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Future causal position vectors along a curve in a convex normal set
Statement
Assume Countable Choice and Dependent Choice (The Axiom of Countable Choice (), The axiom of dependent choice: a relation in which every element is related to something admits an -indexed chain) for the absolutely continuous causal-curve calculus and the supplied causal results used below.
Let be a time-oriented smooth Lorentzian four-manifold (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model), let be a strictly convex normal set (Existence of strictly convex normal neighborhoods: small coordinate balls are normal neighborhoods of each of their points), let , let , and let be a future causal curve in the class of Causal curves, chronological and causal reachability, and inextendibility with . Then for every the position vector is future causal or zero. Moreover, there is such that the position vectors are nonzero for every .
Facts & Assumptions
Given: A strictly convex normal set , a point and a future causal curve with .
Strictly convex normal sets are normal neighborhoods of each of their points and every pair of their points is joined by a unique geodesic contained in ; moreover is open (Existence of strictly convex normal neighborhoods: small coordinate balls are normal neighborhoods of each of their points clauses (a)-(c), Normal neighborhoods, convex normal sets, the position vector and the squared-displacement function).
For a normal neighborhood of and a future causal curve in with position vectors : if is future timelike, then is future timelike for all later with (Length monotonicity of the squared displacement: once a future causal curve in a normal neighborhood has a future timelike position vector, the displacement radius grows at least as fast as the accumulated Lorentzian length clause (a)).
On a strictly convex normal set , the inverse velocity is smooth on all of by The differential of the squared-displacement function and the position vector of the reversed geodesic clause (c) and satisfies .
The velocity of the geodesic is -related to and the geodesic is future timelike for all parameters if is future timelike, by parallel transport and the continuity of the timelike cone (The geodesic initial-value problem and the exponential map of the metric-selected connection clause (c), Length monotonicity of the squared displacement: once a future causal curve in a normal neighborhood has a future timelike position vector, the displacement radius grows at least as fast as the accumulated Lorentzian length fact [L5]).
The closure of the future timelike cone at a point is contained in the union of the future causal cone with : a limit of future timelike vectors is future causal or zero; and the future causal cone is closed (The timelike set has exactly two convex components, described in orthonormal coordinates, Timelike, null, spacelike and causal vectors of a Lorentz vector space).
Proof
(A past point and an appended timelike geodesic.) Let be the star-shaped domain on which maps diffeomorphically onto . Choose a future timelike and then choose so small that ; this follows from openness of at . Star-shapedness implies for all . Thus lies in on this interval. Put ; the segment runs from to with future timelike velocity. Concatenate with the entire future causal curve to obtain a future causal curve by Chart independence, concatenation, reparametrization and transitivity for causal curves clause (d).
(Position vectors with respect to .) Since is convex normal and , the set is a normal neighborhood of . At , the curve lies on the timelike geodesic , and is a positive multiple of the future timelike initial tangent at of the segment from to . By Length monotonicity of the squared displacement: once a future causal curve in a normal neighborhood has a future timelike position vector, the displacement radius grows at least as fast as the accumulated Lorentzian length clause (a), applied to based at , its position vector remains future timelike for every , since the whole curve segment stays in . In particular is future timelike for every .
(Limit to .) Fix . For every sufficiently small , step 1.2 gives that is future timelike, where . The pairs converge to in . By [L3] the inverse vectors converge to . The future causal cone together with zero is closed, so this limit is future causal or zero. This proves the first claim for every .
(Nonvanishing near the initial point.) By Causal cone domination in adapted charts and Lipschitz-graph bounds for causal curves there is an adapted chart around in which the time coordinate is strictly increasing along every future causal curve contained in the chart. Choose so that lies in this chart. Then for every , so and . This proves the second claim without inferring that a return at one time makes the entire preceding curve constant.
Steps 2.1 and 3.1 prove the claim.
Remarks
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Why a strictly convex normal set. The proof uses only: is open, is a normal neighborhood of and of points arbitrarily close to , and contains the appended timelike segment. The strict form supplied by Existence of strictly convex normal neighborhoods: small coordinate balls are normal neighborhoods of each of their points also supplies the smooth pair inverse used when the base point approaches .
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The gain. The lemma converts causality of the curve into causality of geodesic position vectors throughout the contained curve, which is the input of the global maximality argument in 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.
Depends on
The axiom of dependent choice: a relation in which every element is related to something admits an -indexed chain
The Axiom of Countable Choice ()
Length monotonicity of the squared displacement: once a future causal curve in a normal neighborhood has a future timelike position vector, the displacement radius grows at least as fast as the accumulated Lorentzian length
The differential of the squared-displacement function and the position vector of the reversed geodesic
The joint exponential map: smoothness, invertible differential at the diagonal, and the small-velocity two-point inverse
Causal cone domination in adapted charts and Lipschitz-graph bounds for causal curves
Normal neighborhoods, convex normal sets, the position vector and the squared-displacement function
Existence of strictly convex normal neighborhoods: small coordinate balls are normal neighborhoods of each of their points
Causal curves, chronological and causal reachability, and inextendibility
Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold
Timelike, null, spacelike and causal vectors of a Lorentz vector space
The geodesic initial-value problem and the exponential map of the metric-selected connection
The timelike set has exactly two convex components, described in orthonormal coordinates
Chart independence, concatenation, reparametrization and transitivity for causal curves
Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model
and smooth maps between smooth manifolds
Smooth dependence of ODE solutions on parameters
Intervals of : the nine order-convex forms, nondegeneracy, and length
Dependency tree · 2 levels
Sources
- E. Minguzzi, Lorentzian causality theory, Living Reviews in Relativity 22 (2019), article 3: the appended-timelike-geodesic argument in the proof of Theorem 2.9, printed pp. 29-30
- P. T. Chrusciel, Elements of causality theory, arXiv:1110.6706 (2011): local cone structure and the timelike-geodesic smoothing argument, section 2.4