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Trapped surfaces and Penrose incompleteness
1 · Prerequisites
- Abelian Categories
- Absolute and Conditional Convergence; Rearrangement; Products
- Absolute Continuity and the Sharp Fundamental Theorem of Calculus
- Arc Length and Rectifiable Curves
- Areas of Elementary Plane Figures
- Binary Operations, Monoids, Groups and Subgroups
- Bounded Variation and the Riemann–Stieltjes Integral
- Cardinal Arithmetic, Cofinality and the Alephs
- Categories, Functors and Natural Transformations
- Causal And Initial Value Boundaries
- Chain Complexes and Homology
- Chain Homotopy and the Homotopy Category
- Compactness
- Compactness in Metric Spaces
- Completeness, Completion, and Uniform Continuity
- Complex Norms and Realification
- Complexification, Realification and Real Structures
- Connectedness
- Connections And Free Fall
- Connections Levi Civita and Parallel Transport
- Constant Rank, Submersions, Immersions and Regular Level Sets
- Construction of the Natural Numbers
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- Continuity, IVT, EVT, and Uniform Continuity
- Convexity
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- Differentiation of Monotone Functions and the Vitali Covering Theorem
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- Rⁿ as a Normed Space; Vector-Valued Functions
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- The Determinant of a Linear Operator, Cofactors and Cramer's Rule
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- The Exponential Function
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- The Lᵖ Spaces Holder Minkowski and Riesz Fischer
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- Volumes of Elementary Solids and Solids of Revolution
2 · Summary
3 · Logical flowchart
4 · Definitions, postulates, theorems and proofs
Future null geodesic completeness and incompleteness
A purely geometric definition of affine completeness within a specified Lorentzian manifold; it asserts neither curvature blow-up nor the existence of a singular point.
Definition
Let be a time-oriented smooth Lorentzian four-manifold with metric-selected connection . A future-directed affinely parametrized null geodesic is a smooth nonconstant curve , where is an interval with nonempty interior, such that its tangent is future-directed and null at every interior parameter and . Here “null” means and , and future-directed means . The geodesic equation and covariant derivative are those of the metric-selected connection.
The maximal future affine interval of such a geodesic is the future endpoint interval of its maximal extension as an affinely parametrized geodesic in . It is future complete when that interval has no finite upper endpoint, equivalently when its affine parameter tends to . The spacetime is future null geodesically complete when every future-directed null geodesic is future complete, and future null geodesically incomplete when at least one is not.
An affine change of parameter with preserves whether the maximal future interval is unbounded above, so these properties do not depend on the chosen positive affine normalization.
Definition references
Conventions and scope
This definition distinguishes an incomplete geodesic in from a curvature singularity or a point added to an extension. No equation for matter, Einstein equation, or claim about the physical adequacy of is included.
A complete temporal flow identifies smooth Cauchy slices
A differential-topological statement about two smooth Cauchy hypersurfaces and a supplied complete timelike product flow; no field equation or empirical claim is involved.
Statement
Let be a time-oriented smooth Lorentzian four-manifold. Suppose a smooth three-manifold and a smooth diffeomorphism are supplied such that each curve is an inextendible future timelike curve and . Let be a smooth spacelike Cauchy hypersurface, meaning that it is met exactly once by every inextendible causal curve. Then the second-coordinate projection is a diffeomorphism. In particular, and have the same connectedness and compactness properties.
Statement references
Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons
Causal curves, chronological and causal reachability, and inextendibility
Diffeomorphisms and local diffeomorphisms of manifolds
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
Facts & Assumptions
Given: A complete timelike product flow as in the Statement and a smooth spacelike Cauchy hypersurface .
The map is a diffeomorphism, each -curve is an inextendible future timelike curve, and ; these are the explicit product-flow hypotheses. In Causal curves, chronological and causal reachability, and inextendibility, timelikeness of a curve requires a future timelike velocity almost everywhere.
Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons: a Cauchy hypersurface meets every inextendible causal curve exactly once, and a smooth spacelike hypersurface has a three-dimensional positive-definite tangent space at each point.
The smooth inverse function theorem on manifolds: a smooth map with an isomorphism as differential at a point restricts to a diffeomorphism on suitable open neighborhoods.
Write . It is nonzero because is invertible. For each fixed , the smooth function is negative almost everywhere by [F1], hence is nonpositive everywhere: a positive value would, by continuity, give a positive value on an interval of positive measure. Thus every nonzero vector in the orbit tangent line has nonpositive squared norm, whereas [F2] gives positive squared norm for every nonzero vector tangent to . Their intersection is therefore , even at an exceptional null orbit tangent.
Proof
Given: [F1]–[F4].
For each , the orbit is an inextendible timelike curve, so [F2] says it meets in exactly one point. Define by writing and setting . Every occurs because its orbit meets , and if then lie on the same orbit, which meets only once; hence is bijective.
The map is smooth because it is the restriction of the smooth map to the embedded submanifold .
At , the kernel of is the one-dimensional tangent to the -orbit. If is in the kernel, then lies in that orbit tangent line and is tangent to the spacelike hypersurface. By [F4], . Since both tangent spaces have dimension three, is an isomorphism.
By [F3], is a local diffeomorphism at every point. It is already a bijection by step 1.1, so its local smooth inverses agree with the unique set-theoretic inverse on their domains; these neighborhoods cover , proving that is smooth. Thus is a diffeomorphism.
Remarks
The proof uses the Cauchy property of to identify each flow orbit once, and spacelikeness to make the projection a local diffeomorphism. It does not assert that an arbitrary continuous Cauchy set is smoothly diffeomorphic to a chosen slice.
Trapping and the asymptotic black-hole region
Pure Lorentzian-geometric definitions. No field equation, cosmic-censorship assumption, event-horizon existence, or empirical claim is asserted.
Definition
Let be a smooth time-oriented Lorentzian four-manifold of signature . Let be a nonempty smooth embedded two-manifold, compact without boundary, whose induced metric is positive definite. At each point its normal plane is a Lorentzian two-plane with two future null rays. On any open patch carrying a smooth ordered pair of future null normals with , define for tangent vectors to . These are the null second fundamental forms and their expansions. A future trapped surface is such an for which, on every local patch and for both future null normal rays, the corresponding expansion is strictly negative at every point. Positive rescaling of a null normal multiplies its expansion by the same positive factor, so the sign condition is independent of its affine normalization and of a local interchange of the two rays.
When a specified conformal completion is supplied, write it as . Here is a smooth four-dimensional manifold with boundary in the senses of Topological manifolds with boundary and Smooth charts, atlases, and structures with boundary. At each point is a symmetric bilinear form on the tangent space, its components extend smoothly in every boundary chart, and its pointwise inertia is in the convention of Lorentz forms of inertia (3,1,0) on a 4-dimensional real vector space. The vector field likewise has components that extend smoothly in every boundary chart; it satisfies everywhere and on the interior. The map is a diffeomorphism onto the interior. The function is smooth in the boundary-chart sense, positive on , and zero with nonzero differential on the designated smooth three-dimensional boundary subset . On the metric satisfies , where pullback is as in The pullback of a covariant tensor field. The restriction of to has a one-dimensional kernel at every point; this null line is the generator direction, and its future ray is the one whose vectors satisfy . Thus the designated boundary is null and future-oriented; no completeness of its generators is assumed.
