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Exact source/test-field/backreaction consistency distinction

Physical scope

Fixed smooth vacuum metric with smooth source-free or sourced Maxwell data, including joint field/current scaling, the exact quadratic electromagnetic stress residual and its compact-chart component norm, charged-dust scaling, and finite Coulomb-annulus energy. This is test-field bookkeeping; it includes no source-matter stress in the residual, no nearby coupled family, singular point charge, or self-field.

Statement

Use the smooth oriented, time-oriented Lorentzian four-manifold, Levi–Civita connection ∇, and length-coordinate SI conventions of Smooth matter quantities, current and observer observables and the separately prescribed Maxwell test model of Separately adopted fixed-background Maxwell and charged probes. Here U is open, g is the fixed metric, a field strength F is a smooth real two-form, and a prescribed current j is a smooth real vector field. The formal stress tensor and constants are

TEMab(g,F)=1μ0(FacFbc−14gabFcdFcd),TabEM=gacgbdTEMcd,κ=8πGNc4>0.

The adopted Maxwell alternatives are dF=0, d(⋆gF)=0 when source-free, or dF=0, ∇aFab=−μ0jb for a separately prescribed current. Let g satisfy Gab(g)+Λgab=0 on U, where Λ is constant. Define the electromagnetic stress residual relative to this unchanged vacuum metric, with no matter stress included, by

Rab(g,F;Λ):=Gab(g)+Λgab−κTabEM(g,F).

First let F0 be a smooth source-free Maxwell two-form on U. For real dimensionless δ, Fδ:=δF0 remains source-free and

Rab(g,Fδ;Λ)=−κδ2TabEM(g,F0).

The same conclusion holds for an actual smooth sourced Maxwell pair: let F0 be a smooth real two-form and j0 a smooth real vector field on U satisfying dF0=0 and ∇a(F0)ab=−μ0j0b. With Fδ:=δF0 and jδ:=δj0, the pair still satisfies the same sourced Maxwell equations, and

Rab(g,Fδ;Λ)=−κδ2TabEM(g,F0).

For a compact set K in a fixed smooth coordinate chart contained in U and a smooth covariant two-tensor S, define ∥S∥∞,K:=max⁡0≤a,b≤3sup⁡p∈K∣Sab(p)∣ when K≠∅, and set ∥S∥∞,∅:=0. In either Maxwell case,

∥R(g,Fδ;Λ)∥∞,K=κδ2∥TEM(g,F0)∥∞,K.

If δ≠0 and F0 is nonzero at a point, its observer energy is positive there, so this electromagnetic/vacuum-background residual is nonzero. In the sourced case this does not test a full Einstein–Maxwell–matter equation, because no source-matter stress is included in R. The residual is a consistency calculation, not an estimate of distance to a different metric solution.

Separately, on an open region where smooth charged-dust quantities have ρ>0, Tmab=ρUaUb, ja=σUa, and the formal matter-exchange equation holds, replacing (ρ,σ) by (ηρ,ησ) for η>0 scales matter stress and current linearly, leaves σ/ρ unchanged, and preserves the dust force equation when the prescribed F,U are held fixed. Maxwell's sourced equation must still match the scaled current. If instead both F and j are scaled by η, the sourced Maxwell system is linear but electromagnetic stress scales as η2 while dust stress scales as η; these degree differences provide no general coupled-solution family.

Finally, for a fixed Q≠0 and ℓ>0, prescribe only on the finite Minkowski annulus Aℓ={x:ℓ<∣x∣<2ℓ} the radial electric field E=Q(4πε0r2)−1er, B=0. Its field energy on that annulus is Q2/(16πε0ℓ) and diverges as ℓ↓0. This calculation defines no field or source at the origin and supplies no point-charge construction or regularization theorem.

Facts & Assumptions

Given: The smooth fixed-background physical interpretation of Separately adopted fixed-background Maxwell and charged probes, the formal SI tensor definitions of Smooth matter quantities, current and observer observables, a fixed vacuum metric and smooth source-free two-form for the source-free clause, a smooth sourced pair (F0,j0) for the sourced clause, a positive-density dust region for the dust-scaling clause, and the stated finite-annulus profile for the final clause.

[F1]

Separately adopted fixed-background Maxwell and charged probes: the metric and Maxwell data may be prescribed independently; the source-free equations are dF=0, d(⋆gF)=0, while the sourced equations are dF=0, ∇aFab=−μ0jb for a separately prescribed current. No Einstein equation for the unchanged background or probe/source backreaction is part of this test-model postulate.

[F2]

Smooth source/dust scaling and test-backreaction obstructions: its separate positive-density charged-dust/current scaling clause and prescribed finite Coulomb-annulus energy clause have their displayed hypotheses. These are the clauses used below. Its first source-free clause assumes dF0=0 and ∇a(F0)ab=0; that clause is not applied to the model's differential-form assumptions here. Instead, both Maxwell scaling/residual branches and the pointwise nonzero-energy obstruction are proved directly below. None is a nearby-solution estimate.

