On the space of compact diamonds of Lorentzian length spaces
Waldemar Barrera, Luis Montes de Oca, Didier A. Solis

TL;DR
This paper introduces new product constructions for Lorentzian pre-length spaces and demonstrates that the space of causal diamonds can be endowed with a Lorentzian length space structure, revealing its geodesic and global hyperbolicity properties.
Contribution
It develops the concepts of taxicab and uniform products for Lorentzian spaces and applies them to analyze the geometry and causal structure of the space of causal diamonds.
Findings
The space of causal diamonds is a Lorentzian length space.
The space is geodesic for complete X.
The space is globally hyperbolic for complete X.
Abstract
In this work we introduce the taxicab and uniform products for Lorentzian pre-length spaces. We further use these concepts to endow the space of causal diamonds with a Lorentzian length space structure, closely relating its causal properties with its geometry as a metric space furnished with its associated Hausdorff distance. Among the general results, we show that this space is geodesic and globally hyperbolic for complete .
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Taxonomy
TopicsGeometric Analysis and Curvature Flows · Geometric and Algebraic Topology · Advanced Differential Geometry Research
On the space of compact diamonds of Lorentzian length spaces
Waldemar Barrera, Luis Montes de Oca, Didier A. Solis
Abstract
In this work we introduce the taxicab and uniform products for Lorentzian pre-length spaces. We further use these concepts to endow the space of causal diamonds with a Lorentzian length space structure, closely relating its causal properties with its geometry as a metric space furnished with its associated Hausdorff distance. Among the general results, we show that this space is geodesic and globally hyperbolic for complete length space .
Keywords: Lorentzian length spaces, Causality, Hyperspaces
MSC Classification 53C23, 53C22, 51F30, 54F16, 83C99
1 Introduction
In the past few years there has been a remarkable interest in exploring synthetic alternatives to well established notions arising in Lorentzian geometry. The seminal work of Kunzinger and Sämann on Lorentzian length spaces [33] has paved the way to introduce such methods in the realm of Relativity, in which other promising approaches are currently been developed, as is the case of Lorentzian metric spaces [41] or almost Lorentzian length spaces [42] just to mention a few. These developments are suitable candidates to provide useful tools for the analysis of physical scenarios were the standard regular (at least ) framework is no longer assumed, either from the theoretical onset —for instance, when considering [21, 23, 35, 36], [22, 32] or even [19, 16, 24, 20, 48] metrics— or in the interest of further our understanding of the most recent observation of black hole merging and gravitational waves [18, 37].
A cornerstone in Kunzinger and Sämann development consists in the axiomatization of the fundamental causal properties of spacetime through the notion of a Lorentzian pre-length space, which can be regarded as a refinement of the concept of causal space first introduced by Kroenheimer and Penrose in the early years of Mathematical Relativity [31]. As an example of the value of building a causal theory on axiomatic grounds we cite the causet approach to Quantum Gravity (see [50] and references therein), in which no spacetime metric is considered at all. The existence of a time separation function, as proposed in [33], opens the scope of applications to settings where no regular spacetime metric is given a priori, as is the case of Lorentzian manifolds with timelike boundary [2], causal completions of globally hyperbolic spacetimes [1] or even some class of contact structures [27].
Moreover, by considering a suitable class of causal curves, a synthetic notion of curvature bounds is defined and its relation to its geodesic structure analyzed in a way akin to the well established theory of Alexandrov and CAT(k) metric length spaces [12]. In this regard, several results inspired in this theory are currently been pursued in the Lorentzian pre-length space scenario. For instance, Toponogov type triangle comparison [6], or the existence of hyperbolic angles and exponential maps [10]. Applications of these results include gluing and amalgamation [9], as well as a splitting theorem that generalizes the landmark result for Lorentzian manifolds with non-positive timelike sectional curvature [11].
Indeed, curvature bounds are essential in some of the most remarkable results pertaining to metric length spaces, such as the celebrated pre-compactness theorems of Gromov [26, 47]. Recall that these results can be interpreted in terms of stability of curvature bounds with respect to Gromov-Hausdorff convergence. Thus, it is natural to explore the stability of different aspects of the theory of Lorentzian length spaces under suitable notions of convergence. For instance, in [34] Kunzinger and Steinbauer address the behaviour of curvature bounds under Gromov Hausdorff convergence of a class of warped product spacetimes via the null distance first introduced by Sormani and Vega [49]. Another key aspect of the theory closely tied to the notion of Gromov distance was studied in [39], where McCann and Sämann establish notions of Hausdorff measure and dimension in the context of Lorentzian length spaces. Let us emphasize that in this work causal diamonds play a fundamental role just as (compact) metric balls do in the context of metric length spaces.
