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Causal And Initial Value Boundaries — Examples

1 · Prerequisites

2 · Summary

This page collects the worked computations and countermodels of gr-causal-and-initial-value-boundaries on the flat models.

Flat computations. Worked Minkowski slice: Cauchy level sets, causal double cones and the compact diamond verifies the Minkowski Cauchy property, the causal convexity of the double cones, the compactness of a causal diamond and the domain of dependence of an inertial slice by explicit coordinate inequalities. Worked vertical geodesics of the open flat slab: affine parameter, limit point and proper time records the affine parameter and length of the vertical geodesics of the open slab, their maximal domain and the absent boundary point. Sharp radial focusing in flat Minkowski space: equality in the Raychaudhuri bound without a singularity computes the radial congruence converging to one event, shows σ=ω=0, θ=−3/ρ, and exhibits equality in the Raychaudhuri focusing bound at the focal event even though the curvature vanishes and every geodesic extends.

Countermodels. A flat time-oriented Lorentzian four-manifold with a closed timelike curve exhibits the closed future timelike curve of the flat cylinder, refuting chronology for flat time-oriented models. A spacelike hypersurface of a globally hyperbolic model that is not a Cauchy hypersurface shows that a bounded spacelike fragment of an inertial slice of globally hyperbolic Minkowski space is missed by an inextendible causal curve, so spacelike is not Cauchy. An achronal set that is not acausal: two null-related points separates the two set conditions with two null-related events: achronal but not acausal.

The general causal-curve conclusions use the Countable Choice and Dependent Choice premises recorded in their suppliers and consuming items. All six items are mathematics: conditional computations and counterexamples inside the explicitly displayed models. None reports a measurement, and none asserts anything about nature.

3 · Logical flowchart

4 · Definitions, postulates, theorems and proofs

None yet.

5 · Examples, experiments and counterexamples

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Worked Minkowski slice: Cauchy level sets, causal double cones and the compact diamond

Example

Assume Countable Choice and Dependent Choice (The Axiom of Countable Choice (ACω), The axiom of dependent choice: a relation in which every element is related to something admits an N-indexed chain) for the general absolutely continuous causal-curve conclusions used here.

Let (A,η,N) be the flat model of The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets, written A=R4, with its global inertial chart x=(x0,z)=(t,z), and write e0:=(1,0,0,0)∈A. This example works through the explicit computations behind The flat model is globally hyperbolic and its inertial level sets are Cauchy hypersurfaces.

(i) For every c∈R the level set Σc:=x−1({c}×R3) is a spacelike embedded hypersurface with induced metric δ=diag⁡(1,1,1) in the coordinates (z1,z2,z3) and future unit normal ∂0 (Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons clause (a)).

(ii) The coordinate t=x0 is a temporal function: its gradient in the chart is ∇t=−∂0, with η(∇t,∇t)=−1<0 and dt(∂0)=1>0 (Chronology, causality, strong causality, global hyperbolicity and time functions clause (e), Monotonicity of inertial time and the Lipschitz graph property for causal curves in the flat model clause (d)).

(iii) For ε>0 and p∈A the double cone Vε(p):=I+(p−εe0)∩I−(p+εe0) is open, contains p, and is causally convex for causal curves that meet it twice: if a future causal curve γ:[a,b]→A has γ(a),γ(b)∈Vε(p), then γ(s)∈Vε(p) for every s∈(a,b). In coordinates, Vε(p)={q: ∣z(q)−z(p)∣e<ε−∣x0(q)−x0(p)∣}.

(iv) For o:=0∈A and q:=Te0, T>0, the causal diamond is J+(o)∩J−(Te0)={r: ∣z(r)∣e≤x0(r)≤T−∣z(r)∣e}, a closed bounded subset of R4, hence compact; its t-sections are closed balls of radius min⁡(t,T−t) for 0≤t≤T, and are empty otherwise.

(v) The domain of dependence of each Σc is all of A: D+(Σc)⊇{t≥c}, D−(Σc)⊇{t≤c} and D(Σc)=A (Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons clause (d)).

Facts & Assumptions

Given: The flat model (A,η,N) of The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets, its global inertial chart, and the sets and curves of the claims.

[L1]

In the global inertial chart x, η=diag⁡(−1,1,1,1), the cone sets of clause (f) are C+={v:v0>∣vs∣e} and C+‾={v:v0≥∣vs∣e}, and q−p∈C+‾ exactly when q∈J+(p), q−p∈C+ exactly when q∈I+(p) (The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets clauses (a), (b), (f), The flat model is globally hyperbolic and its inertial level sets are Cauchy hypersurfaces clause (a), Time orientation, future and past timelike/null/causal vectors, and the closed cones).