A curve is locally absolutely continuous when it is continuous and, around each parameter value, its coordinate functions in a boundary or interior chart are absolutely continuous on every compact subinterval of that chart neighborhood, in the sense of Absolute continuity on a compact interval. Boundary charts take values in relatively open subsets of the closed half-space. To compare two charts around a parameter value, shrink its parameter neighborhood so the coordinate image lies in a compact convex subset of a local-extension domain of the transition map. Its derivative is bounded there, so the mean-value estimate (The mean value theorem, as the case of Cauchy's: for continuous on with and differentiable on there is with ) makes the transition Lipschitz. Applying that bound to the finite disjoint-interval condition for absolute continuity shows that the transformed coordinate functions remain absolutely continuous; the argument in both directions proves chart independence. At an interior parameter value where the coordinate derivatives exist, is the tangent vector with those components; the chain rule for the chart transitions (Chain rule for smooth half-space maps) makes it independent of chart. A future causal curve in is a locally absolutely continuous curve for which, for almost every , this derivative exists and satisfies and . These inequalities make the derivative nonzero and select the future direction. On the interior, for every tangent vector , so causal character is unchanged, and the specified orientation condition makes the future cone agree with that of (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model). Define . The black region relative to this completion and its event horizon are, respectively, If no such completion is supplied, these two sets are undefined; their existence is not a consequence of the definition of a trapped surface.
Given in addition a designated smooth future null normal ray field on , called the outward direction, is marginally outer trapped relative to this choice when everywhere. If the outward label comes from a side of an embedded spacelike hypersurface or from an asymptotic end, that side or end is part of the supplied data; it is not inferred from alone. The zero condition is invariant under positive rescaling of the chosen ray.
Definition references
Null normal pairs and screen geometry
Causal curves, chronological and causal reachability, and inextendibility
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
Lorentz forms of inertia (3,1,0) on a 4-dimensional real vector space
Absolute continuity on a compact interval
and smooth maps between smooth manifolds
The differential of a smooth map
The pullback of a covariant tensor field
Derivations at a point and the tangent space
Diffeomorphisms and local diffeomorphisms of manifolds
Intervals of : the nine order-convex forms, nondegeneracy, and length
Chain rule for smooth half-space maps
Smooth functions on relatively open half-space sets
Topological manifolds with boundary
Smooth charts, atlases, and structures with boundary
Interior, closure, boundary, exterior, derived set and isolated point in a topological space
Conventions and scope
The screen geometry supplier fixes the null second fundamental form and expansion and proves their boost law: under , one has . Thus the two inequalities in the trapped-surface definition are local, branch-independent conditions. The event horizon is a global boundary in a specified completion; it is not identified with a trapped surface or a marginally outer trapped surface. In the SI geometric convention with dimensionless metric and affine parameter in metres, the expansion has units , as in the screen geometry supplier.
Compactness of the future horismos under null completeness
A conditional Lorentzian-geometric deduction from compact trapping, global hyperbolicity, null Ricci convergence, and future null completeness; it asserts no curvature singularity or event horizon.
Statement
Assume the Axioms of Countable Choice and Dependent Choice. Let be a time-oriented smooth Lorentzian four-manifold that is globally hyperbolic, meaning strongly causal with compact causal diamonds. Let be a nonempty compact smooth embedded spacelike two-surface whose two future null expansions are negative everywhere. Assume the direct null Ricci condition for every null vector and assume every future-directed affinely parametrized null geodesic in is future complete. Define Then is a closed topological three-manifold without boundary and is compact in the subspace topology of .
Statement references
Facts & Assumptions
Given: A time-oriented globally hyperbolic smooth Lorentzian four-manifold, a nonempty compact future trapped surface , null Ricci nonnegativity, Countable Choice, Dependent Choice, and future null geodesic completeness.
Chronology, causality, strong causality, global hyperbolicity and time functions: global hyperbolicity is strong causality together with compactness of each causal diamond .
Causal curves, chronological and causal reachability, and inextendibility: means a future timelike curve joins to ; means or a future causal curve joins them; and are the corresponding unions over .
In a globally hyperbolic manifold the causal relation is closed and truncated causal cones over compact sets are compact: in a globally hyperbolic spacetime, is closed for every compact .
Time separation in a globally hyperbolic manifold: finiteness, existence of maximizing geodesics and the radial formula on causally convex normal regions: if and , a maximizing causal curve from to exists and is a causal geodesic up to increasing reparametrization; its Lorentzian length is zero exactly when .
