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+ < > A domain of spacetime intervals for General Relativity Keye Martin and Prakash Panangaden Tulane University and McGill University work done at University of Oxford Dagstuhl August 2004 – p.1/33
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Page 1: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

A domain of spacetime intervals for GeneralRelativity

Keye Martin and Prakash Panangaden

Tulane University and McGill University

work done at University of Oxford

Dagstuhl August 2004 – p.1/33

Page 2: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Viewpoint

Understand the role of order in analysing the causalstructure of spacetime.

Reconstruct spacetime topology from causal order:obvious links with domain theory.

Not looking at the combinatorial aspects of order:continuous posets play a vital role; Scott, Lawsonand interval topologies play a vital role.

Everything is about classical spacetime: we see thisas a step on Sorkin’s programme to understandquantum gravity in terms of causets.

Dagstuhl August 2004 – p.2/33

Page 3: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Viewpoint

Understand the role of order in analysing the causalstructure of spacetime.

Reconstruct spacetime topology from causal order:obvious links with domain theory.

Not looking at the combinatorial aspects of order:continuous posets play a vital role; Scott, Lawsonand interval topologies play a vital role.

Everything is about classical spacetime: we see thisas a step on Sorkin’s programme to understandquantum gravity in terms of causets.

Dagstuhl August 2004 – p.2/33

Page 4: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Viewpoint

Understand the role of order in analysing the causalstructure of spacetime.

Reconstruct spacetime topology from causal order:obvious links with domain theory.

Not looking at the combinatorial aspects of order:continuous posets play a vital role; Scott, Lawsonand interval topologies play a vital role.

Everything is about classical spacetime: we see thisas a step on Sorkin’s programme to understandquantum gravity in terms of causets.

Dagstuhl August 2004 – p.2/33

Page 5: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Viewpoint

Understand the role of order in analysing the causalstructure of spacetime.

Reconstruct spacetime topology from causal order:obvious links with domain theory.

Not looking at the combinatorial aspects of order:continuous posets play a vital role; Scott, Lawsonand interval topologies play a vital role.

Everything is about classical spacetime: we see thisas a step on Sorkin’s programme to understandquantum gravity in terms of causets.

Dagstuhl August 2004 – p.2/33

Page 6: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Overview

The causal structure of globally hyperbolicspacetimes defines a bicontinuous poset. Thetopology can be recovered from the order and fromthe way-below relation but with no appeal tosmoothness. The order can be taken to befundamental.

The entire spacetime manifold can be reconstructedgiven a countable dense subset with the inducedorder: no metric information need be given.

Globally hyperbolic spacetimes can be seen as themaximal elements of interval domains. There is anequivalence of categories between globallyhyperbolic spacetimes and interval domains. Themain theorem.

Dagstuhl August 2004 – p.3/33

Page 7: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Overview

The causal structure of globally hyperbolicspacetimes defines a bicontinuous poset. Thetopology can be recovered from the order and fromthe way-below relation but with no appeal tosmoothness. The order can be taken to befundamental.

The entire spacetime manifold can be reconstructedgiven a countable dense subset with the inducedorder: no metric information need be given.

Globally hyperbolic spacetimes can be seen as themaximal elements of interval domains. There is anequivalence of categories between globallyhyperbolic spacetimes and interval domains. Themain theorem.

Dagstuhl August 2004 – p.3/33

Page 8: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Overview

The causal structure of globally hyperbolicspacetimes defines a bicontinuous poset. Thetopology can be recovered from the order and fromthe way-below relation but with no appeal tosmoothness. The order can be taken to befundamental.

The entire spacetime manifold can be reconstructedgiven a countable dense subset with the inducedorder: no metric information need be given.

Globally hyperbolic spacetimes can be seen as themaximal elements of interval domains. There is anequivalence of categories between globallyhyperbolic spacetimes and interval domains. Themain theorem.

Dagstuhl August 2004 – p.3/33

Page 9: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Work in Progress

The space of causal curves between two compactsets is itself compact in the Vietoris topology. Causalcurves are maximal elements of the convexpowerdomain. Paper by Keye Martin is on the ArXiv(gr-qc).

Incorporating metric information as a measurement(in Keye Martin’s sense) on top of the poset.

Dagstuhl August 2004 – p.4/33

Page 10: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Work in Progress

The space of causal curves between two compactsets is itself compact in the Vietoris topology. Causalcurves are maximal elements of the convexpowerdomain. Paper by Keye Martin is on the ArXiv(gr-qc).

Incorporating metric information as a measurement(in Keye Martin’s sense) on top of the poset.

Dagstuhl August 2004 – p.4/33

Page 11: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causality in Computer Science

In distributed systems one loses synchronization andabsolute global state just as in relativity. One workswith causal structure.

Causal precedence in distributed systems studied byPetri (65) and Lamport (77): clever algorithms, butthe mathematics was elementary and combinatorialand did not reveal the connections with generalrelativity.

Event structures studied by Winskel, Plotkin andothers (80-85): more sophisticated, invoked domaintheory. The mathematics comes closer to what wewill see today.

Dagstuhl August 2004 – p.5/33

Page 12: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causality in Computer Science

In distributed systems one loses synchronization andabsolute global state just as in relativity. One workswith causal structure.

Causal precedence in distributed systems studied byPetri (65) and Lamport (77): clever algorithms, butthe mathematics was elementary and combinatorialand did not reveal the connections with generalrelativity.

Event structures studied by Winskel, Plotkin andothers (80-85): more sophisticated, invoked domaintheory. The mathematics comes closer to what wewill see today.

Dagstuhl August 2004 – p.5/33

Page 13: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causality in Computer Science

In distributed systems one loses synchronization andabsolute global state just as in relativity. One workswith causal structure.

Causal precedence in distributed systems studied byPetri (65) and Lamport (77): clever algorithms, butthe mathematics was elementary and combinatorialand did not reveal the connections with generalrelativity.

Event structures studied by Winskel, Plotkin andothers (80-85): more sophisticated, invoked domaintheory. The mathematics comes closer to what wewill see today.