[L2]

Along every future causal curve the coordinate t is strictly increasing and ∣z(b)−z(a)∣e≤t(b)−t(a) for a<b; every inextendible causal curve has t-range all of R and meets each level t=c exactly once (Monotonicity of inertial time and the Lipschitz graph property for causal curves in the flat model clauses (a), (b), (c), The flat model is globally hyperbolic and its inertial level sets are Cauchy hypersurfaces clause (b)).

[L3]

Cone additivity: C++C+‾⊆C+ and C+‾+C+‾⊆C+‾ (The causal cones of the flat model in inertial coordinates, and closure of the future cone under sums clause (c)).

[L4]

The hyperplanes {t=c} are embedded submanifolds with slice chart x, and the restriction of η to span⁡(∂1,∂2,∂3) is diag⁡(1,1,1) (Embedded submanifolds and slice charts, The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets clauses (a), (b)).

[L7]

The domain of dependence of S⊆A consists of the points through which every past-inextendible (respectively future-inextendible) causal curve meets S (Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons clause (d)).

[L8]

Euclidean space R3 is complete: every Cauchy sequence in its Euclidean norm converges to a point of R3 (R and Rn for n≥1 with the Euclidean metric are complete, componentwise from the Cauchy criterion in R).

Verification

technique · direct
1.1givenL4

(The level sets.) By [L4] each Σc is an embedded three-dimensional submanifold with tangent space span⁡(∂1,∂2,∂3) on which η restricts to diag⁡(1,1,1)>0; hence Σc is a spacelike embedded hypersurface. Its normal line is spanned by ∂0 with η(∂0,∂0)=−1, and g(∂0,N)=g(∂0,∂0)=−1<0 with N=∂0, so ∂0 is the future unit normal. This proves (i).

1.2givenL1L4

(The coordinate is temporal.) The function t=x0 has differential dt with dt(∂0)=1 and dt(∂a)=0 for a=1,2,3; the vector field w:=−∂0 satisfies η(w,X)=dt(X) for every X because η(−∂0,∂0)=η(∂0,∂0)(−1)=1 and η(−∂0,∂a)=0; hence ∇t=w with η(∇t,∇t)=−1<0 and dt(∂0)=1>0. This is (ii).

2.1step 1.2givenL1L2L3

(The double cone is causally convex.) Let p∈A, ε>0, let γ:[a,b]→A be future causal with γ(a),γ(b)∈Vε(p) and let a<s<b. Since γ(a)∈I+(p−εe0), [L1] gives γ(a)−(p−εe0)∈C+; since γ∣[a,s] is future causal, [L1] gives γ(s)−γ(a)∈C+‾; by [L3], γ(s)−(p−εe0)∈C+, so p−εe0≪γ(s). Similarly γ(b)∈I−(p+εe0) gives (p+εe0)−γ(b)∈C+; since γ∣[s,b] is future causal, γ(b)−γ(s)∈C+‾ and [L3] gives (p+εe0)−γ(s)∈C+, so γ(s)≪p+εe0. Hence γ(s)∈Vε(p), which is causally convex. The displayed coordinate description follows from [L1]: q∈Vε(p) iff (x0(q)−x0(p)+ε, z(q)−z(p))∈C+ and (x0(p)+ε−x0(q), z(p)−z(q))∈C+, i.e. ∣z(q)−z(p)∣e<ε+x0(q)−x0(p) and ∣z(q)−z(p)∣e<ε−x0(q)+x0(p), which is the stated inequality. This proves (iii).

2.2step 1.2givenL1L5

(The diamond is compact.) Let r∈A with coordinates (tr,zr). By [L1], r∈J+(o) means tr≥∣zr∣e and r∈J−(Te0) means T−tr≥∣zr∣e; this is the displayed description. The set described is closed (non-strict inequalities of continuous functions) and bounded: tr∈[0,T] and ∣zr∣e≤min⁡(tr,T−tr)≤T/2. By [L5] it is compact, and its t-section is the closed ball of radius min⁡(t,T−t) in R3. This proves (iv).