Covariant differentiation along curves: metric pairing, parallel transport and geodesic speed: along an affinely parametrized geodesic, is constant.
Future sets, past sets, achronal boundaries and their elementary properties and Openness of the chronological future and past, openness of the chronological relation, and closure of future and past sets: is an open future set, so its boundary is an achronal boundary.
Achronal boundaries are locally Lipschitz graphs, topological hypersurfaces and null for smooth volume densities: the boundary of an open future set is closed and is a topological three-manifold without boundary. Its statement assumes Countable Choice and Dependent Choice.
Null normal pairs and screen geometry: on a patch with a smooth future null normal , , where ; a positive boost sends to .
Local null normal pairs and the positive screen quotient: near every point of a spacelike two-surface, there are smooth future null normal fields representing the two rays, normalized as a pair by .
Null Raychaudhuri and focal-point bound: along a smooth null normal congruence with and , a focal instant occurs by affine parameter if the congruence exists through that parameter.
Null focal points exclude later horismos generators: a focal instant on a future null geodesic normal to puts all sufficiently close later points on that generator in , provided the geodesic and variation data continue slightly past the focal instant.
The geodesic initial-value problem and the exponential map of the metric-selected connection: the maximal geodesic evaluation is smooth on its open domain , where is the maximal affine interval for initial data . The exponential map satisfies when defined, its differential at zero is the identity, and short geodesics are its radial curves.
The joint exponential map: smoothness, invertible differential at the diagonal, and the small-velocity two-point inverse: the joint exponential map is a diffeomorphism near with differential ; its inverse therefore has differential on the diagonal.
Existence of strictly convex normal neighborhoods: small coordinate balls are normal neighborhoods of each of their points and Local causality in a convex normal ball: causal reachability is the exponential cone, the Lorentzian length is bounded by the displacement radius, and null endpoints force the null geodesic: in a sufficiently small strictly convex normal neighborhood, a future timelike position vector gives a future timelike radial geodesic.
The push-up rule: p << q and q <= r imply p << r, together with the timelike-piece criterion: if and , then ; a future causal curve containing a timelike subcurve has chronologically related endpoints.
Smooth dependence of ODE solutions on parameters: for a smooth ODE, near fixed initial data there is a common local compact time interval on which solutions depend smoothly on the initial data and parameters. For the full maximal geodesic domain use [F12].
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, claim 1: for topological spaces and a continuous map , the image of every compact subset is compact in .
A closed subspace of a compact space is compact, and a finite union of compact subspaces is compact: a closed subset of a compact topological space is compact, and a finite union of compact subsets of any topological space is compact.
Heine-Borel in : with the Euclidean metric a subset of is compact if and only if it is closed and bounded, and the proof by bisection uses no choice principle; the same holds on the real line and For a metric space with its metric topology, compactness in the topological sense is compactness in the metric sense, and the two notions of compact subset coincide: closed bounded Euclidean subsets, including closed balls and , are compact for their metric topologies; compactness in a metric space agrees with topological compactness for that topology.
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model: the time-orientation field is future timelike, and a future null vector satisfies .
Future null geodesic completeness and incompleteness: future null completeness means every maximal future affine interval of a future null geodesic is unbounded above.
A product of finitely many compact spaces is compact in the product topology: the product of finitely many compact spaces is compact.
Countable Choice and Dependent Choice are explicit mathematical assumptions, as defined by The Axiom of Countable Choice () and The axiom of dependent choice: a relation in which every element is related to something admits an -indexed chain.
is future trapped and compact; the null Ricci inequality holds along every future null normal geodesic; and every such geodesic exists for all future affine parameters. These are hypotheses, not deductions from an Einstein equation or a matter-energy condition.
Proof
Given: [F1]–[F22] and [A1]–[A2].
Put . It is open because it is the union of the open sets , . If and , then some satisfies ; transitivity gives , so . Thus is an open future set.