Dagstuhl August 2004 – p.5/33

Page 14: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The layers of spacetime structure

Set of events: no structure

Topology: 4 dimensional real manifold

Differentiable structure: tangent spaces

Causal structure: light cones (defines metric up toconformal transformations)

Lorentzian metric: gives a length scale.

Dagstuhl August 2004 – p.6/33

Page 15: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The layers of spacetime structure

Set of events: no structure

Topology: 4 dimensional real manifold

Differentiable structure: tangent spaces

Causal structure: light cones (defines metric up toconformal transformations)

Lorentzian metric: gives a length scale.

Dagstuhl August 2004 – p.6/33

Page 16: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The layers of spacetime structure

Set of events: no structure

Topology: 4 dimensional real manifold

Differentiable structure: tangent spaces

Causal structure: light cones (defines metric up toconformal transformations)

Lorentzian metric: gives a length scale.

Dagstuhl August 2004 – p.6/33

Page 17: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The layers of spacetime structure

Set of events: no structure

Topology: 4 dimensional real manifold

Differentiable structure: tangent spaces

Causal structure: light cones (defines metric up toconformal transformations)

Lorentzian metric: gives a length scale.

Dagstuhl August 2004 – p.6/33

Page 18: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The layers of spacetime structure

Set of events: no structure

Topology: 4 dimensional real manifold

Differentiable structure: tangent spaces

Causal structure: light cones (defines metric up toconformal transformations)

Lorentzian metric: gives a length scale.

Dagstuhl August 2004 – p.6/33

Page 19: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causal Structure of Spacetime I

At every point a pair of “cones” is defined in thetangent space: future and past light cone. A vectoron the cone is called null or lightlike and one insidethe cone is called timelike.

We assume that spacetime is time-orientable: thereis a global notion of future and past.

A timelike curve from x to y has a tangent vector thatis everywhere timelike: we write x � y. (We avoidx � y for now.) A causal curve has a tangent that, atevery point, is either timelike or null: we write x ≤ y.

A fundamental assumption is that ≤ is a partial order.Penrose and Kronheimer give axioms for ≤ and �.

Dagstuhl August 2004 – p.7/33

Page 20: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causal Structure of Spacetime I

At every point a pair of “cones” is defined in thetangent space: future and past light cone. A vectoron the cone is called null or lightlike and one insidethe cone is called timelike.

We assume that spacetime is time-orientable: thereis a global notion of future and past.

A timelike curve from x to y has a tangent vector thatis everywhere timelike: we write x � y. (We avoidx � y for now.) A causal curve has a tangent that, atevery point, is either timelike or null: we write x ≤ y.

A fundamental assumption is that ≤ is a partial order.Penrose and Kronheimer give axioms for ≤ and �.

Dagstuhl August 2004 – p.7/33

Page 21: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causal Structure of Spacetime I

At every point a pair of “cones” is defined in thetangent space: future and past light cone. A vectoron the cone is called null or lightlike and one insidethe cone is called timelike.

We assume that spacetime is time-orientable: thereis a global notion of future and past.

A timelike curve from x to y has a tangent vector thatis everywhere timelike: we write x � y. (We avoidx � y for now.) A causal curve has a tangent that, atevery point, is either timelike or null: we write x ≤ y.

A fundamental assumption is that ≤ is a partial order.Penrose and Kronheimer give axioms for ≤ and �.

Dagstuhl August 2004 – p.7/33

Page 22: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causal Structure of Spacetime I

At every point a pair of “cones” is defined in thetangent space: future and past light cone. A vectoron the cone is called null or lightlike and one insidethe cone is called timelike.

We assume that spacetime is time-orientable: thereis a global notion of future and past.

A timelike curve from x to y has a tangent vector thatis everywhere timelike: we write x � y. (We avoidx � y for now.) A causal curve has a tangent that, atevery point, is either timelike or null: we write x ≤ y.

A fundamental assumption is that ≤ is a partial order.Penrose and Kronheimer give axioms for ≤ and �.

Dagstuhl August 2004 – p.7/33

Page 23: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causal Structure of Spacetime II

I+(x) := {y ∈ M |x � y}; similarly I−

J+(x) := {y ∈ M |x ≤ y}; similarly J−.

I± are always open sets in the manifold topology; J±

are not always closed sets.

Chronology: x � y ⇒ y 6� x.

Causality: x ≤ y and y ≤ x implies x = y.

Dagstuhl August 2004 – p.8/33

Page 24: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causal Structure of Spacetime II

I+(x) := {y ∈ M |x � y}; similarly I−

J+(x) := {y ∈ M |x ≤ y}; similarly J−.

I± are always open sets in the manifold topology; J±

are not always closed sets.

Chronology: x � y ⇒ y 6� x.

Causality: x ≤ y and y ≤ x implies x = y.

Dagstuhl August 2004 – p.8/33

Page 25: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causal Structure of Spacetime II

I+(x) := {y ∈ M |x � y}; similarly I−

J+(x) := {y ∈ M |x ≤ y}; similarly J−.

I± are always open sets in the manifold topology; J±

are not always closed sets.

Chronology: x � y ⇒ y 6� x.

Causality: x ≤ y and y ≤ x implies x = y.

Dagstuhl August 2004 – p.8/33

Page 26: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causal Structure of Spacetime II

I+(x) := {y ∈ M |x � y}; similarly I−

J+(x) := {y ∈ M |x ≤ y}; similarly J−.

I± are always open sets in the manifold topology; J±

are not always closed sets.

Chronology: x � y ⇒ y 6� x.

Causality: x ≤ y and y ≤ x implies x = y.

Dagstuhl August 2004 – p.8/33

Page 27: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causal Structure of Spacetime II

I+(x) := {y ∈ M |x � y}; similarly I−

J+(x) := {y ∈ M |x ≤ y}; similarly J−.

I± are always open sets in the manifold topology; J±

are not always closed sets.

Chronology: x � y ⇒ y 6� x.

Causality: x ≤ y and y ≤ x implies x = y.