2.3step 1.1givenL2L7L8

(The domain of dependence is everything.) Let p∈A with t(p)≥c, and let γ:I→A be any past-inextendible causal curve through p. I claim inf⁡ (t∘γ)(I)=−∞. Otherwise put m:=inf⁡ (t∘γ)(I)>−∞. Since t∘γ is increasing, it tends to m as the parameter tends to inf⁡I. For every ε>0 choose a parameter a∈I with m≤t(γ(a))<m+ε. For any u,v∈I with u,v≤a, the Lipschitz bound [L2] gives ∣z(γ(u))−z(γ(v))∣e≤∣t(γ(u))−t(γ(v))∣<ε. Thus the full spatial tail is Cauchy as the parameter tends to inf⁡I; by completeness [L8] it converges to some z∞∈R3. Since t(γ(⋅))→m, the full curve tail converges to x−1(m,z∞)∈A, contradicting past-inextendibility by clause (d) of Causal curves, chronological and causal reachability, and inextendibility. Hence its time range is unbounded below. Since t∘γ is continuous and strictly increasing on the interval I and attains t(p)≥c at the parameter of p, its image contains (−∞,t(p)], in particular c; so some parameter lies on Σc and p∈D+(Σc). The case t(p)≤c is the time reverse: every future-inextendible causal curve through p has time range unbounded above and hence meets Σc, so p∈D−(Σc). Therefore D+(Σc)∪D−(Σc)=A, which is (v).

3.1step 1.1step 1.2step 2.1step 2.2step 2.3∎

(Conclusion.) Parts (i)-(v) are steps 1.1, 1.2, 2.1, 2.2 and 2.3; this completes the example.

Remarks

  • Reparametrization of the proof. The computations above are exactly the content of the general theorem for this model; they are recorded separately because the concrete inequalities are used by the flat cylinder and slab examples.
  • The double cone. The set Vε(p) has two vertex tips at p±εe0 and is the standard causally convex neighborhood of strong causality; it is not an open coordinate ball.
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Worked vertical geodesics of the open flat slab: affine parameter, limit point and proper time

Example

Assume Countable Choice and Dependent Choice (The Axiom of Countable Choice (ACω), The axiom of dependent choice: a relation in which every element is related to something admits an N-indexed chain) for the general absolutely continuous causal-curve conclusions used here.

Let (M,g,N) be the open flat slab M=x−1((0,1)×R3) of The open flat slab: an incomplete timelike geodesic, a Cauchy slice and global hyperbolicity with restricted inertial chart x=(x0,z). Fix z0∈R3 and let γ:(0,1)→M, γ(s):=x−1(s,z0). This example records the explicit numbers behind the incompleteness claim of that theorem:

(i) γ is a smooth future timelike geodesic with affine parameter s and unit tangent γ′(s)=∂0; in the chart the geodesic equation is y¨=0.

(ii) The affine separation and the Lorentzian length of the segment from s1 to s2, 0<s1<s2<1, are Δs=s2−s1,L(γ∣[s1,s2])=∫s1s2−g(γ′,γ′) ds=s2−s1; with the fixed mathematical scaling constant c>0 of Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold, the metric-defined proper-time increment is τ(s2)−τ(s1)=(s2−s1)/c.

(iii) The maximal domain of a geodesic with the data of γ is exactly (0,1); the image converges in the ambient affine space to the event x−1(1,z0), which does not belong to M. Hence γ is future-inextendible in M with bounded affine parameter, and the slab is timelike geodesically incomplete.

(iv) The slice Σ1/2={x0=1/2} is a Cauchy hypersurface and the slab is globally hyperbolic, so the example exhibits incompleteness in a globally hyperbolic model.

Facts & Assumptions

Given: The open flat slab (M,g,N) with its restricted inertial chart, the point z0∈R3, and real numbers 0<s1<s2<1.

[L1]

M is an open subset of the flat model (A,η,N) of The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets with restricted metric g=η∣M and time orientation N=∂0∣M; the restricted chart has constant components diag⁡(−1,1,1,1); the Christoffel symbols of the metric-selected connection vanish in this chart, every coordinate curve is a geodesic, and the curvature vanishes (The open flat slab: an incomplete timelike geodesic, a Cauchy slice and global hyperbolicity clause (a), A chart with constant metric components has vanishing metric-selected Christoffel symbols and curvature, The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets clauses (b), (c)).

[L2]

A smooth curve whose coordinate path satisfies the geodesic equation is a geodesic, and coordinate curves with y¨=0 satisfy it (Coordinate geodesic equation, A chart with constant metric components has vanishing metric-selected Christoffel symbols and curvature clause (c)).

[L3]

For a piecewise-C1 future timelike curve the metric-defined proper-time increment is c−1∫−g(γ′,γ′) ds, and its Lorentzian length is the integral without the factor c−1 (Timelike worldlines, proper time, length and four-velocity on a Lorentzian four-manifold clause (d)).

[L4]

No geodesic of M with the initial data of γ extends the parameter interval beyond (0,1); γ does not converge to a point of M as s→1, and (M,g,N) is globally hyperbolic with Cauchy slice Σ1/2 (The open flat slab: an incomplete timelike geodesic, a Cauchy slice and global hyperbolicity clauses (b)-(d), Chronology, causality, strong causality, global hyperbolicity and time functions, Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons).

