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Penrose null geodesic incompleteness
A conditional Lorentzian-geometric theorem. The null Ricci inequality is assumed directly; no Einstein equation, matter-energy condition, event horizon, curvature blow-up, or singular point in the manifold is concluded.
Statement
Assume the Axiom of Choice. Let be a smooth time-oriented Lorentzian four-manifold of signature that is globally hyperbolic (strongly causal with compact causal diamonds). Let be a connected noncompact smooth spacelike Cauchy hypersurface, meaning that every inextendible causal curve meets exactly once. Let be a nonempty compact smooth spacelike two-surface on which both future null expansions are negative for the two local future null normal rays. Assume directly that for every point and every null vector . Then is future null geodesically incomplete: at least one maximal future-directed affinely parametrized null geodesic has an affine parameter interval with finite upper endpoint. This conclusion asserts no curvature divergence or singular point belonging to .
Statement references
Chronology, causality, strong causality, global hyperbolicity and time functions
Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons
Trapping and the asymptotic black-hole region
Future null geodesic completeness and incompleteness
Future null geodesic completeness and incompleteness
Compactness of the future horismos under null completeness
A complete temporal flow identifies smooth Cauchy slices
Temporal functions are time functions, and time functions forbid closed causal curves
Existence of a positive smooth volume density of total mass one on a smooth Lorentzian four-manifold
Facts & Assumptions
Given: Axiom of Choice; a globally hyperbolic time-oriented smooth Lorentzian four-manifold; a connected noncompact smooth spacelike Cauchy hypersurface ; a compact future trapped surface ; and the pointwise null Ricci inequality.
The Axiom of Choice: AC is the assertion that every family of nonempty sets has a choice function.
AC implies DC implies countable choice: in ZF, , so the Countable Choice and Dependent Choice hypotheses of the causal suppliers follow from [A1].
Existence of a positive smooth volume density of total mass one on a smooth Lorentzian four-manifold, The Geroch volume function: a continuous strictly increasing time function whose levels are Cauchy sets, and Smooth Cauchy temporal splitting: a global temporal function with Cauchy levels and an orthogonal complete flow: under Countable Choice and Dependent Choice, a nonempty time-oriented smooth Lorentzian four-manifold has a normalized smooth volume measure; global hyperbolicity and that measure give the volume time input required by the splitting theorem; the latter then gives a smooth temporal function with Cauchy levels and a complete future timelike flow diffeomorphism satisfying .
A complete temporal flow identifies smooth Cauchy slices: for this complete timelike product flow, projection along its flow lines identifies any smooth spacelike Cauchy hypersurface diffeomorphically with the slice . Thus is connected and noncompact.
Compactness of the future horismos under null completeness: under the stated trapped-surface, null Ricci, global-hyperbolicity, and future-null-completeness assumptions, is a compact topological three-manifold without boundary.
Achronal boundaries are locally Lipschitz graphs, topological hypersurfaces and null for smooth volume densities: the boundary of an open future set is achronal; in particular no two distinct points of are chronologically related.
Temporal functions are time functions, and time functions forbid closed causal curves: a temporal function strictly increases along every nonconstant future causal curve, hence along every future timelike curve.
Invariance of domain: assuming AC, a continuous injective map between open subsets of has open image; applying this in charts makes a continuous injective map between topological three-manifolds an open map.
A continuous image of a compact space is compact; a continuous real-valued map on a nonempty compact space attains a maximum and a minimum; and a continuous bijection from a compact space to a Hausdorff space is a homeomorphism: a continuous real-valued map on a nonempty compact space attains its minimum, and a continuous image of a compact space is compact.
In a Hausdorff space a point and a disjoint compact set, and two disjoint compact sets, have disjoint open neighbourhoods; hence every compact subset is closed, and in a compact Hausdorff space the compact subsets are exactly the closed ones and Separation of a topological space, connected and disconnected spaces, clopen sets, and connected subsets: compact subsets of a Hausdorff space are closed, and a nonempty subset that is both open and closed in a connected space is the whole space.
Future null geodesic completeness and incompleteness: future null geodesic incompleteness means the existence of a maximal future null affine interval with finite upper endpoint.
The inequality for null is a direct mathematical premise. It is not derived from a matter model, energy condition, or Einstein equation.
Proof
Given: [A1]–[A2] and [F1]–[F10]. Assume, for contradiction, that every future-directed null geodesic is future complete.
