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 givesThe 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 projectorprojects onto the -dimensional transverse space. The optical tensor isIts irreducible decomposition definesthe null expansion,the null shear, andthe null twist, also called rotation.
Affine geodesic evolution and the Ricci identity give the screen-projected optical equationTaking the screen trace yieldsThe optical decomposition and the antisymmetry of implyTherefore the -dimensional Null Raychaudhuri equation isand 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 givesAs long as remains finite,If , integration givesThe right-hand side reaches zero at , which a finite negative cannot cross. Hence the null focusing theorem forcesprovided 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 lengthwhich is the incompleteness conclusion of the Penrose singularity theorem.
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