Verification

technique · direct
1.1givenL1L2

(The curve is a unit timelike geodesic.) Write y(s):=(s,z0) for the coordinate path of γ. Then y˙=(1,0,0,0) and y¨=0, so the geodesic equation holds by [L2] because the Christoffel symbols vanish; hence γ is a geodesic with affine parameter s. Its tangent is γ′(s)=∂0, with g(γ′,γ′)=η(∂0,∂0)=−1<0 and g(γ′,N)=−1<0; so it is future unit timelike and the chart geodesic equation is y¨=0. This is (i).

2.1step 1.1givenL3

(Affine and length computations.) By step 1.1, −g(γ′,γ′)=1 on (0,1); the length of the segment over [s1,s2] is therefore ∫s1s21 ds=s2−s1, equal to the affine separation, and [L3] gives the metric-defined proper-time increment (s2−s1)/c. This proves (ii).

3.1step 1.1step 2.1givenL4∎

(Maximal domain, limit point and conclusion.) By [L4] no geodesic of M with the data of γ extends the parameter interval beyond (0,1), and γ does not converge to a point of M as s→1: its coordinate x0(γ(s))=s tends to 1, while every point of M has x0∈(0,1). Hence γ, restricted to the maximal geodesic domain (0,1), is future-inextendible in the sense of Causal curves, chronological and causal reachability, and inextendibility clause (d) and its affine parameter is bounded above; the slab is timelike geodesically incomplete. By [L4] the slice Σ1/2 is a Cauchy hypersurface and the model is globally hyperbolic, which is (iii) and (iv).

Remarks

  • Conditional physical interpretation. Under the framework's SI length-coordinate convention SI unit and coordinate conventions of the classical gravitational framework clause (b), the coordinates x0=s and the affine parameter values s1,s2 are lengths in metres, while c has units m s−1; thus (s2−s1)/c is a duration in seconds. If γ is also interpreted as an ideal clock's worldline, the ideal-clock assumption of Adopted clock, free-fall and light-ray assumptions of the classical gravitational framework clause (i) identifies that metric-defined proper-time increment with the clock-reading difference. This is contextual physical interpretation, outside the mathematical claims and their Verification. The postulate restricts it to ideal clocks in the smooth classical test-field regime without back-reaction; it asserts no real device is exactly ideal and reports no measured reading. The mathematical example itself supplies neither this assumption nor empirical evidence.

  • Numbers used. The affine parameter interval has length 1 in these coordinates; the value is a coordinate statement about the chart x and changes under affine reparametrizations of x0 by a constant factor, under which the incompleteness verdict is unchanged.

  • Not a singularity. Curvature vanishes identically on the slab; the incompleteness is caused by the absent boundary of the region, not by curvature blow-up.

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Sharp radial focusing in flat Minkowski space: equality in the Raychaudhuri bound without a singularity

Example

Let (A,η,N) be the flat model of The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets, written A=R4, with its global inertial chart x=(t,z). Fix T>0 and let e:=x−1(T,0) be the event at coordinate time T on the worldline of the origin. Let O:={q∈A: T−t(q)>∣z(q)∣e} be the interior of the past light cone of e, and define ρ:O→(0,∞),ρ(q):=(T−t(q))2−∣z(q)∣e2, and the vector field W on O whose chart components are Wa(q):=ea−qaρ(q)(a=0,1,2,3). Then:

(i) W is a smooth future unit timelike vector field on the open set O; it is a smooth future unit timelike geodesic congruence in the sense of Geodesic congruences and their expansion, shear and vorticity clause (a).

(ii) The maximal forward flow line of W through p∈O is γp(s)=e−(1−sρ(p))(e−p),s∈[0,ρ(p)), with ρ(γp(s))=ρ(p)−s and γp(0)=p; it reaches e at s=ρ(p). The parameter s=0 is included as a one-sided endpoint, and e∉O so it is excluded from the flow domain. Each affine geodesic s↦γp(s) extends beyond s=ρ(p) as a straight line of A defined for all real s.

(iii) With hab=gab+WaWb the rest-space metric of the congruence and Bab=∇bWa, one has Bab=−1ρ hab,θ=−3ρ,σab=0,ωab=0.

(iv) Along the flow line through a point p with θ0:=θ(p)=−3/ρ(p)<0 one has, for 0≤s<ρ(p), θ(γp(s))=−3ρ(p)−s,1−θ(γp(s))=1−θ0−s3: the Raychaudhuri focusing bound of The Raychaudhuri equation for a geodesic congruence and finite-time focusing clause (b) holds with equality, and the congruence cannot be continued as a smooth geodesic congruence to affine parameter 3/(−θ0)=ρ(p) or beyond.