Dagstuhl August 2004 – p.8/33

Page 28: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causality Conditions

I± = I± ⇒ p = q.

Strong causality at p: Every neighbourhood O of p

contains a neighbourhood U ⊂ O such that no causalcurve can enter U , leave it and then re-enter it.

Stable causality: perturbations of the metric do notcause violations of causality.

Causal simplicity: for all x ∈ M , J±(x) are closed.

Global hyperbolicity: M is strongly causal and foreach p, q in M , [p, q] := J+(p) ∩ J−(q) is compact.

Dagstuhl August 2004 – p.9/33

Page 29: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causality Conditions

I± = I± ⇒ p = q.

Strong causality at p: Every neighbourhood O of p

contains a neighbourhood U ⊂ O such that no causalcurve can enter U , leave it and then re-enter it.

Stable causality: perturbations of the metric do notcause violations of causality.

Causal simplicity: for all x ∈ M , J±(x) are closed.

Global hyperbolicity: M is strongly causal and foreach p, q in M , [p, q] := J+(p) ∩ J−(q) is compact.

Dagstuhl August 2004 – p.9/33

Page 30: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causality Conditions

I± = I± ⇒ p = q.

Strong causality at p: Every neighbourhood O of p

contains a neighbourhood U ⊂ O such that no causalcurve can enter U , leave it and then re-enter it.

Stable causality: perturbations of the metric do notcause violations of causality.

Causal simplicity: for all x ∈ M , J±(x) are closed.

Global hyperbolicity: M is strongly causal and foreach p, q in M , [p, q] := J+(p) ∩ J−(q) is compact.

Dagstuhl August 2004 – p.9/33

Page 31: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causality Conditions

I± = I± ⇒ p = q.

Strong causality at p: Every neighbourhood O of p

contains a neighbourhood U ⊂ O such that no causalcurve can enter U , leave it and then re-enter it.

Stable causality: perturbations of the metric do notcause violations of causality.

Causal simplicity: for all x ∈ M , J±(x) are closed.

Global hyperbolicity: M is strongly causal and foreach p, q in M , [p, q] := J+(p) ∩ J−(q) is compact.

Dagstuhl August 2004 – p.9/33

Page 32: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Causality Conditions

I± = I± ⇒ p = q.

Strong causality at p: Every neighbourhood O of p

contains a neighbourhood U ⊂ O such that no causalcurve can enter U , leave it and then re-enter it.

Stable causality: perturbations of the metric do notcause violations of causality.

Causal simplicity: for all x ∈ M , J±(x) are closed.

Global hyperbolicity: M is strongly causal and foreach p, q in M , [p, q] := J+(p) ∩ J−(q) is compact.

Dagstuhl August 2004 – p.9/33

Page 33: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The Alexandrov Topology

Define〈x, y〉 := I+(x) ∩ I−(y).

The sets of the form 〈x, y〉 form a base for a topology onM called the Alexandrov topology.Theorem (Penrose): TFAE:

1. (M, g) is strongly causal.

2. The Alexandrov topology agrees with the manifoldtopology.

3. The Alexandrov topology is Hausdorff.

The proof is geometric in nature.

Dagstuhl August 2004 – p.10/33

Page 34: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The Way-below relation

In domain theory, in addition to ≤ there is anadditional, (often) irreflexive, transitive relation written�: x � y means that x has a “finite” piece ofinformation about y or x is a “finite approximation” toy. If x � x we say that x is finite.

The relation x � y - pronounced x is “way below” y -is directly defined from ≤.

Official definition of x � y: If X ⊂ D is directed andy ≤ (tX) then there exists u ∈ X such that x ≤ u. If alimit gets past y then, at some finite stage of thelimiting process it already got past x.

Dagstuhl August 2004 – p.11/33

Page 35: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The Way-below relation

In domain theory, in addition to ≤ there is anadditional, (often) irreflexive, transitive relation written�: x � y means that x has a “finite” piece ofinformation about y or x is a “finite approximation” toy. If x � x we say that x is finite.

The relation x � y - pronounced x is “way below” y -is directly defined from ≤.

Official definition of x � y: If X ⊂ D is directed andy ≤ (tX) then there exists u ∈ X such that x ≤ u. If alimit gets past y then, at some finite stage of thelimiting process it already got past x.

Dagstuhl August 2004 – p.11/33

Page 36: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The Way-below relation

In domain theory, in addition to ≤ there is anadditional, (often) irreflexive, transitive relation written�: x � y means that x has a “finite” piece ofinformation about y or x is a “finite approximation” toy. If x � x we say that x is finite.

The relation x � y - pronounced x is “way below” y -is directly defined from ≤.

Official definition of x � y: If X ⊂ D is directed andy ≤ (tX) then there exists u ∈ X such that x ≤ u. If alimit gets past y then, at some finite stage of thelimiting process it already got past x.

Dagstuhl August 2004 – p.11/33

Page 37: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The role of way below in spacetime structure

Theorem: Let (M, g) be a spacetime with Lorentziansignature. Define x � y as the way-below relation ofthe causal order. If (M, g) is globally hyperbolic thenx � y iff y ∈ I+(x).

One can recover I from J without knowing whatsmooth or timelike means.

Intuition: any way of approaching y must involvegetting into the timelike future of x.

We can stop being coy about notational clashes:henceforth � is way-below and the timelike order.

Dagstuhl August 2004 – p.12/33

Page 38: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The role of way below in spacetime structure

Theorem: Let (M, g) be a spacetime with Lorentziansignature. Define x � y as the way-below relation ofthe causal order. If (M, g) is globally hyperbolic thenx � y iff y ∈ I+(x).

One can recover I from J without knowing whatsmooth or timelike means.

Intuition: any way of approaching y must involvegetting into the timelike future of x.

We can stop being coy about notational clashes:henceforth � is way-below and the timelike order.

Dagstuhl August 2004 – p.12/33

Page 39: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The role of way below in spacetime structure

Theorem: Let (M, g) be a spacetime with Lorentziansignature. Define x � y as the way-below relation ofthe causal order. If (M, g) is globally hyperbolic thenx � y iff y ∈ I+(x).

