Locally write the null hypersurface as a level set and its normal as . Since a null normal is also tangent, lies within the hypersurface. The symmetry of the Levi-Civita connection gives
The scalar vanishes on the hypersurface, so its gradient there is normal and hence proportional to :
This is the nonaffine geodesic equation. A rescaling of removes , proving that the null hypersurface normal generates null geodesics lying in the hypersurface.
Let be the affine null tangent and choose another null vector with . The screen-space projector
projects onto the -dimensional transverse space. The optical tensor is
Its irreducible decomposition defines
the null expansion,
the null shear, and
the null twist, also called rotation.
Affine geodesic evolution and the Ricci identity give the screen-projected optical equation
Taking the screen trace yields
The optical decomposition and the antisymmetry of imply
Therefore the -dimensional Null Raychaudhuri equation is
and the requested constant is .
For generators of a null hypersurface, the Frobenius theorem gives . The null energy condition and the Einstein field equations imply , while the shear norm is nonnegative. With , Raychaudhuri's equation gives
As long as remains finite,
If , integration gives
The right-hand side reaches zero at , which a finite negative cannot cross. Hence the null focusing theorem forces
provided the generator extends that far.
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.

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