(v) The spacetime is flat, the Ricci tensor vanishes identically, every maximal geodesic of the model has domain all of R, and at s=ρ(p) the flow lines merely meet at the event e, where the field W is not defined. Thus the finite-time breakdown in (iv) is the focal crossing of the congruence and not a singularity of the spacetime or of any individual geodesic.

Facts & Assumptions

Given: The flat model (A,η,N) of The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets, its global inertial chart x, the event e=x−1(T,0) with T>0, the open set O, the function ρ and the field W, and a point p∈O.

[L1]

In the global inertial chart x, η=diag⁡(−1,1,1,1), the coordinate field ∂0=N is future unit timelike and satisfies η(∂0,∂0)=−1; the coordinate connection of the chart is the metric-selected connection, its Christoffel symbols vanish, straight coordinate lines are its geodesics and the curvature and Ricci tensor vanish identically (The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets clauses (a)-(c), A chart with constant metric components has vanishing metric-selected Christoffel symbols and curvature, Coordinate geodesic equation).

[L2]

With y:=e−q one has y0=T−t(q), yi=−zi(q) and η(y,y)=−(T−t(q))2+∣z(q)∣e2=−ρ(q)2; hence on O the vector y is timelike and W=y/ρ satisfies η(W,W)=−1 and η(W,N)=η(W,∂0)=−(T−t)/ρ<0, so W lies in Cq+ and is future-directed (Timelike, null, spacelike and causal vectors of a Lorentz vector space, Classification of future and past causal vectors by a timelike field clause 3, Time orientation, future and past timelike/null/causal vectors, and the closed cones, Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model).

[L3]

A smooth future unit timelike vector field on an open set is an observer congruence, and if it is geodesic it is a smooth future unit timelike geodesic congruence (Observer congruences, their observer curves and adapted charts, Observers, rest spaces and the spatial projection at an event, Geodesic congruences and their expansion, shear and vorticity clause (a)).

[L4]

For a smooth geodesic congruence the expansion, shear and vorticity are θ=gabBab, σab=B(ab)−13θhab, ωab=B[ab] with Bab=∇bWa and hab=gab+WaWb, and habWb=0, gabhab=3 (Geodesic congruences and their expansion, shear and vorticity clauses (c), Rest-space character of the kinematic fields and the double contraction of B clause (b)).

[L5]

Raychaudhuri equation and focusing: along a flow line of a geodesic congruence, dθds=−13θ2−σabσab+ωabωab−Ric⁡abWaWb; if ω=0, Ric⁡(W,W)≥0 and θ0<0 at s0, then 1−θ(s)≤1−θ0−s−s03 (The Raychaudhuri equation for a geodesic congruence and finite-time focusing clauses (a), (b)).

Verification

technique · direct
1.1givenL1L2L3algebra

(The field is a smooth unit future timelike geodesic congruence.) On O the function ρ is smooth and strictly positive, and the components Wa=(ea−qa)/ρ are smooth; by [L2], η(W,W)=−1 and W is future-directed relative to the time-orientation field N=∂0. It remains to verify the geodesic condition. Put y:=e−q, so y0=T−t and yi=−zi. From ρ2=(T−t)2−∣z∣e2 one computes ∂0ρ=−(T−t)/ρ=y0/ρ and ∂iρ=−zi/ρ=yi/ρ, hence ∂bρ=yb/ρ with yb=ηbcyc; also ∂bya=−δba. Therefore ∂bWa=∂b(yaρ)=−δbaρ−yaybρ3=−δbaρ−WaWbρ. Using ybyb=η(y,y)=−ρ2, Wb∂bWa=ybρ(−δbaρ−yaybρ3)=−yaρ2−ya(ybyb)ρ4=−yaρ2+yaρ2=0. Since the metric-selected connection of the flat model has vanishing Christoffel symbols in this chart, ∇WW=0; with [L3] the field W is a smooth future unit timelike geodesic congruence. This proves (i).

2.1step 1.1givenL1

(The flow lines.) For fixed p∈O define γ(s):=e−(1−s/ρ(p))(e−p) for s∈[0,ρ(p)). Then γ(0)=p, γ is affine in s with derivative γ′(s)=(e−p)/ρ(p)=W(p), a constant vector; by [L1] straight coordinate lines are geodesics, so s↦γ(s) is a geodesic of the model with γ′(s)=W(p). Its ρ-value is ρ(γ(s))=−η(e−γ(s),e−γ(s)); since e−γ(s)=(1−s/ρ(p))(e−p), one gets ρ(γ(s))=(1−s/ρ(p))ρ(p)=ρ(p)−s, which is positive for s<ρ(p) and vanishes at s=ρ(p); in particular γ(s)∈O for 0≤s<ρ(p) and γ(ρ(p))=e in the ambient affine space A. Also W(γ(s))=(e−γ(s))/ρ(γ(s))=(e−p)/ρ(p)=γ′(s), so it is an integral curve. Therefore γ is the maximal forward flow line of W through p, with e as its limiting focal event at finite affine parameter ρ(p). The same straight line continues for all real s and is a geodesic of A defined on all of R by [L1]. This proves (ii).