One can recover I from J without knowing whatsmooth or timelike means.

Intuition: any way of approaching y must involvegetting into the timelike future of x.

We can stop being coy about notational clashes:henceforth � is way-below and the timelike order.

Dagstuhl August 2004 – p.12/33

Page 40: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

The role of way below in spacetime structure

Theorem: Let (M, g) be a spacetime with Lorentziansignature. Define x � y as the way-below relation ofthe causal order. If (M, g) is globally hyperbolic thenx � y iff y ∈ I+(x).

One can recover I from J without knowing whatsmooth or timelike means.

Intuition: any way of approaching y must involvegetting into the timelike future of x.

We can stop being coy about notational clashes:henceforth � is way-below and the timelike order.

Dagstuhl August 2004 – p.12/33

Page 41: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Continuous Domains and Topology

A continuous domain D has a basis of elementsB ⊂ D such that for every x in D the setx↓↓ := {u ∈ B|u � x} is directed and t(x↓↓) = x.

The Scott topology: the open sets of D are upwardsclosed and if O is open, then if X ⊂ D, directed andtX ∈ O it must be the case that some x ∈ X is in O.

The Lawson topology: basis of the form

O \ [∪i(xi ↑)]

where O is Scott open. This topology is metrizable ifthe domain is ω-continuous.

The interval topology: basis sets of the form(x, y) := {u|x � u � y}.

Dagstuhl August 2004 – p.13/33

Page 42: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Continuous Domains and Topology

A continuous domain D has a basis of elementsB ⊂ D such that for every x in D the setx↓↓ := {u ∈ B|u � x} is directed and t(x↓↓) = x.

The Scott topology: the open sets of D are upwardsclosed and if O is open, then if X ⊂ D, directed andtX ∈ O it must be the case that some x ∈ X is in O.

The Lawson topology: basis of the form

O \ [∪i(xi ↑)]

where O is Scott open. This topology is metrizable ifthe domain is ω-continuous.

The interval topology: basis sets of the form(x, y) := {u|x � u � y}.

Dagstuhl August 2004 – p.13/33

Page 43: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Continuous Domains and Topology

A continuous domain D has a basis of elementsB ⊂ D such that for every x in D the setx↓↓ := {u ∈ B|u � x} is directed and t(x↓↓) = x.

The Scott topology: the open sets of D are upwardsclosed and if O is open, then if X ⊂ D, directed andtX ∈ O it must be the case that some x ∈ X is in O.

The Lawson topology: basis of the form

O \ [∪i(xi ↑)]

where O is Scott open. This topology is metrizable ifthe domain is ω-continuous.

The interval topology: basis sets of the form(x, y) := {u|x � u � y}.

Dagstuhl August 2004 – p.13/33

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+ < >

Continuous Domains and Topology

A continuous domain D has a basis of elementsB ⊂ D such that for every x in D the setx↓↓ := {u ∈ B|u � x} is directed and t(x↓↓) = x.

The Scott topology: the open sets of D are upwardsclosed and if O is open, then if X ⊂ D, directed andtX ∈ O it must be the case that some x ∈ X is in O.

The Lawson topology: basis of the form

O \ [∪i(xi ↑)]

where O is Scott open. This topology is metrizable ifthe domain is ω-continuous.

The interval topology: basis sets of the form(x, y) := {u|x � u � y}.

Dagstuhl August 2004 – p.13/33

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+ < >

Bicontinuity and Global Hyperbolicity

The definition of continuous domain - or poset - isbiased towards approximation from below. If wesymmetrize the definitions we get bicontinuity (detailsin the paper).

Theorem: If (M, g) is globally hyperbolic then (M,≤)is a bicontinuous poset. In this case the intervaltopology is the manifold topology.

We feel that bicontinuity is a significant causalitycondition in its own right; perhaps it sits betweenglobally hyperbolic and causally simple.

Topological property of causally simple spacetimes:If (M, g) is causally simple then the Lawson topologyis contained in the interval topology.

Dagstuhl August 2004 – p.14/33

Page 46: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Bicontinuity and Global Hyperbolicity

The definition of continuous domain - or poset - isbiased towards approximation from below. If wesymmetrize the definitions we get bicontinuity (detailsin the paper).

Theorem: If (M, g) is globally hyperbolic then (M,≤)is a bicontinuous poset. In this case the intervaltopology is the manifold topology.

We feel that bicontinuity is a significant causalitycondition in its own right; perhaps it sits betweenglobally hyperbolic and causally simple.

Topological property of causally simple spacetimes:If (M, g) is causally simple then the Lawson topologyis contained in the interval topology.

Dagstuhl August 2004 – p.14/33

Page 47: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Bicontinuity and Global Hyperbolicity

The definition of continuous domain - or poset - isbiased towards approximation from below. If wesymmetrize the definitions we get bicontinuity (detailsin the paper).

Theorem: If (M, g) is globally hyperbolic then (M,≤)is a bicontinuous poset. In this case the intervaltopology is the manifold topology.

We feel that bicontinuity is a significant causalitycondition in its own right; perhaps it sits betweenglobally hyperbolic and causally simple.

Topological property of causally simple spacetimes:If (M, g) is causally simple then the Lawson topologyis contained in the interval topology.

Dagstuhl August 2004 – p.14/33

Page 48: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Bicontinuity and Global Hyperbolicity

The definition of continuous domain - or poset - isbiased towards approximation from below. If wesymmetrize the definitions we get bicontinuity (detailsin the paper).

Theorem: If (M, g) is globally hyperbolic then (M,≤)is a bicontinuous poset. In this case the intervaltopology is the manifold topology.

We feel that bicontinuity is a significant causalitycondition in its own right; perhaps it sits betweenglobally hyperbolic and causally simple.

Topological property of causally simple spacetimes:If (M, g) is causally simple then the Lawson topologyis contained in the interval topology.

Dagstuhl August 2004 – p.14/33

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+ < >

An “abstract” version of globally hyperbolic

We define a globally hyperbolic poset (X,≤) to be

1. bicontinuous and,

2. all segments [a, b] := {x : a ≤ x ≤ b} are compact inthe interval topology on X.

