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Smooth local geometric existence and uniqueness for source-free Einstein–Maxwell data

Statement

Assume Countable Choice and Dependent Choice. Let Σ be a smooth oriented three-manifold without boundary, with smooth Riemannian metric h, smooth symmetric covariant tensor K, and smooth spatial vectors e,b. Fix κ>0, μ0>0, Λ∈R, use signature (−,+,+,+) and K(X,Y)=g(∇Xn,Y), and suppose the four Einstein–Maxwell constraints of Gauss-Codazzi and Maxwell initial constraints hold. In SI convention use length coordinate x0=ct, dimensionless g,h, K in m−1, and e=E/c, b=B in tesla. Reconstruct the complete initial two-form on RN⊕TΣ by F(N,ei)=−ei,F(ei,ej)=ϵijkbk, where N is the future unit normal symbol and (ei) is a positively oriented h-orthonormal frame. Then the data have a smooth time-oriented local source-free Einstein–Maxwell development on an open variable-width neighborhood of the entire initial surface. After restriction to a smaller collar, the interior of its intrinsic domain of dependence is a globally hyperbolic neighborhood with Σ Cauchy. Any two developments of this same model and complete data are related near the entire initial surface by a data-fixing, time-orientation-preserving isometry carrying F to F. There is no uniform positive time width for noncompact Σ and no global-in-time conclusion.

Facts & Assumptions

Given: Countable Choice, Dependent Choice, the smooth oriented data and constants in the Statement, and the specified tetrad, field and extrinsic-curvature conventions.

[L1]

Draft model Electrovacuum tensor Cauchy system fixes G+Λg=κT, Tab=μ0−1(FacFbc−14gabFcdFcd), dF=d⋆gF=0, and the curvature and orientation/sign conventions. Its item file is listed in batch 6; its status is draft and its precheck is pending; the application remains conditional.

[L2]

Draft constraint result Gauss-Codazzi and Maxwell initial constraints states, with this K and field convention, Diei=Dibi=0,R(h)+(tr⁡hK)2−∣K∣h2=2Λ+κμ0(∣e∣h2+∣b∣h2),DjKji−Ditr⁡hK=−κμ0(e×hb)i. Its item file is present but listed in batch 6 and has verification precheck pending, so the interface remains conditional.

[L3]

Draft stress identity Maxwell stress algebra and covariant conservation gives ∇aTab=−Fbcjc for smooth fields satisfying dF=0 and ∇aFab=−μ0jb. The exact source-free Hodge conversion is ∇aFab=13!εbacd(d⋆gF)acd=1∣det⁡g∣∂a(∣det⁡g∣Fab),εabcd:=(volg)abcd, with indices raised by g−1. It follows by expanding d⋆gF=3∇[a(⋆gF)cd], using metric-compatibility ∇aεbcde=0, (⋆gF)cd=12εcdefFef and εbacdεcdef=−2(δebδfa−δfbδea); the coordinate divergence uses Γaac=∂clog⁡∣det⁡g∣ and the vanishing contraction ΓbacFac. Hence the source-free equations in [L1] meet both hypotheses with j=0 before the unreduced Einstein equation is used. The file exists but is listed in batch 6 and its precheck is pending; this input remains conditional.

[L4]

Draft harmonic initialization Harmonic initial data relative to a fixed smooth background specifies all initial metric first derivatives, including auxiliary reduction variables, so H=0 and the initial reduced state is compatible with the chosen smooth background. Its file exists but is listed in batch 6 and its precheck is pending; this use remains conditional.

[F1]

Positive symmetric Maxwell field-strength reduction gives the symmetric Maxwell principal block and positive time matrix; Principal part of the reduced Einstein operator and its first-order symmetric hyperbolic reduction gives the metric wave block; Coupled reduced Einstein–Maxwell local evolution combines them, verifies smooth coefficients and no derivative coupling through the algebraic stress, and applies the conditional local solver.

[F2]

Local high-Sobolev and smooth electrovacuum includes the local smooth existence clause on arbitrary smooth initial slices. It proves the derivative-variable compatibility, local Maxwell constraint propagation and Einstein harmonic recovery, conditional on the CP01 carriers named above.

[F3]

Maxwell Gauss constraints propagate by form transport proves local recovery of dF=d⋆gF=0 from the normal-slot equations ιndF=ιnd⋆gF=0 and zero initial Gauss divergences for C1 metric, field and transverse future unit normal; the smooth local developments here satisfy these hypotheses. Einstein harmonic gauge propagation with Maxwell on shell proves local H=0 and recovery of the unreduced Einstein equation from the normal constraints and conserved stress.