2.2step 1.1givenL1L4algebra

(The kinematic quantities.) By [L1] the connection is flat and Bab=∇bWa=∂bWa; from the computation in step 1.1, with Wa=ya/ρ, Bab=∂b(yaρ)=−ηabρ−yaybρ3=−1ρ(ηab+WaWb)=−habρ. In particular B is symmetric, so ωab=B[ab]=0, and BabWb=−habWb/ρ=0. For the expansion, [L4] and gabhab=3 give θ=gabBab=−1ρgabhab=−3ρ; then the shear is σab=B(ab)−13θhab=−habρ+1ρhab=0. This proves (iii).

3.1step 2.2givenL4L5algebraconstruct

(The focusing bound is attained and the congruence does not extend.) Let γ=γp be the flow line of step 2.1 and write θ(s):=θ(γ(s)). By step 2.2 and ρ(γ(s))=ρ(p)−s, θ(s)=−3/(ρ(p)−s) for 0≤s<ρ(p). Hence θ0:=θ(p)=−3/ρ(p)<0 and 1−θ(s)=ρ(p)−s3=1−θ0−s3, so the focusing bound of [L5] holds with equality for s0=0. To see directly that this congruence field cannot extend continuously across its focal event e, use the translation identification of tangent spaces of A=R4 and set v1:=∂0∣e and v2:=2∂0∣e+∂1∣e. The flat metric gives η(vi,vi)=−1 and η(vi,Ne)<0 for i=1,2, while v1≠v2. Put pi:=e−vi∈O. Their flow lines have γpi(s)=e−(1−s)vi for 0≤s<1 and W(γpi(s))=vi; both base curves tend to e as s↑1, but the two limits of W are distinct. A continuous extension of W to e would have to take both values v1 and v2, which is impossible. Thus this smooth congruence has no continuous, hence no smooth, extension through e; the individual affine geodesics still continue in A. This proves the local nonextension directly, independent of continuation beyond the region to which the hypotheses of [L5] apply.

4.1step 2.1step 3.1givenL1∎

(No singularity.) By [L1] the curvature and the Ricci tensor of the model vanish identically, every maximal geodesic of the model is a straight coordinate line with domain all of R, and at s=ρ(p) all flow lines pass through the single event e; the field W is not defined at e because ρ(e)=0. Hence the finite-time breakdown of the congruence in step 3.1 is exactly the focal crossing of the flow lines at e, while the spacetime and each individual geodesic continue; the example therefore shows that the local focusing theorem's conclusion is sharp and must be read as a statement about the congruence, not as a singularity. This proves (v) and completes the example.

Remarks

  • Equality case. The radial congruence of future-directed geodesics converging to one event achieves equality in the Raychaudhuri focusing inequality with Ric⁡(W,W)=0, σ=0, ω=0 and initial θ0=−3/ρ(p); the trace of the extrinsic curvature of the level sets of ρ (the hyperbolic "spheres" around e) is −3/ρ in the convention of this library.
  • Interpretation cautions. The ray θ→−∞ at s→ρ(p) is an artifact of the congruence, not of the geometry: the curvature is zero and the geodesics extend. No singularity theorem is proved or illustrated by this computation.
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A flat time-oriented Lorentzian four-manifold with a closed timelike curve

Statement refuted

Statement refuted: "every smooth time-oriented flat Lorentzian four-manifold is chronological, that is, contains no closed future timelike curve" (Chronology, causality, strong causality, global hyperbolicity and time functions clause (a), Causal curves, chronological and causal reachability, and inextendibility clause (c)).

Facts & Assumptions

Given: The flat cylinder model (M,g,N)=A/Λ of The flat cylinder model: closed timelike curves, total viciousness and no Cauchy set, built from the flat model (A,η,N) of The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets with Λ={nLe0:n∈Z}, L>0, orbit map q, a fixed point o∈A, and the curve γ:R→M, γ(s)=q(o+se0).

