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Geometric electrovac equations and flux normalization — Examples

1 · Prerequisites

2 · Summary

This companion records exact parameter substitutions and counterexamples for the geometric electrovac page. The zero-rotation limits identify coordinate forms only; equal metric coefficients do not determine the sign of electric flux, and zero scalar curvature does not force zero Ricci curvature. Every entry is a mathematical model deduction, not a reported observation.

3 · Logical flowchart

4 · Definitions, postulates, theorems and proofs

None yet.

5 · Examples, experiments and counterexamples

ExampleConstruction: AI-adaptedVerification: AI-adaptedjudge pass (gpt-6-luna)Open item page →

Zero-rotation and zero-charge metric substitutions

Example

Consider the exact Kerr-Newman metric and potential on a pole-free domain with Σ>0 and Δ≠0. Its three parameter substitutions give the Reissner-Nordström, vacuum Kerr, and Schwarzschild metric forms as follows. At zero rotation the RN coordinate formulas agree for every admitted r≠0; identification with the RN datum defined here uses only the common positive-radius pole-free domains.

Facts & Assumptions

Given: The electric KN and RN data and their verified field equations, with M,a,q real length parameters.

[F1]

Fully verified electric Kerr-Newman electrovacuum: the KN metric and potential satisfy the source-free geometric equations on their common domain.

[F2]

Dyonic Reissner-Nordström metric and field domains: the electric RN specialization has f=1−2M/r+q2/r2 and potential −q dx0/r when qe=q and qm=0.

[F3]

The Schwarzschild exterior model datum: domain, metric, mass parameter and time orientation: with Schwarzschild radius s=2GNm∗/c2, the exterior metric function is 1−s/r on r>s.

Verification

1.1F1F2algebra

Set a=0 and retain the electric parameter q. Then Σ=r2, Δ=r2−2Mr+q2, and the KN line element reduces term by term to −(1−2Mr+q2r2)(dx0)2+(1−2Mr+q2r2)−1dr2+r2dΩ2. Its potential becomes −q dx0/r. For every open J⊂(0,∞) on which f=Δ/r2≠0, the resulting metric, potential and field on the common pole-free chart are the restrictions of the electric RN datum with qe=q,qm=0 in [F2]. When r<0 is admitted by the KN definition, the same coordinate expressions hold, but that chart is outside the positive-radius RN datum in [F2]. No global-domain equality or uniqueness theorem is used.

1.2F1algebra

Set q=0 with a arbitrary. The potential and field vanish, while Δ=r2−2Mr+a2 and the displayed metric is the vacuum Kerr form. Since the KN residual identity of [F1] remains valid at q=0, its Ricci tensor vanishes. This is the vacuum rotating limit, not a classification claim.

2.1F1F3algebra∎

Set both a=0 and q=0. On the component M>0 and r>2M, the metric function is 1−2M/r. With s=2M and m∗=c2M/GN, [F3] identifies it with the Schwarzschild exterior metric form. The conclusion is only the coordinate substitution and local metric identity.

ExampleConstruction: AI-adaptedVerification: AI-adaptedOpen item page →

Opposite electric charges give the same RN metric

Example

Fix a length ℓ>0 and a real mass parameter M. On any positive-radius interval where the two functions f±(r)=1−2M/r+ℓ2/r2 are nonzero, compare the pure electric RN data with qe=+ℓ and qe=−ℓ.

Facts & Assumptions

Given: The dyonic RN formula with qm=0 and the same M,r domain in both cases.

[F1]

Dyonic Reissner-Nordström metric and field domains: f=1−2M/r+(qe2+qm2)/r2 and F=−qer−2dx0∧dr+qmωS2.

[F2]

Lorentzian exterior calculus and Hodge star: on a positively oriented Lorentzian orthonormal coframe, the two-form Hodge map is determined by the metric and orientation and satisfies ⋆(e0∧e1)=−e2∧e3.