Dagstuhl August 2004 – p.15/33

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+ < >

Properties of globally hyperbolic posets

A globally hyperbolic poset is locally compact andHausdorff.

The Lawson topology is contained in the intervaltopology.

Its partial order ≤ is a closed subset of X2.

Each directed set with an upper bound has asupremum.

Each filtered set with a lower bound has an infimum.

Dagstuhl August 2004 – p.16/33

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+ < >

Properties of globally hyperbolic posets

A globally hyperbolic poset is locally compact andHausdorff.

The Lawson topology is contained in the intervaltopology.

Its partial order ≤ is a closed subset of X2.

Each directed set with an upper bound has asupremum.

Each filtered set with a lower bound has an infimum.

Dagstuhl August 2004 – p.16/33

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+ < >

Properties of globally hyperbolic posets

A globally hyperbolic poset is locally compact andHausdorff.

The Lawson topology is contained in the intervaltopology.

Its partial order ≤ is a closed subset of X2.

Each directed set with an upper bound has asupremum.

Each filtered set with a lower bound has an infimum.

Dagstuhl August 2004 – p.16/33

Page 53: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Properties of globally hyperbolic posets

A globally hyperbolic poset is locally compact andHausdorff.

The Lawson topology is contained in the intervaltopology.

Its partial order ≤ is a closed subset of X2.

Each directed set with an upper bound has asupremum.

Each filtered set with a lower bound has an infimum.

Dagstuhl August 2004 – p.16/33

Page 54: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Properties of globally hyperbolic posets

A globally hyperbolic poset is locally compact andHausdorff.

The Lawson topology is contained in the intervaltopology.

Its partial order ≤ is a closed subset of X2.

Each directed set with an upper bound has asupremum.

Each filtered set with a lower bound has an infimum.

Dagstuhl August 2004 – p.16/33

Page 55: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Second countability

Globally hyperbolic posets share a remarkableproperty with metric spaces, that separability(countable dense subset) and second countability(countable base of opens) are equivalent.

Let (X,≤) be a bicontinuous poset. If C ⊆ X is acountable dense subset in the interval topology, then:(i) The collection

{(ai, bi) : ai, bi ∈ C, ai � bi}

is a countable basis for the interval topology.(ii) For all x ∈ X, ↓↓x ∩ C contains a directed set with

supremum x, and ↑↑x ∩ C contains a filtered set withinfimum x.

Dagstuhl August 2004 – p.17/33

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+ < >

Second countability

Globally hyperbolic posets share a remarkableproperty with metric spaces, that separability(countable dense subset) and second countability(countable base of opens) are equivalent.

Let (X,≤) be a bicontinuous poset. If C ⊆ X is acountable dense subset in the interval topology, then:(i) The collection

{(ai, bi) : ai, bi ∈ C, ai � bi}

is a countable basis for the interval topology.(ii) For all x ∈ X, ↓↓x ∩ C contains a directed set with

supremum x, and ↑↑x ∩ C contains a filtered set withinfimum x.

Dagstuhl August 2004 – p.17/33

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+ < >

An Important Example of a Domain: I

�The collection of compact intervals of the real line

I

= {[a, b] : a, b ∈

& a ≤ b}

ordered under reverse inclusion

[a, b] v [c, d] ⇔ [c, d] ⊆ [a, b]

is an ω-continuous dcpo.

For directed S ⊆ I ,⊔

S =⋂

S,

I � J ⇔ J ⊆ int(I), and

{[p, q] : p, q ∈ & p ≤ q} is a countable basis for I .

The domain I is called the interval domain.

We also have max(I ) ' in the Scott topology.

Dagstuhl August 2004 – p.18/33

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+ < >

An Important Example of a Domain: I

�The collection of compact intervals of the real line

I

= {[a, b] : a, b ∈

& a ≤ b}

ordered under reverse inclusion

[a, b] v [c, d] ⇔ [c, d] ⊆ [a, b]

is an ω-continuous dcpo.

For directed S ⊆ I

,⊔

S =⋂

S,

I � J ⇔ J ⊆ int(I), and

{[p, q] : p, q ∈ & p ≤ q} is a countable basis for I .

The domain I is called the interval domain.

We also have max(I ) ' in the Scott topology.

Dagstuhl August 2004 – p.18/33

Page 59: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

An Important Example of a Domain: I

�The collection of compact intervals of the real line

I

= {[a, b] : a, b ∈

& a ≤ b}

ordered under reverse inclusion

[a, b] v [c, d] ⇔ [c, d] ⊆ [a, b]

is an ω-continuous dcpo.

For directed S ⊆ I

,⊔

S =⋂

S,

I � J ⇔ J ⊆ int(I), and

{[p, q] : p, q ∈ & p ≤ q} is a countable basis for I .

The domain I is called the interval domain.

We also have max(I ) ' in the Scott topology.

Dagstuhl August 2004 – p.18/33

Page 60: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

An Important Example of a Domain: I

�The collection of compact intervals of the real line

I

= {[a, b] : a, b ∈

& a ≤ b}

ordered under reverse inclusion

[a, b] v [c, d] ⇔ [c, d] ⊆ [a, b]

is an ω-continuous dcpo.

For directed S ⊆ I

,⊔

S =⋂

S,

I � J ⇔ J ⊆ int(I), and

{[p, q] : p, q ∈�

& p ≤ q} is a countable basis for I

.

The domain I is called the interval domain.

We also have max(I ) ' in the Scott topology.

Dagstuhl August 2004 – p.18/33

Page 61: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

An Important Example of a Domain: I

�The collection of compact intervals of the real line

I

= {[a, b] : a, b ∈

& a ≤ b}

ordered under reverse inclusion

[a, b] v [c, d] ⇔ [c, d] ⊆ [a, b]

is an ω-continuous dcpo.

For directed S ⊆ I

,⊔

S =⋂

S,

I � J ⇔ J ⊆ int(I), and

{[p, q] : p, q ∈�

& p ≤ q} is a countable basis for I

.