[L1]

M is a smooth four-manifold, g is a smooth Lorentzian metric obtained by descent so that gq(p)(dqpV,dqpW)=ηp(V,W), N=dq(∂0) is a time orientation, the model is flat, and the curve γ is a nonconstant smooth future timelike curve with γ(s+L)=γ(s) for all s, hence a closed future timelike curve (The flat cylinder model: closed timelike curves, total viciousness and no Cauchy set clauses (a), (b), The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets clauses (b), (c)).

[L2]

A model is chronological when no future timelike curve γ:[a,b]→M with a<b and γ(a)=γ(b) exists, and nonconstant on [a,b] (Chronology, causality, strong causality, global hyperbolicity and time functions clause (a), Causal curves, chronological and causal reachability, and inextendibility clauses (b), (c)).

Counterexample

1.1givenL1

(The witness is a future timelike curve.) By [L1] γ is a smooth mapping into M with velocity γ′(s)=dqo+se0(∂0); the local isometry identity gives g(γ′,γ′)=η(∂0,∂0)=−1<0 and g(γ′,N)=η(∂0,∂0)=−1<0, so every tangent is future unit timelike and γ is a future timelike curve in the class of Causal curves, chronological and causal reachability, and inextendibility.

2.1step 1.1givenL1

(The witness is closed and nonconstant on one period.) By [L1] γ(s+L)=q(o+se0+Le0)=q(o+se0)=γ(s) because Le0∈Λ. It is nonconstant on [0,L]: if γ(s)=γ(0) for some 0<s<L, then se0∈Λ, so s=nL for some nonzero integer n, which is impossible for 0<s<L. Hence γ∣[0,L] is a nonconstant future timelike curve with equal endpoints.

3.1step 2.1givenL1L2∎

(Conclusion.) By step 2.1 and [L2] the model (M,g,N) is not chronological: it contains a closed future timelike curve. Since M is flat and time-oriented by [L1], this refutes the displayed statement. It also shows that a model with a closed timelike curve is not causal, and by The flat cylinder model: closed timelike curves, total viciousness and no Cauchy set clause (d) it admits no Cauchy set at all.

Remarks

  • Where flatness survives. The identification acts by isometries and the quotient is locally isometric to the flat model; the pathology is global and invisible to curvature. This is the flat analogue of the Misner-space warning recorded by Carroll.
  • Scope. The model is a mathematical quotient of the flat model of The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets; the counterexample says nothing about the physical realizability of such an identification.
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A spacelike hypersurface of a globally hyperbolic model that is not a Cauchy hypersurface

Statement refuted

Statement refuted: "every spacelike embedded hypersurface of a globally hyperbolic time-oriented smooth Lorentzian four-manifold is a Cauchy set" (Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons clauses (a) and (c), Chronology, causality, strong causality, global hyperbolicity and time functions clause (c)).

Facts & Assumptions

Assume Countable Choice and Dependent Choice (The Axiom of Countable Choice (ACω), The axiom of dependent choice: a relation in which every element is related to something admits an N-indexed chain) for the general absolutely continuous causal-curve conclusions used here.

Given: The flat model (A,η,N) of The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets, written A=R4, with its global inertial chart x=(t,z), the open unit ball B={z∈R3:∣z∣e<1} and the set Σ:={p∈A:t(p)=0, z(p)∈B}, and the point z0∈R3 with ∣z0∣e=2.

[L1]

The flat model is globally hyperbolic and its level sets {t=c} are Cauchy hypersurfaces (The flat model is globally hyperbolic and its inertial level sets are Cauchy hypersurfaces clauses (b), (d)).

[L2]

Along an inextendible future causal curve of A the coordinate t is a strictly increasing surjection onto R (Monotonicity of inertial time and the Lipschitz graph property for causal curves in the flat model clause (c)).

[L3]

On the open neighborhood U=x−1(R×B) of Σ, the smooth chart y=(x1,x2,x3,t) has y(U)=B×R and y(Σ∩U)=B×{0}=y(U)∩(R3×{0}), so Σ is an embedded submanifold; its tangent space is span⁡(∂1,∂2,∂3) with positive definite metric restriction (Embedded submanifolds and slice charts, Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons clause (a)).

[L4]

A Cauchy set meets every inextendible causal curve in exactly one parameter value (Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons clause (c)).

Counterexample

1.1givenL3

(The set is spacelike.) By [L3] the set Σ is an embedded three-dimensional submanifold of A with tangent space spanned by ∂1,∂2,∂3, on which η=diag⁡(1,1,1) is positive definite; hence Σ is a spacelike embedded hypersurface.