For each point of , choose a neighborhood with the two smooth null normal branches supplied by [F9]. On each branch rescale by a positive smooth factor so that ; this is possible by [F20] and does not change the sign of the expansion by [F8]. Both normalized expansions are continuous and negative at the chosen point by the trapped-surface hypothesis. Shrink the neighborhood so that both are at most for some . Compactness of gives a finite subcover; the minimum of its finitely many positive constants gives such that every normalized future null normal has initial expansion .
By [F1] and [F3], is closed, and ; hence . Therefore . Conversely, take and choose with . The timelike vector and the local exponential map give future timelike points by [F12], [F14] and [F20]. If then ; if then and [F15] gives . Thus and, since , . Hence .
Set . For each normalized null normal at , future completeness [F21], local smooth dependence [F16], and smooth evaluation on the maximal geodesic domain [F12] give a smooth null normal geodesic congruence near that initial datum through . Applying [F10] with and the null Ricci hypothesis gives a first focal parameter . The extension required in [F11] is supplied by future null completeness, so its local variation data also exist slightly beyond .
Apply [F7] to the open future set . The equality in step 2.1 shows that is closed and is a topological three-manifold without boundary.
Let and choose with . If , use the zero-length segment at . If , [F4] supplies a maximizing causal geodesic from to . Since , , so the maximizing length is zero; the nonconstant affine geodesic has constant squared speed by [F5], and therefore its future causal tangent is null. Rescale its affine parameter by a positive constant so that , and translate the parameter so that its initial value is .
Every point on this segment satisfies . If , some satisfies ; the push-up rule [F15] then gives , contradicting . Thus the entire segment lies in .
The initial null tangent is normal to . Suppose otherwise. Then some has ; since is spacelike, . Choose a smooth curve with and . The joint exponential map lemma [F13] gives a smooth two-point inverse near whose differential in local tangent-bundle coordinates at the diagonal sends basepoint/endpoint variations to . Therefore, after identifying nearby tangent spaces by a smooth local frame, . Choose a small nonzero with and . With , , so for sufficiently small the vector is timelike; its future orientation follows by continuity from the future null vector for small . By [F14], . The remaining segment is causal; [F15] gives , contradicting . Hence .
Return to and its normal generator from steps 3.2, 4.1, and 5.1, with endpoint parameter . If a focal instant occurred strictly before , [F11] would give a point with and . Since , [F15] would imply , a contradiction. Hence ; for the parameter is and the same bound holds.
Choose finitely many relatively compact coordinate patches covering , each contained in a patch with the two smooth normalized null normal fields from step 1.2. Their compact closures exist by choosing smaller Euclidean chart balls and applying Heine–Borel [F19] and the continuous-image theorem [F17]. For each and each branch , the parameter domain is compact by [F22], and the map is continuous on it by [F12], [F16] and future completeness. Its image is compact by [F17]. By [F18], the finite union of these compact images is compact. Step 6.1 shows that every lies in .
By step 3.1, is closed in . Since step 7.1 places it inside the compact set , it is closed in and hence compact by [F18]. This proves the claim.
Remarks
The proof does not assume that is globally achronal or that its normal bundle has a global null frame. It uses local normal branches and their positive, observer-normalized rescalings. Null Ricci nonnegativity is a direct geometric hypothesis; no Einstein equation or matter condition is inferred. A focal point is used only to bound the part of the null generator that can remain in , not as a curvature singularity.
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.
5 · Examples, experiments and counterexamples
None yet.
Sources
- Edward Witten, Light Rays, Singularities, and All That, Clay Mathematics Institute lecture notes, arXiv:1901.03928v6 (2023), §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 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 and 6.2.2, full 72-page PDF.
- Edward Witten, Light Rays, Singularities, and All That, Clay Mathematics Institute lecture notes, arXiv:1901.03928v6 (2023), §§5.5–5.6 and 6.2, 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, §4.2.
- 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.