The domain I�

is called the interval domain.

We also have max(I ) ' in the Scott topology.

Dagstuhl August 2004 – p.18/33

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+ < >

Generalizing I

The closed segments of a globally hyperbolic posetX

IX := {[a, b] : a ≤ b & a, b ∈ X}

ordered by reverse inclusion form a continuousdomain with

[a, b] � [c, d] ≡ a � c & d � b.

X has a countable basis iff IX is ω-continuous.

max(IX) ' X

where the set of maximal elements has the relativeScott topology from IX.

Dagstuhl August 2004 – p.19/33

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+ < >

Generalizing I

The closed segments of a globally hyperbolic posetX

IX := {[a, b] : a ≤ b & a, b ∈ X}

ordered by reverse inclusion form a continuousdomain with

[a, b] � [c, d] ≡ a � c & d � b.

X has a countable basis iff IX is ω-continuous.

max(IX) ' X

where the set of maximal elements has the relativeScott topology from IX.

Dagstuhl August 2004 – p.19/33

Page 64: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Generalizing I

The closed segments of a globally hyperbolic posetX

IX := {[a, b] : a ≤ b & a, b ∈ X}

ordered by reverse inclusion form a continuousdomain with

[a, b] � [c, d] ≡ a � c & d � b.

X has a countable basis iff IX is ω-continuous.

max(IX) ' X

where the set of maximal elements has the relativeScott topology from IX.

Dagstuhl August 2004 – p.19/33

Page 65: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Generalizing I

The closed segments of a globally hyperbolic posetX

IX := {[a, b] : a ≤ b & a, b ∈ X}

ordered by reverse inclusion form a continuousdomain with

[a, b] � [c, d] ≡ a � c & d � b.

X has a countable basis iff IX is ω-continuous.

max(IX) ' X

where the set of maximal elements has the relativeScott topology from IX.

Dagstuhl August 2004 – p.19/33

Page 66: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Spacetime from a discrete ordered set

If we have a countable dense subset C of M, aglobally hyperbolic spacetime, then we can view theinduced causal order on C as defining a discreteposet. An ideal completion construction in domaintheory, applied to a poset constructed from C yields adomain IC with

max(IC) ' M

where the set of maximal elements have the Scotttopology. Thus from a countable subset of themanifold we can reconstruct the whole manifold.

We do not know any conditions that allow us to lookat a given poset and say that it arises as a densesubset of a manifold, globally hyperbolic orotherwise.

Dagstuhl August 2004 – p.20/33

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+ < >

Spacetime from a discrete ordered set

If we have a countable dense subset C of M, aglobally hyperbolic spacetime, then we can view theinduced causal order on C as defining a discreteposet. An ideal completion construction in domaintheory, applied to a poset constructed from C yields adomain IC with

max(IC) ' M

where the set of maximal elements have the Scotttopology. Thus from a countable subset of themanifold we can reconstruct the whole manifold.

We do not know any conditions that allow us to lookat a given poset and say that it arises as a densesubset of a manifold, globally hyperbolic or otherwise.

Dagstuhl August 2004 – p.20/33

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+ < >

Compactness of the space of causal curves

A fundamental result in relativity is that the space ofcausal curves between points is compact on aglobally hyperbolic spacetime. We use domains asan aid in proving this fact for any globally hyperbolicposet. This is the analogue of a theorem of Sorkinand Woolgar: they proved it for K-causalspacetimes; we did it for globally hyperbolic posets.

The Vietoris topology on causal curves arises as thenatural counterpart to the manifold topology onevents, so we can understand that its use by Sorkinand Woolgar is very natural.

The causal curves emerge as the maximal elementsof a natural domain; in fact a “powerdomain”: adomain-theoretic analogue of a powerset.

Dagstuhl August 2004 – p.21/33

Page 69: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Compactness of the space of causal curves

A fundamental result in relativity is that the space ofcausal curves between points is compact on aglobally hyperbolic spacetime. We use domains asan aid in proving this fact for any globally hyperbolicposet. This is the analogue of a theorem of Sorkinand Woolgar: they proved it for K-causalspacetimes; we did it for globally hyperbolic posets.

The Vietoris topology on causal curves arises as thenatural counterpart to the manifold topology onevents, so we can understand that its use by Sorkinand Woolgar is very natural.

The causal curves emerge as the maximal elementsof a natural domain; in fact a “powerdomain”: adomain-theoretic analogue of a powerset.

Dagstuhl August 2004 – p.21/33

Page 70: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Compactness of the space of causal curves

A fundamental result in relativity is that the space ofcausal curves between points is compact on aglobally hyperbolic spacetime. We use domains asan aid in proving this fact for any globally hyperbolicposet. This is the analogue of a theorem of Sorkinand Woolgar: they proved it for K-causalspacetimes; we did it for globally hyperbolic posets.

The Vietoris topology on causal curves arises as thenatural counterpart to the manifold topology onevents, so we can understand that its use by Sorkinand Woolgar is very natural.

The causal curves emerge as the maximal elementsof a natural domain; in fact a “powerdomain”: adomain-theoretic analogue of a powerset.

Dagstuhl August 2004 – p.21/33

Page 71: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Globally Hyperbolic Posets and Interval Domains

One can define categories of globally hyperbolicposets and an abstract notion of “interval domain”:these can also be organized into a category.

These two categories are equivalent.

Thus globally hyperbolic spacetimes are domains -not just posets - but

not with the causal order but, rather, with the ordercoming from the notion of intervals; i.e. from notionsof approximation.

Dagstuhl August 2004 – p.22/33

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+ < >

Globally Hyperbolic Posets and Interval Domains

One can define categories of globally hyperbolicposets and an abstract notion of “interval domain”:these can also be organized into a category.

These two categories are equivalent.

Thus globally hyperbolic spacetimes are domains -not just posets - but

not with the causal order but, rather, with the ordercoming from the notion of intervals; i.e. from notionsof approximation.