[F4]

Local geometric development for a fixed covariant Einstein-matter model with complete constrained data applies to a fixed covariant matter model with a symmetric-hyperbolic reduction, complete smooth matter initialization, propagated auxiliary compatibility, on-shell stress conservation, and the Einstein constraints. Its actual published carrier has precheck pending; its statement and full local proof were inspected.

[F5]

Causal and Cauchy-surface inputs for smooth electrovacuum developments collects the exact local causal-neighborhood, globally hyperbolic Cauchy-neighborhood, and choice interfaces used in the local-development conclusion.

Proof

1.1givenL1L2algebra

On the abstract initial bundle RN⊕TΣ, the displayed formulas assign the three normal-spatial components and the three spatial-spatial components of an antisymmetric two-form. These are all six independent components of a two-form in four dimensions, so they determine a unique complete initial F without choosing a potential or assuming global exactness. They are smooth because h,e,b are smooth and the reconstruction is tensorial under oriented orthonormal-frame changes.

1.2givenL4F1F2F3F4algebra

In each relatively compact initial coordinate ball choose product coordinates (x0,xi) with x0=0 on the slice and ∂0=n there. Choose a smooth positive spatial background γ and put Qi:=hjk(Γ(h)ijk−Γ(γ)ijk). Relative to gˉ=−(dx0)2+γij(x)dxidxj, prescribe gij=hij, g00=−1, g0i=0, ∂0gij=2Kij, ∂0g00=−2tr⁡hK, and ∂0g0i=hijQj. The same Christoffel computation as the periodic construction [L4], now carried out on this local chart, gives H0=−tr⁡hK+tr⁡hK=0 and Hi=−Qi+hjk(Γ(h)ijk−Γ(γ)ijk)=0. This local jet is smooth and compatible with the first-order reduction. The metric block has time matrix diag⁡(I,−g00I,gijI) by [F1]'s reduced Einstein principal-part supplier, and the Maxwell block has time matrix α−1I6 by [F1]. On the open state neighborhood where g00<0, (gij)>0 and α>0, their block sum is positive definite; every spatial matrix is symmetric. Since T(g,F) is algebraic in the state, it contributes only to lower-order terms and creates no off-diagonal derivative blocks. The prescribed local high-Sobolev construction [F2] applies after the compact chart localization in its proof and yields a reduced solution. Its derivative relations propagate; [F3] restores both Maxwell equations and the full Einstein equation on a smaller local domain. Every smooth physical solution in the same harmonic chart extracts to this same coefficient system because the component equations are precisely the harmonic-reduced Einstein equation and field-strength Maxwell evolution. This verifies the local symmetric-hyperbolic, recovery and compatibility hypotheses of [F4].

2.1step 1.1L1F4algebra

The equations dF=0 and d⋆gF=0 are covariant: pullback commutes with exterior differentiation, and for an orientation-preserving diffeomorphism ϕ, ϕ∗(⋆gF)=⋆ϕ∗g(ϕ∗F). The algebraic stress T(g,F) is likewise natural under pullback. Thus the matter field, equations, stress and initial reconstruction define one fixed covariant model of the kind required by [F4]; no coordinate-dependent potential gauge is introduced.

2.2step 1.1step 1.2L1L2L3F3F4

Step 1.2, using [F3], has already recovered dF=d⋆gF=0 on the local development; [L1] fixes the corresponding source-free model and stress tensor. The exact Hodge conversion in [L3] gives ∇aFab=0, so the stress identity applies with j=0 and yields ∇aTab=0, independently of the unreduced Einstein equation. The constraints in the Statement are exactly [L2]'s four normal-projection constraints with the same sign, orientation, κ,μ0,Λ and K conventions. This verifies the conservation and Einstein-constraint hypotheses of [F4].

3.1step 1.1step 2.1step 2.2step 1.2L2L3L4F4F5∎

We have now checked every specific input of [F4]: a fixed covariant model by step 2.1, complete matter data and smooth initialization by step 1.1 and the local harmonic jet in step 1.2, a smooth symmetric-hyperbolic reduction and reconstruction by step 1.2, on-shell stress conservation by step 2.2, and the model's Einstein constraints by [L2]. The choice assumptions are those in the Statement. Applying [F4] gives the smooth local development, variable-width collar, intrinsic globally hyperbolic Cauchy neighborhood and data-fixing isometry matching F. The causal qualifications in [F5] confirm that no compactness or uniform collar width is used.

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