1.2givenL2

(An inextendible causal curve missing it.) Define u:R→A, u(s):=x−1(s,z0). This is a smooth curve with constant tangent ∂0=N, which satisfies η(∂0,∂0)=−1<0 and is future-directed by clause (c) of The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets, so u is a future timelike (hence causal) curve; its t-coordinate is the identity of R, so it has no point limit at either infinite parameter end: such a limit would force its continuous real time coordinate to have a finite limit. Thus u is inextendible by Causal curves, chronological and causal reachability, and inextendibility clause (d). But t(u(s))=s and z(u(s))=z0 with ∣z0∣e=2>1, so u(s)∉Σ for every s; the parameter set {s:u(s)∈Σ} is empty and in particular not a singleton.

2.1step 1.1step 1.2givenL1L4∎

(Conclusion.) By step 1.2 there is an inextendible causal curve that meets Σ in no parameter value; by [L4] the set Σ is not a Cauchy set, and by step 1.1 it is a spacelike embedded hypersurface, so it is not a Cauchy hypersurface. Since the ambient model is globally hyperbolic by [L1], this refutes the displayed statement: in a globally hyperbolic model a spacelike hypersurface need not be Cauchy.

Remarks

  • Why Cauchy leaves are special. The full inertial level sets {t=c} are Cauchy because t is a strictly increasing surjection onto R on every inextendible future causal curve ([L2]); being an entire level set of a temporal function alone does not imply the Cauchy property. The fragment Σ is achronal and spacelike, but inextendible causal curves outside the spatial ball B never see it.
  • Scope. The example is purely kinematic; no field equation, matter content or measurement enters.
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An achronal set that is not acausal: two null-related points

Statement refuted

Statement refuted: "every achronal subset of a time-oriented smooth Lorentzian four-manifold is acausal" (Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons clause (b)).

Facts & Assumptions

Assume Countable Choice and Dependent Choice (The Axiom of Countable Choice (ACω), The axiom of dependent choice: a relation in which every element is related to something admits an N-indexed chain) for the general absolutely continuous causal-curve conclusions used here.

Given: The flat model (A,η,N) of The flat model: Minkowski space R^4, its standard Lorentz form, inertial charts and cone sets, written A=R4, with its global inertial chart x=(t,z), and the two events p:=x−1(0,0,0,0), r:=x−1(1,1,0,0).

[L1]

For all events u,v in the flat model, u≤v exactly when v−u∈C+‾ and u≪v exactly when v−u∈C+, with C+={w:w0>∣ws∣e} and C+‾={w:w0≥∣ws∣e} in the global inertial chart. For u≠v the straight path realizes the relation when the displayed condition holds; for u=v, u≤u instead follows from the equality alternative, without a constant causal curve (The flat model is globally hyperbolic and its inertial level sets are Cauchy hypersurfaces clause (a), The causal cones of the flat model in inertial coordinates, and closure of the future cone under sums clauses (a), (b), Time orientation, future and past timelike/null/causal vectors, and the closed cones, Timelike, null, spacelike and causal vectors of a Lorentz vector space).

[L2]

For events u,v of the model: u≪v when there is a future timelike curve from u to v, and u≤v when u=v or there is a future causal curve from u to v; a set is achronal when no two distinct of its points are chronologically related and acausal when no two distinct of its points are causally related (Causal curves, chronological and causal reachability, and inextendibility clause (c), Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons clause (b)).

Counterexample

1.1givenL1

(The two points.) The displacement r−p has coordinates (1,1,0,0), so η(r−p,r−p)=−1+1=0 and r−p≠0: it is a future null vector. By [L1], its closed-cone membership gives p≤r, while it is not in the open cone C+, so the full reachability equivalence gives p≪̸r.

2.1step 1.1L1L2

(Achronality.) Suppose p≪r; then by [L1] r−p∈C+, i.e. 1>∣(1,0,0)∣e=1, a contradiction. In the other direction, r≪p would require p−r∈C+, i.e. −1>∣(−1,0,0)∣e=1, also false. Hence the two distinct points p,r are not chronologically related in either direction and the set S:={p,r} is achronal by [L2].

3.1step 1.1step 2.1givenL2∎

(Conclusion.) By step 1.1 the distinct points p,r∈S satisfy p≤r, so S is not acausal by [L2]. By step 2.1 the set S is achronal. Hence an achronal set need not be acausal, which refutes the displayed statement.

Remarks

  • Why the two notions differ. Achronality excludes only timelike relations, acausality also excludes null ones; the lightlike separation of two events is the elementary witness. Both notions are defined for arbitrary subsets; the two-point set S is not a hypersurface, and no regularity is claimed for it.
  • Use. The example shows that the implication "acausal implies achronal" of Spacelike hypersurfaces, acausal sets, Cauchy sets, domains of dependence and Cauchy horizons clause (b) cannot be reversed, so a proof that only establishes achronality does not establish acausality.

Sources