Dagstuhl August 2004 – p.22/33

Page 73: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Globally Hyperbolic Posets and Interval Domains

One can define categories of globally hyperbolicposets and an abstract notion of “interval domain”:these can also be organized into a category.

These two categories are equivalent.

Thus globally hyperbolic spacetimes are domains -not just posets - but

not with the causal order but, rather, with the ordercoming from the notion of intervals; i.e. from notionsof approximation.

Dagstuhl August 2004 – p.22/33

Page 74: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Globally Hyperbolic Posets and Interval Domains

One can define categories of globally hyperbolicposets and an abstract notion of “interval domain”:these can also be organized into a category.

These two categories are equivalent.

Thus globally hyperbolic spacetimes are domains -not just posets - but

not with the causal order but, rather, with the ordercoming from the notion of intervals; i.e. from notionsof approximation.

Dagstuhl August 2004 – p.22/33

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+ < >

Interval Posets

An interval poset D has two functionsleft : D → max(D) and right : D → max(D) such that

(∀x ∈ D)x = left(x) u right(x).

The union of two intervals with a common endpoint isanother interval and

each point p ∈ max(D) above x determines twosubintervals left(x) u p and p u right(x) with evidentendpoints.

Dagstuhl August 2004 – p.23/33

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+ < >

Interval Posets

An interval poset D has two functionsleft : D → max(D) and right : D → max(D) such that

(∀x ∈ D)x = left(x) u right(x).

The union of two intervals with a common endpoint isanother interval and

each point p ∈ max(D) above x determines twosubintervals left(x) u p and p u right(x) with evidentendpoints.

Dagstuhl August 2004 – p.23/33

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+ < >

Interval Posets

An interval poset D has two functionsleft : D → max(D) and right : D → max(D) such that

(∀x ∈ D)x = left(x) u right(x).

The union of two intervals with a common endpoint isanother interval and

each point p ∈ max(D) above x determines twosubintervals left(x) u p and p u right(x) with evidentendpoints.

Dagstuhl August 2004 – p.23/33

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+ < >

Interval Domains

(D, left, right) with D a continuous dcpo

satisfying some reasonable conditions about how leftand right interact with sups and with � and

intervals are compact: ↑x ∩ max(D) is Scott compact.

Dagstuhl August 2004 – p.24/33

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+ < >

Interval Domains

(D, left, right) with D a continuous dcpo

satisfying some reasonable conditions about how leftand right interact with sups and with � and

intervals are compact: ↑x ∩ max(D) is Scott compact.

Dagstuhl August 2004 – p.24/33

Page 80: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Interval Domains

(D, left, right) with D a continuous dcpo

satisfying some reasonable conditions about how leftand right interact with sups and with � and

intervals are compact: ↑x ∩ max(D) is Scott compact.

Dagstuhl August 2004 – p.24/33

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+ < >

Globally Hyperbolic Posets are an Example

For a globally hyperbolic (X,≤), we defineleft : IX → IX :: [a, b] 7→ [a] andright : IX → IX :: [a, b] 7→ [b].

Lemma: If (X,≤) is a globally hyperbolic poset, then(IX, left, right) is an interval domain.

In essence, we now prove that this is the onlyexample.

Dagstuhl August 2004 – p.25/33

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+ < >

Globally Hyperbolic Posets are an Example

For a globally hyperbolic (X,≤), we defineleft : IX → IX :: [a, b] 7→ [a] andright : IX → IX :: [a, b] 7→ [b].

Lemma: If (X,≤) is a globally hyperbolic poset, then(IX, left, right) is an interval domain.

In essence, we now prove that this is the onlyexample.

Dagstuhl August 2004 – p.25/33

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+ < >

Globally Hyperbolic Posets are an Example

For a globally hyperbolic (X,≤), we defineleft : IX → IX :: [a, b] 7→ [a] andright : IX → IX :: [a, b] 7→ [b].

Lemma: If (X,≤) is a globally hyperbolic poset, then(IX, left, right) is an interval domain.

In essence, we now prove that this is the onlyexample.

Dagstuhl August 2004 – p.25/33

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+ < >

The category of Interval Domains

The category IN of interval domains and commutativemaps is given by

objects Interval domains (D, left, right).

arrows Scott continuous f : D → E that commute withleft and right, i.e., such that both

DleftD

- D

E

f

?

leftE- E

f

?

andDagstuhl August 2004 – p.26/33

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+ < >

The category of Interval Domains cont.

Dright

D - D

E

f

?

rightE

- E

f

?

commute.

identity 1 : D → D.

composition f ◦ g.

Dagstuhl August 2004 – p.27/33

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+ < >

The Category GlobHyP

The category GlobHyP is given by

objects Globally hyperbolic posets (X,≤).

arrows Continuous in the interval topology, monotone.

identity 1 : X → X.

composition f ◦ g.

Dagstuhl August 2004 – p.28/33

Page 87: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

From GlobHyP to IN

The correspondence I : GlobHyP → IN given by

(X,≤) 7→ (IX, left, right)

(f : X → Y ) 7→ (f̄ : IX → IY )

is a functor between categories.

Dagstuhl August 2004 – p.29/33

Page 88: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

From IN to GlobHyP

Given (D, left, right) we have a poset (max(D),≤)where the order on the maximal elements is given by:

a ≤ b ≡ (∃x ∈ D) a = left(x) & b = right(x).

After a five page long proof (due entirely to Keye!) itcan be shown that (max(D),≤) is always a globallyhyperbolic poset.

Showing that this gives an equivalence of categoriesis easy.

Dagstuhl August 2004 – p.30/33

Page 89: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

From IN to GlobHyP

Given (D, left, right) we have a poset (max(D),≤)where the order on the maximal elements is given by:

a ≤ b ≡ (∃x ∈ D) a = left(x) & b = right(x).

After a five page long proof (due entirely to Keye!) itcan be shown that (max(D),≤) is always a globallyhyperbolic poset.

Showing that this gives an equivalence of categoriesis easy.

Dagstuhl August 2004 – p.30/33

Page 90: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

From IN to GlobHyP

Given (D, left, right) we have a poset (max(D),≤)where the order on the maximal elements is given by:

a ≤ b ≡ (∃x ∈ D) a = left(x) & b = right(x).

