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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.
Depends on
Trapping and the asymptotic black-hole region
Null normal pairs and screen geometry
Chronology, causality, strong causality, global hyperbolicity and time functions
Causal curves, chronological and causal reachability, and inextendibility
Openness of the chronological future and past, openness of the chronological relation, and closure of future and past sets
Future sets, past sets, achronal boundaries and their elementary properties
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
Future null geodesic completeness and incompleteness
The Axiom of Countable Choice ()
The axiom of dependent choice: a relation in which every element is related to something admits an -indexed chain
In a globally hyperbolic manifold the causal relation is closed and truncated causal cones over compact sets are compact
Time separation in a globally hyperbolic manifold: finiteness, existence of maximizing geodesics and the radial formula on causally convex normal regions
Covariant differentiation along curves: metric pairing, parallel transport and geodesic speed
Achronal boundaries are locally Lipschitz graphs, topological hypersurfaces and null for smooth volume densities
Local null normal pairs and the positive screen quotient
The push-up rule: p << q and q <= r imply p << r, together with the timelike-piece criterion
Null Raychaudhuri and focal-point bound
Null focal points exclude later horismos generators
The geodesic initial-value problem and the exponential map of the metric-selected connection
The joint exponential map: smoothness, invertible differential at the diagonal, and the small-velocity two-point inverse
Existence of strictly convex normal neighborhoods: small coordinate balls are normal neighborhoods of each of their points
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
The differential of the squared-displacement function and the position vector of the reversed geodesic
Smooth dependence of ODE solutions on parameters
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 product of finitely many compact spaces is compact in the product topology
A closed subspace of a compact space is compact, and a finite union of compact subspaces 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
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
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 and 6.2.2, full 72-page PDF.