In the two null coordinates the inverse metric has and . ThereforeBoth tangents are null and future-directed, since and both coordinate directions are future-directed. To prove the affine parameter property, use the null-gradient affine-geodesic identity. The one-form is closed, so . ConsequentlyThe same argument applies to . Thus both vector fields satisfy the geodesic equation without a nonaffinity term, and generate affinely parametrized null geodesic congruences. The coordinate vectors alone need not be affine; the factors are essential.
For the spherical null expansions in double-null coordinates, the cross-sectional area of a symmetry sphere is . For the two affine null geodesic congruences, the definition of null expansion therefore givesThere is no extra derivative of in these formulas: the null expansion differentiates the transverse area, not the normalization of the tangent. Equivalently, the projected metric is and its optical tensor is , or for the other congruence. It is purely trace, so both null shears vanish.
The null twist vanishes because the covector tangents are gradients of and , and hence their exterior derivatives vanish. Each congruence is orthogonal to a family of null hypersurfaces. This also identifies the Frobenius theorem reason for zero null twist.
Use the Null Raychaudhuri equation for . Its null shear and null twist vanish, and . Substitution of givesThe quadratic terms cancel. Thus the double-null focusing identity isHere the last equality uses the Einstein field equations in units ; terms proportional to the metric vanish in this null component. The inequality follows from the null energy condition.
For any point of the future domain of dependence , the past continuation of its generator must meet the Cauchy hypersurface : every past-inextendible causal curve from that point meets . Along its future continuation, increases, and is nonincreasing by the focusing identity. Its initial value is negative, so it stays negative. Since , throughout the regular part of . The argument is used only where the smooth double-null chart has ; it does not extend a congruence beyond a singular endpoint.
A spherical trapped surface has both future null expansions negative. Thus the initial sphere has and . The result of the previous part already gives at every regular future sphere in .
Apply the same Null Raychaudhuri equation to . The exchanged-coordinate double-null focusing identity isAlong , increasing is future-directed. ThereforeBoth null expansions remain negative, proving persistence of spherical trapping along this future null direction. As usual, the conclusion concerns every for which the sphere exists in the regular chart in ; the inequality does not assert existence of such spheres beyond a focusing singularity.
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