After a five page long proof (due entirely to Keye!) itcan be shown that (max(D),≤) is always a globallyhyperbolic poset.

Showing that this gives an equivalence of categoriesis easy.

Dagstuhl August 2004 – p.30/33

Page 91: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Summary

We can recover the topology from the order.

We can reconstruct the spacetime from a countabledense subset.

We can characterise causal simplicity ordertheoretically.

We can prove the Sorkin-woolgar theorem oncompactness of the space of causal curves.

We have shown that globally hyperbolic posets areessentially a certain kind of domain: generalizing oneof the earliest and most-loved example of acontinuous dcpo.

Dagstuhl August 2004 – p.31/33

Page 92: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Summary

We can recover the topology from the order.

We can reconstruct the spacetime from a countabledense subset.

We can characterise causal simplicity ordertheoretically.

We can prove the Sorkin-woolgar theorem oncompactness of the space of causal curves.

We have shown that globally hyperbolic posets areessentially a certain kind of domain: generalizing oneof the earliest and most-loved example of acontinuous dcpo.

Dagstuhl August 2004 – p.31/33

Page 93: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Summary

We can recover the topology from the order.

We can reconstruct the spacetime from a countabledense subset.

We can characterise causal simplicity ordertheoretically.

We can prove the Sorkin-woolgar theorem oncompactness of the space of causal curves.

We have shown that globally hyperbolic posets areessentially a certain kind of domain: generalizing oneof the earliest and most-loved example of acontinuous dcpo.

Dagstuhl August 2004 – p.31/33

Page 94: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Summary

We can recover the topology from the order.

We can reconstruct the spacetime from a countabledense subset.

We can characterise causal simplicity ordertheoretically.

We can prove the Sorkin-woolgar theorem oncompactness of the space of causal curves.

We have shown that globally hyperbolic posets areessentially a certain kind of domain: generalizing oneof the earliest and most-loved example of acontinuous dcpo.

Dagstuhl August 2004 – p.31/33

Page 95: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Summary

We can recover the topology from the order.

We can reconstruct the spacetime from a countabledense subset.

We can characterise causal simplicity ordertheoretically.

We can prove the Sorkin-woolgar theorem oncompactness of the space of causal curves.

We have shown that globally hyperbolic posets areessentially a certain kind of domain: generalizing oneof the earliest and most-loved example of acontinuous dcpo.

Dagstuhl August 2004 – p.31/33

Page 96: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Summary

We can recover the topology from the order.

We can reconstruct the spacetime from a countabledense subset.

We can characterise causal simplicity ordertheoretically.

We can prove the Sorkin-woolgar theorem oncompactness of the space of causal curves.

We have shown that globally hyperbolic posets areessentially a certain kind of domain: generalizing oneof the earliest and most-loved example of acontinuous dcpo.

Dagstuhl August 2004 – p.31/33

Page 97: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Conclusions

Domain theoretic methods are fruitful in this setting.

The fact that globally hyperbolic posets are intervaldomains gives a sensible way of thinking of“approximations” to spacetime points in terms ofintervals. Gives us a way to understand coarsegraining.

Dagstuhl August 2004 – p.32/33

Page 98: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

Conclusions

Domain theoretic methods are fruitful in this setting.

The fact that globally hyperbolic posets are intervaldomains gives a sensible way of thinking of“approximations” to spacetime points in terms ofintervals. Gives us a way to understand coarsegraining.

Dagstuhl August 2004 – p.32/33

Page 99: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

What is to be done?

There is a notion of measurement on a domain; away of adding quantitative information. This wasinvented by Keye Martin. We are trying to see if thereis a natural measurement on a domain thatcorresponds to spacetime volume of an interval ormaximal geodesic length in an interval from whichthe rest of the geometry may reappear.

We would like to understand conditions that allow usto tell if a given poset came from a manifold. Can welook at a poset and discern a “dimension”? Perhapsthis will be a fusion of topology and combinatorics.

Understand the quantum theory of causal sets.

Destroy string theory!

Dagstuhl August 2004 – p.33/33

Page 100: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

What is to be done?

There is a notion of measurement on a domain; away of adding quantitative information. This wasinvented by Keye Martin. We are trying to see if thereis a natural measurement on a domain thatcorresponds to spacetime volume of an interval ormaximal geodesic length in an interval from whichthe rest of the geometry may reappear.

We would like to understand conditions that allow usto tell if a given poset came from a manifold. Can welook at a poset and discern a “dimension”? Perhapsthis will be a fusion of topology and combinatorics.

Understand the quantum theory of causal sets.

Destroy string theory!

Dagstuhl August 2004 – p.33/33

Page 101: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

What is to be done?

There is a notion of measurement on a domain; away of adding quantitative information. This wasinvented by Keye Martin. We are trying to see if thereis a natural measurement on a domain thatcorresponds to spacetime volume of an interval ormaximal geodesic length in an interval from whichthe rest of the geometry may reappear.

We would like to understand conditions that allow usto tell if a given poset came from a manifold. Can welook at a poset and discern a “dimension”? Perhapsthis will be a fusion of topology and combinatorics.

Understand the quantum theory of causal sets.

Destroy string theory!

Dagstuhl August 2004 – p.33/33

Page 102: A domain of spacetime intervals for General Relativityprakash/Talks/gr-slides.pdfViewpoint Understand the role of order in analysing the causal structure of spacetime. Reconstruct

+ < >

What is to be done?

There is a notion of measurement on a domain; away of adding quantitative information. This wasinvented by Keye Martin. We are trying to see if thereis a natural measurement on a domain thatcorresponds to spacetime volume of an interval ormaximal geodesic length in an interval from whichthe rest of the geometry may reappear.

We would like to understand conditions that allow usto tell if a given poset came from a manifold. Can welook at a poset and discern a “dimension”? Perhapsthis will be a fusion of topology and combinatorics.

Understand the quantum theory of causal sets.

Destroy string theory!

Dagstuhl August 2004 – p.33/33


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