabvolg. (The Hilbert stress-energy tensor of a metric-dependent action)

[F4]

If a continuous symmetric coefficient pairs to zero with every smooth compactly supported symmetric test tensor, then it vanishes pointwise. (A continuous symmetric coefficient orthogonal to every compactly supported variation vanishes)

[F5]

The contracted Bianchi identity is ∇aGab=0, and the metric is covariantly constant: ∇g=0. (The second Bianchi identity and the vanishing divergence of the Einstein tensor)

[A1]

The compact variations are smooth families fixed off a common compact set K for all sufficiently small parameters, within the fixed Lorentzian signature and fixed bundle sector; Λ,c,GN,μ0 are held constant. For any compactly supported direction q, such a family is realized by g(s)=g+sh, h=−gqg, on a sufficiently small uniform parameter interval as proved in the Maxwell supplier.

[A2]

The supporting smooth Lorentzian geometry is under the published ACω tangent-bundle convention; no use of full AC is needed in these variational calculations. (The Axiom of Countable Choice (ACω))

[F6]

Compactly supported top forms have the finite-chart integral of Integral of a compactly supported top form, independent of partition by Independence of atlas, partition and refinement. Under ACω a subordinate smooth partition exists by Smooth partitions of unity exist on manifolds.

Proof

technique · add the three independent first variations, normalize the common coefficient, and use compactly supported test tensors for the pointwise Euler–Lagrange equation
1.1givenA1A2F1F2F6algebra

For a family in [A1], the top form ωs=(R(g(s))−2Λ)volg(s)−(R(g)−2Λ)volg is supported in the common compact K. Define its relative action by [F6], even if the separate background integrals diverge. Fix a subordinate partition independently of s; only finitely many terms meet K, and each has compact support inside its chart. The uniform difference-quotient argument in the Maxwell supplier [F2] differentiates this finite sum. Clause (d) of [F1] gives its derivative density locally, and δ(−2Λvolg)=Λgabqabvolg. The field V is global because δΓ is a tensor, and is supported in K. The compact divergence argument in [F2] now gives ∫M∇aVavolg=0: apply chart FTC to each ρiV and sum, with ∑idρi=0 near K. Thus no single chart or enclosing finite singular chain is presumed. Multiplication by c3/(16πGN) yields c316πGN∫M(Gab+Λgab)qabvolg, as claimed.

2.1F2F3step 1.1algebra

Add [F2] and [F3]. Since 12c=c316πGN8πGNc4, the total variation is exactly the expression in the Statement with κE=8πGN/c4.

3.1A1F4step 2.1algebra

If the action is stationary for every compactly supported qab, step 2.1 implies that the continuous symmetric coefficient Gab+Λgab−κE(TabEM+Tabm) pairs to zero with every such q. Because c,GN>0, its prefactor is nonzero; [F4] therefore gives the displayed field equation pointwise.

4.1step 2.1step 3.1algebra

Conversely, if the displayed field equation holds pointwise, the coefficient in step 2.1 is zero everywhere, so its integral vanishes for every compactly supported q. This proves stationarity and the equivalence.

5.1A2F5step 3.1algebra∎

Take the covariant divergence of the field equation in step 3.1. By [F5], ∇aGab=0 and ∇a(Λgab)=Λ∇agab=0 because Λ is constant. Since κE>0, division gives ∇a(TabEM+Tabm)=0. No PDE existence follows from this necessary compatibility identity.

Remarks

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