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Theorem 3 (Wall 2013): null generators with decreasing generalized entropy terminate

Proved
WallGSL.null_generator_terminates

by Lucas · Oct 4, 2026 · Mathlib 0df444a (Lean v4.33.1)

general-relativitygeneralized-second-law

Theorem 3. Let (M,g)(M,g)(M,g) be a time-oriented Lorentzian spacetime (C∞C^\inftyC∞, Hausdorff, second countable) with a generalized entropy SgenS_{\rm gen}Sgen​. Let NNN be an achronal null surface with exterior region XXX, and let g0g_0g0​ be a point at which the fine-grained generalized entropy of XXX is decreasing: there is a Cauchy surface Σ∋g0\Sigma\ni g_0Σ∋g0​ such that for every neighbourhood UUU of g0g_0g0​ the slice can be pushed forwards in time inside UUU to Σ′\Sigma'Σ′ with

Sgen(Σ′∩X)<Sgen(Σ∩X).S_{\rm gen}(\Sigma'\cap X)<S_{\rm gen}(\Sigma\cap X).Sgen​(Σ′∩X)<Sgen​(Σ∩X).

Assume the semiclassical approximation holds near g0g_0g0​ (in the form of the comparison principle of Theorem 1 at g0g_0g0​) and the fine-grained GSL holds. Then no future-directed null geodesic ray WWW starting at g0g_0g0​ with infinite affine parameter stays on NNN forever:

W([a,∞))⊈N.W([a,\infty))\not\subseteq N.W([a,∞))⊆N.

Equivalently, the null generator through g0g_0g0​ must terminate when traced towards the future, either because it exits NNN or because spacetime is null geodesically incomplete.

This is the thermodynamic half of the singularity theorem: the GSL forbids a surface whose generalized entropy decreases from being a horizon.

Formalization Note Achronality of NNN is the property of null surfaces (boundaries of past or future sets) that the paper's proof uses when it states that the horizon HHH lies on or to the past of NNN.

Preamble
import Definitions.Def_WallGSL_GeneralizedEntropy

open scoped Manifold Topology ContDiff
open Set
Formal statement
namespace WallGSL

/-- Theorem 3 of Wall (2013): if the fine-grained generalized entropy outside the
achronal null surface `N` is decreasing at `g₀`, the semiclassical comparison of
Theorem 1 holds at `g₀`, and the fine-grained GSL holds, then no future-directed null
geodesic ray starting at `g₀` with infinite affine parameter stays on `N` forever. -/
theorem null_generator_terminates
    {E : Type*} [NormedAddCommGroup E] [InnerProductSpace ℝ E] [FiniteDimensional ℝ E]
    {M : Type*} [TopologicalSpace M] [T2Space M] [SecondCountableTopology M]
    [ChartedSpace E M] [IsManifold 𝓘(ℝ, E) ∞ M]
    (st : LorentzianMetric E M) (Sgen : Set M → ℝ) (N X : Set M) (g₀ : M)
    (hN : st.IsAchronal N)
    (hdec : st.EntropyDecreasingAt Sgen X g₀)
    (hSC : st.TheoremOneComparisonAt Sgen N X g₀)
    (hGSL : st.FineGrainedGSL Sgen)
    (W : ℝ → M) (a : ℝ) (hW : st.IsFutureInfiniteNullRay W a) (hWa : W a = g₀) :
    ¬ (W '' Ici a ⊆ N) := by sorry

end WallGSL
Source
A. C. Wall, The generalized second law implies a quantum singularity theorem, Class. Quantum Grav. 30 (2013) 165003, https://doi.org/10.1088/0264-9381/30/16/165003, §3.2, Theorem 3, pp. 14–15
Read-back

What the Lean code literally says, in plain math · Aristotle (Harmonic) - same agent as the drafter; non-blind

Provenance note — this read-back is NOT blind. It was written by the same agent (Aristotle, by Harmonic) that drafted the Lean statements, with full knowledge of the source paper and of the intended meaning. It is therefore not independent testimony and must not be mistaken for a blind audit; reviewers should treat it as the drafter's own literal reading of the code and compare it against the source themselves.

Data. EEE, MMM (Hausdorff, second countable, C∞C^\inftyC∞ manifold modelled on EEE), a time-oriented Lorentzian metric (g,τ)(g,\tau)(g,τ), an arbitrary function SgenS_{\rm gen}Sgen​ from subsets of MMM to R\mathbb RR, subsets N,X⊆MN,X\subseteq MN,X⊆M, a point g0∈Mg_0\in Mg0​∈M, a curve W:R→MW:\mathbb R\to MW:R→M and a real number aaa.

Hypotheses.

  1. NNN is achronal: no p,q∈Np,q\in Np,q∈N with p≪qp\ll qp≪q.
  2. The entropy is decreasing at g0g_0g0​ for XXX: some Cauchy surface Σ∋g0\Sigma\ni g_0Σ∋g0​ has, for each neighbourhood UUU of g0g_0g0​, a Cauchy surface Σ′\Sigma'Σ′ with Σ′∖U=Σ∖U\Sigma'\setminus U=\Sigma\setminus UΣ′∖U=Σ∖U, Σ′⊆J+(Σ)\Sigma'\subseteq J^+(\Sigma)Σ′⊆J+(Σ) and Sgen(Σ′∩X)<Sgen(Σ∩X)S_{\rm gen}(\Sigma'\cap X)<S_{\rm gen}(\Sigma\cap X)Sgen​(Σ′∩X)<Sgen​(Σ∩X).
  3. The Theorem-1 comparison holds at g0g_0g0​ for (N,X)(N,X)(N,X) (as defined in WallGSL_GeneralizedEntropy: for each observer W′W'W′ from a′a'a′ with R=I−(W′([a′,∞)))R=I^-(W'([a',\infty)))R=I−(W′([a′,∞))), if N∩R=∅N\cap R=\emptysetN∩R=∅ and a future-null geodesic segment from g0g_0g0​ lies in N∩∂RN\cap\partial RN∩∂R, then decreasing at g0g_0g0​ for XXX implies decreasing at g0g_0g0​ for RRR).
  4. The fine-grained GSL holds (for every observer and Cauchy surfaces Σ′⊆J+(Σ)\Sigma'\subseteq J^+(\Sigma)Σ′⊆J+(Σ), Sgen(Σ∩R)≤Sgen(Σ′∩R)S_{\rm gen}(\Sigma\cap R)\le S_{\rm gen}(\Sigma'\cap R)Sgen​(Σ∩R)≤Sgen​(Σ′∩R)).
  5. WWW is a future-infinite null ray from aaa: a geodesic on (a,∞)(a,\infty)(a,∞), right-continuous at aaa, with future-null velocity for all t>at>at>a.
  6. W(a)=g0W(a)=g_0W(a)=g0​.

Conclusion. It is not the case that W(t)∈NW(t)\in NW(t)∈N for all t≥at\ge at≥a.

There is no hypothesis relating XXX to NNN, and NNN is not required to be a null hypersurface beyond being achronal.

Human review
  • Endorsed by Shuze Chen · Oct 8, 2026

    Confirmed by the moderator at approval.

  • Endorsed by Lucas · Oct 8, 2026

    Confirmed by the mission captain (proposal self-audit).

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