[F3]

A continuous function on [a,b] is Riemann integrable, by Heine-Cantor and Riemann's criterion makes a continuous real function on a compact interval Riemann integrable. The second fundamental theorem: if G is differentiable on [a,b] with G′=f and f is integrable, then ∫abf=G(b)−G(a) evaluates its integral as G(b)−G(a) when the integrand is the derivative of a differentiable primitive G.

[F4]

Geometric electrovac equations and flux normalization defines sphere flux by pulling back the smooth field or its Hodge dual along a smooth embedding of a compact oriented sphere and integrating the resulting top form. The integral uses the inherited ACω convention; the flux parameter is the integral divided by 4π.

Verification

1.1F1algebra

Since (+ℓ)2=(−ℓ)2, both lapse functions equal 1−2M/r+ℓ2/r2. Every metric coefficient is consequently identical.

2.1F1F2F3F4step 1.1algebra∎

At fixed x0 and admitted radius r>0, the sphere map u↦(x0,r,u) from the oriented unit sphere into the RN product is a smooth embedding; it is a product-factor inclusion, so it is injective with injective differential and has the continuous inverse given by the sphere projection. The source sphere is compact and has no boundary, and the fields are smooth on a neighborhood since r>0 and f(r)≠0. Thus its pulled-back field and dual are smooth compactly supported top forms, and the flux integrals below are the well-defined operation in [F4]. The two fields are F±=∓ℓr−2dx0∧dr, so F−=−F+. If f>0, use the positively oriented coframe e0=f dx0, e1=f−1/2dr, e2=r dθ, e3=rsin⁡θ dϕ. If f<0, use e0=(−f)−1/2dr, e1=−(−f)1/2dx0, e2=r dθ, e3=rsin⁡θ dϕ. In both cases dx0∧dr=e0∧e1 and e2∧e3=r2ωS2, so [F2] gives ⋆g(dx0∧dr)=−r2ωS2 and ⋆gF±=±ℓ ωS2. For the explicit sphere parametrization s(θ,ϕ)=(sin⁡θcos⁡ϕ,sin⁡θsin⁡ϕ,cos⁡θ), differentiation gives s⋅(sθ×sϕ)=sin⁡θ, so the outward form pulls back to sin⁡θ dθ∧dϕ, as in [F1]. The sine density is continuous, hence integrable by [F3]; its primitive is −cos⁡θ. Its integral on δ≤θ≤π−δ, 0≤ϕ≤2π is 4πcos⁡δ, and the two omitted caps have total area 4π(1−cos⁡δ)→0 by the same bounded polar density; the seam has zero width in the azimuthal integral. Thus ∫S2ωS2=2π[−cos⁡θ]0π=4π. The normalized oriented electric sphere fluxes are therefore (4π)−1∫Sr⋆gF±=±ℓ. Thus the metric does not determine the sign of the electric flux parameter.

CounterexampleConstruction: AI-adaptedVerification: AI-adaptedjudge pass (gpt-6-luna)Open item page →

Zero scalar curvature does not imply vacuum Ricci

Statement refuted

For every four-dimensional Lorentzian metric, scalar curvature S=0 implies Ric⁡=0.

Counterexample instance

Let ℓ>0, set M=0, qe=ℓ, qm=0, and choose the RN datum on a small open interval about r=2ℓ. Then f=1+ℓ2/r2 is positive there, so the metric is smooth Lorentzian and nondegenerate.

Facts & Assumptions

Given: The RN metric and curvature formulas for r>0 and f≠0.

[F1]

Exact Reissner-Nordström Ricci and curvature identities: S=0 and Ric⁡22=Q2/r2 for the dyonic RN datum.

[A1]

ℓ>0, M=0, qe=ℓ, qm=0, and r=2ℓ lies in the selected positive-radius interval.

Verification

1.1A1F1algebra

At r=2ℓ, Q2=ℓ2 and Ric⁡22=Q2/r2=1/4≠0, while [F1] gives S=0. By continuity the same nonvanishing holds on a sufficiently small open neighborhood of that radius.

2.1F1step 1.1algebra∎

The hypotheses of the refuted statement hold on this smooth RN chart but its conclusion fails because the displayed Ricci component is nonzero. Hence the universal implication is false.

Sources