Assume for contradiction that every future-directed null geodesic is future complete. By [F1], Countable Choice and Dependent Choice hold under the assumed Axiom of Choice, so the hypotheses of the volume-time, Cauchy-splitting and causal-boundary suppliers are satisfied.
Apply [F2] to obtain a volume time input, a temporal function , a smooth Cauchy slice , and a complete timelike product flow . The splitting satisfies . Hence tends to and along the two ends of every orbit; continuity prevents an endpoint in , so each orbit is an inextendible timelike curve.
Apply [F3] to identify the given hypersurface diffeomorphically with by projection along these flow lines. Therefore is connected and noncompact.
The restriction is continuous and is nonempty compact, so [F8] gives a point at which is minimal. If , some satisfies ; since is temporal, [F6] gives , contradicting minimality. Thus . As by reflexivity, , so this boundary is nonempty.
Define by . This is continuous because is smooth. If have and , their flow coordinates differ, so the timelike orbit between them makes them chronologically related. This contradicts the achronality in [F5]. Hence is injective.
The domain is a topological three-manifold without boundary by [F4], and is a smooth three-manifold by [F2]. For each , choose manifold charts about and and shrink the source chart so its image lies in the target chart. In these coordinates is continuous and injective between open subsets of ; [F7] makes its image open. Taking the union over shows is open in .
By [F4], is compact, and is continuous, so [F8] makes compact. The smooth manifold is Hausdorff; [F9] therefore makes this image closed in .
The image is nonempty by step 3.2 and both open and closed by steps 4.1 and 4.2. Since is connected by step 3.1, [F9] implies . But is compact by step 4.2, which would make compact, contradicting step 3.1. Thus the assumed future null completeness is false. By [F10], at least one maximal future-directed null geodesic has finite upper affine endpoint, which is the asserted conclusion.
Remarks
The null Ricci condition is a geometric hypothesis in the library curvature convention; it is not silently replaced by an Einstein equation or a matter energy condition. The conclusion is affine incompleteness only. It neither identifies an incomplete endpoint inside nor asserts curvature blow-up, cosmic censorship, or the existence of an event horizon. A trapped surface is not itself an event horizon; that comparison requires separate asymptotic and global hypotheses.
Depends on
The Axiom of Choice
AC implies DC implies countable choice
Chronology, causality, strong causality, global hyperbolicity and time functions
Causal curves, chronological and causal reachability, and inextendibility
Future sets, past sets, achronal boundaries and their elementary properties
Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons
Future null geodesic completeness and incompleteness
Trapping and the asymptotic black-hole region
Achronal boundaries are locally Lipschitz graphs, topological hypersurfaces and null for smooth volume densities
A complete temporal flow identifies smooth Cauchy slices
Compactness of the future horismos under null completeness
Temporal functions are time functions, and time functions forbid closed causal curves
Existence of a positive smooth volume density of total mass one on a smooth Lorentzian four-manifold
Smooth Cauchy temporal splitting: a global temporal function with Cauchy levels and an orthogonal complete flow
The Geroch volume function: a continuous strictly increasing time function whose levels are Cauchy sets
Invariance of domain
A continuous image of a compact space is compact; a continuous real-valued map on a nonempty compact space attains a maximum and a minimum; and a continuous bijection from a compact space to a Hausdorff space is a homeomorphism
In a Hausdorff space a point and a disjoint compact set, and two disjoint compact sets, have disjoint open neighbourhoods; hence every compact subset is closed, and in a compact Hausdorff space the compact subsets are exactly the closed ones
Hausdorff space: distinct points have disjoint open neighbourhoods; every metrizable space is Hausdorff and the indiscrete topology on two points is not
Separation of a topological space, connected and disconnected spaces, clopen sets, and connected subsets
Dependency tree · 2 levels
Sources
- Edward Witten, Light Rays, Singularities, and All That, Clay Mathematics Institute lecture notes, arXiv:1901.03928v6 (2023), §§5.2–5.6, latest v6 PDF (107 pages).
- José M. M. Senovilla and David Garfinkle, The 1965 Penrose singularity theorem, Classical and Quantum Gravity 32 (2015), 124008, arXiv:1410.5226v2, §4.1, §4.2 and Theorem 2.
- José Luis Jaramillo, Juan Antonio Valiente Kroon, and Éric Gourgoulhon, From Geometry to Numerics: Interdisciplinary Aspects in Mathematical and Numerical Relativity, arXiv:0712.2332v2 (2008), §§2.1–2.2, full 72-page PDF.