[F3]

Smooth matter quantities, current and observer observables: TEMab=μ0−1(FacFbc−14gabFcdFcd), TabEM=gacgbdTEMcd, ε0=(μ0c2)−1, κ=8πGN/c4>0, charged dust has Tmab=ρUaUb and ja=σUa, and observer energy is Tabnanb for each future unit observer n.

[F4]

Lorentzian exterior calculus and Hodge star, Statement: for the given fixed oriented Lorentzian geometry, (⋆gF)ab=12(volg)abcdFcd, and exterior differentiation has its alternating coordinate derivative formula. Consequently metric raising and this Hodge formula are real-linear in F when g is fixed, and d commutes with multiplication by a constant real scalar. Neither formula assumes a Maxwell equation or a current.

[A1]

The vacuum metric, each Maxwell solution, the dust data, and the annulus profile are independent assumptions of their respective clauses. In the sourced-pair clause the current is prescribed, and its matter stress is not part of the stated electromagnetic residual. No source is extended to the origin and no coupled family is assumed to exist.

Proof

1.1givenF1F3F4A1algebra

Since δ is a constant real scalar, the component Hodge formula in [F4] with the fixed inverse metric gives ⋆gFδ=δ⋆gF0, and the coordinate exterior derivative formula gives dFδ=δdF0=0 and d(⋆gFδ)=δd(⋆gF0)=0. Thus Fδ satisfies exactly the source-free differential-form equations in [F1], without inferring or assuming a sourced divergence equation. Every term in [F3]'s electromagnetic stress is quadratic in F and index raising/lowering is linear for fixed g, so TEM(g,Fδ)=δ2TEM(g,F0). Substituting the vacuum equation G(g)+Λg=0 gives R(g,Fδ;Λ)=−κδ2TEM(g,F0). Since κδ2≥0, componentwise absolute-value homogeneity gives the asserted fixed-chart norm identity, with both norms zero for empty K. This includes δ=0 and negative δ and uses no form/divergence equivalence.

1.2F1F3F4A1algebra

By the real-linearity of d and ∇ and the prescribed sourced equation in [F1], dFδ=δdF0=0 and ∇a(Fδ)ab=δ∇a(F0)ab=−μ0δj0b=−μ0jδb. Every term of the tensor in [F3] is quadratic in F, so TEM(g,Fδ)=δ2TEM(g,F0). Using G(g)+Λg=0 in the definition of R gives the stated identity; componentwise homogeneity of the maximum norm gives the compact-chart norm identity, including the empty-set convention. This residual includes no source-matter stress.

1.3F2F3A1algebra

On ρ>0, (ησ)/(ηρ)=σ/ρ. The exact force-equation and sourced-Maxwell qualifications, linear dust/current scaling, and mismatch between the η and η2 stress scalings are the corresponding clauses proved in [F2] for the matter forms defined in [F3]. Thus these rescalings alone do not establish a coupled solution family.

2.1F3step 1.1step 1.2algebra

At a point where F0≠0, take any future unit observer n and a positively oriented orthonormal rest frame. In this frame write (F0)0i=−Ei/c and (F0)ij=ϵijkBk. Raising indices with diag⁡(−1,1,1,1) gives (F0)ab(F0)ab=2(∣B∣2−∣E∣2/c2); substitution in the stress formula [F3] then gives TabEM(g,F0)nanb=(∣E∣2/c2+∣B∣2)/(2μ0). The six components determine F0, so E,B cannot both vanish, and the energy is strictly positive because μ0,c>0. This pointwise algebra uses no Maxwell equation and therefore applies in both the source-free and sourced branches. For δ≠0, the residual in step 1.1 or 1.2 is nonzero because κδ2>0 and this observer contraction of TEM(g,F0) is nonzero. In the source-free case this excludes the unchanged-metric vacuum Einstein–Maxwell solution; in the sourced case it excludes only vanishing of the defined residual without matter stress, and says nothing about other metrics or source matter.

3.1F2F3A1algebra∎

On Aℓ, the SI field-energy density is ε0∣E∣2/2=Q2/(32π2ε0r4) by [F3]. Polar coordinates on this finite annulus give Eℓ=4π∫ℓ2ℓ(Q2/(32π2ε0r4))r2 dr=(Q2/(8πε0))∫ℓ2ℓr−2 dr=Q2/(16πε0ℓ), using the annulus calculation supplied by [F2]. This diverges at fixed nonzero Q as ℓ↓0, while every field evaluation remains on r>ℓ>0; no field, source, or point limit at r=0 is asserted.

Depends on

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