Suppose, for contradiction, that every future null geodesic orthogonal to the compact trapped surface extends beyond . Both families begin with expansion at most , so part d gives a point conjugate to on every generator by affine length . A generator of the achronal boundary cannot remain on that boundary beyond its first conjugate point, because afterward it can be deformed to a timelike curve from .
The two bundles of initial null directions over compact , restricted to , form a compact set. Their image under the geodesic exponential map contains all of , so this achronal boundary is compact. Project it along a complete timelike flow onto the noncompact Cauchy hypersurface . The projection is both open and closed in the connected Cauchy surface, hence would be all of ; compactness of the source would then make compact, a contradiction.
Therefore at least one orthogonal future null geodesic cannot extend to affine length . Its maximal future development is future-inextendible with total affine length
which is the incompleteness conclusion of the Penrose singularity theorem.
The second law of black-hole mechanics states that, assuming the null energy condition and the usual predictability hypotheses, the area of cross-sections of a future event horizon never decreases toward the future.
Indeed, the horizon generators form a hypersurface-orthogonal null congruence, so their twist vanishes. If the expansion were negative anywhere, the null focusing theorem would make it diverge to within finite affine parameter, provided the generator extends that far. This produces a conjugate point, after which the generator cannot remain on an achronal set such as an event horizon. Future completeness rules out the alternative that the generator simply ends first. Therefore everywhere, and