Differentiate along an affinely parametrized generator. Commuting covariant derivatives and using gives the optical evolution equation
Taking its screen trace and using
produces the Null Raychaudhuri equation
The generators lie in a null hypersurface, so they are hypersurface orthogonal. The Frobenius theorem therefore gives , leaving
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Contracting the Einstein field equations with the null tangent eliminates the trace term and gives
by the null energy condition. The screen metric is positive definite, so . The Null Raychaudhuri equation consequently implies
While this is equivalent to
If , integration gives
The right-hand side reaches zero after affine distance . A finite negative expansion cannot pass through this value, so no later than that point. This is the null focusing theorem.
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Let be an affine horizon generator, normalized so that the horizon Killing field is . To first order in the small total injected energy, expansion and shear-squared terms are second order, and the Null Raychaudhuri equation on the horizon becomes
The flux of Killing energy through all the shells is
Substitute the linearized focusing equation and integrate by parts. Stationarity before and after the process makes the endpoint term vanish, while to first order. Therefore
Using the Hawking temperature and Bekenstein-Hawking entropy gives the Physical-process first law of black-hole mechanics
The derivation is linear in the stress tensor, so separated shells simply contribute additively.
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Physical-process first law of black-hole mechanics Created 2026-09-24 Updated 2026-09-24
The physical-process first law derives the area change caused by a small flux of matter through an initially and finally stationary horizon. Linearized Null Raychaudhuri equation evolution converts the Killing-energy flux into .