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ExampleConstruction: Literature-sourcedVerification: AI-generatedPipeline-generatedprecheck passverified 2026-10-22 (gpt-6.1-sol)
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Round spheres in Minkowski spacetime

Physical scope

Pure mathematical Minkowski example; no observation or field equation is used.

Statement

Take M=R×R3 with length-valued coordinates (t,x), Lorentzian metric g=−dt2+dx2, and time orientation N=∂t. For x≠0, set r:=∣x∣ and ∂r:=∑i=13(xi/r)∂xi. For R>0, let S={(0,Rω):ω∈S2}. The future null normals ℓ=∂t+∂r and k=∂t−∂r satisfy g(ℓ,k)=−2 and have expansions θℓ=2R,θk=−2R. Along the inward congruence generated by k, the screen Jacobi map is Aλ=(1−λ/R)id⁡, so its first focal instant is λ=R. The affine focusing bound from Null Raychaudhuri and focal-point bound is attained, and every point γω(λ)=(λ,(R−λ)ω) with R<λ<3R lies in I+(S).

Facts & Assumptions

Given: The Minkowski metric, sphere radius R>0, null normals and congruence specified in the Statement.

[F1]

On the positive screen, χℓ(X,Y)=g(∇Xℓ,Y), θ=tr⁡qχ, and the screen Jacobi map detects focal instants (Null normal pairs and screen geometry).

[F2]

Under Countable Choice for its Lorentzian supplier conventions, an affine twist-free null congruence satisfies θ′=−θ2/2−∣σ∣2−Ric⁡(ℓ,ℓ); under Ric⁡(ℓ,ℓ)≥0 and θ(0)<0, the focal bound is 2/∣θ(0)∣, provided the smooth congruence and generator exist through that comparison parameter (Null Raychaudhuri and focal-point bound).

[F3]

Under Countable Choice and Dependent Choice, a focal point on a future null normal generator is followed immediately by points of its unique geodesic extension in I+(S) (Null focal points exclude later horismos generators).

[A1]

Coordinates are length-valued, N=∂t fixes the future time orientation, R and λ are measured in metres, and no field equation or physical energy condition is assumed.

Proof

Given: [F1]–[F3] and [A1].

1.1A1F1constructalgebra

On S, q=R2dΩ2. For tangent X,Y, flat-space differentiation gives ∇X∂r=X/R and ∇X∂t=0. Therefore χℓ=q/R and χk=−q/R, and since the screen dimension is two, θℓ=2/R and θk=−2/R. Direct inner products give g(ℓ,ℓ)=g(k,k)=0 and g(ℓ,k)=−1−1=−2; both fields are future because their t components are 1.

2.1A1F1F2step 1.1algebra

In Cartesian coordinates the inward geodesic is γω(λ)=(λ,(R−λ)ω). Varying ω in a tangent direction X∈TRω(RS2) gives the Jacobi field JX(λ)=(1−λ/R)X. Its screen map is therefore Aλ=(1−λ/R)id⁡ for 0≤λ<R, with first rank loss at R. Hence B=−id⁡/(R−λ), θ=−2/(R−λ), σ=0, and Ric⁡=0. Differentiating θ verifies the displayed equation directly, and 2/∣θ(0)∣=2/(2/R)=R. Thus the explicit focal parameter equals the comparison value; under its Countable Choice convention, [F2] gives the same sharp bound.

3.1A1F3step 2.1algebra∎

Fix R<λ<3R. The point p−=(0,−Rω)∈S and qλ=γω(λ) have time separation λ and spatial separation ∣(R−λ)ω−(−Rω)∣=∣2R−λ∣<λ. The straight segment from p− to qλ is future timelike because its time component is positive and its squared interval is −λ2+(2R−λ)2<0. Thus qλ∈I+(S). Under Countable Choice and Dependent Choice this also agrees with [F3] for parameters sufficiently close to R; the displayed segment proves the stronger stated range R<λ<3R directly, without either choice assumption.

Remarks

The two signs distinguish the outward and inward future null directions; the negative expansion corresponds to the inward congruence and its focal radius R. The example is a flat-space calculation, not an empirical claim.

Depends on

Dependency tree · 2 levels

Sources