In this work we aim at providing a first glance on the structure of the space of causal diamonds of a globally hyperbolic Lorentzian pre-length space , furnished with the Hausdorff distance induced by . Recall that the metric spaces thus obtained from families of compact subsets of a metric space –or isometry classes thereof– are commonly referred to as hyperspaces and their study is cornerstone in the theory of continua [44, 29] as well as infinite dimensional topological manifolds and function spaces [14, 51]. From the topological point of view, the celebrated theorem of Curtis establishes that the hyperspace of compact subsets of is homeomorphic to the punctured Hilbert cube [17], and a similar characterization holds for the hyperspace of isometry classes under the Gromov Hausdorff distance [4, 5]. In spite of these accurate topological descriptions, the geodesic structure of hyperspaces remains unexplored for the most part. For instance, only recently the intrinsic nature of has been established [15, 30]. Moreover, by the well known Gromov’s Embedding Lemma, a family of compact metric spaces can be embedded in a space endowed with its Hausdorff distance [25]. Thus, exploring the geodesic structure of the space of causal diamonds with respect to the Hausdorff distance is an important step in the program of understanding the geometry of its corresponding Gromov Hasudorff hyperspace. By focusing on the class of Lorentzian taxicab spaces we provide a precise description of the space of causal diamonds of Minkowski space and establish that it has the structure of a globally hyperbolic Lorentzian length space, and thus it satisfies de Avez-Seifert property. Moreover, we give explicit parametrizations for maximal curves joining any pair of causally related diamonds.
This paper is organized as follows. In Section 2 we state the basic definitions and establish the notation to be used throughout this work. In Section 3 we describe the Lorentzian taxicab product of a Lorentzian pre-length space and a metric space; as well as the uniform Lorentzian product of two Lorentzian pre-length spaces, and study in more detail the case of the Lorentzian taxicab product . In Section 4 we prove that the hyperspace of compact subsets of a Lorentzian pre-length space can be endowed with such a structure. Finally, as application of this fundamental result, in Section 5 we study the space of causal diamonds and prove that it admits a structure of globally hyperbolic Lorentzian Length space, give explicit parametrization for a family of maximal timelike curves and provide an explicit realization as a subspace of a Lorentzian uniform product.
2 Preliminaries
In this section we set up the basic notions on Lorentzian length spaces and the Hausdorff distance.
2.1 Lorentzian length spaces
There are two fundamental aspects in mathematical relativity that are rooted in Lorentzian geometry. In one hand we have the causal structure, and in the other, the locally Minkowskian nature of spacetime; the former coming from the causal character of vectors and the latter from properties of the exponential map. Any attempt to axiomatize the fundamental properties of spacetime must take into account these issues in a way that does not depend on the existence of a smooth metric tensor. In their seminal work Kunzinger and Sämann develop an original notion of Lorentzian length of causal curves by encoding causality in the definition of Lorentzian pre-length space and by describing the local structure via the so called localizing neighborhoods (see [33] for a detailed account).
Definition 2.1**.**
A Lorentzian pre-length space is quintuple where is a metric space and
* and are two relations in that satisfy*
- •
* is a pre-order.*
- •
* is a transitive relation containing .111In [31] Kronheimer and Penrose define a causal space as a triple that satisfies properties property (1) plus the causality axiom: and .* 2. 2.
* is a lower semi-continuous function for which the reverse triangle inequality holds:*
[TABLE]
In this setting, and are the chronological and causal relations, respectively; whereas is called a time separation function. The relations , enable us to define the chronological and causal sets in the standard way:
[TABLE]
Example 2.2**.**
The set of real numbers is a Lorentzian pre-length space when we define the chronological and casual relations by and , respectively. Here and
[TABLE]
In what follows, we will denote this Lorentzian pre-length space by .
Example 2.3**.**
Any smooth spacetime is a Lorentzian pre-length space when we consider any metric inducing the manifold topology. The relations and , as well as the time separation function are the standard ones constructed from the Lorentzian metric .
Lorentzian pre-length spaces have just enough structure to guarantee the most basic results in causality theory. As straightforward consequence of the definition we have the following lemma.
Lemma 2.4**.**
Let be a Lorentzian pre-length space, then
The chronological sets , are open in . 2. 2.
If or then . (Push-up property).
The relations , can be used to define the class of causal curves in a Lorentzian pre-length space. We say that a Lipschitz continuous curve is future timelike (causal) if for any we have (). Past timelike and causal curves are defined analogously. If a curve is causal and no pair of its points are chronologically related we call it null222Observe that if a smooth spacetime does not have closed causal curves then this notion of causal character of curves coincides with the usual one.. Notice that since the relations , are not defined in terms of curves, it might happen that causally related points can not be joined by any causal curve. A Lorentzian pre-length space for which any chronologically (causally) related pair of points there exists a timelike (causal) curve connecting them is called causally path connected.
Normal neighborhoods are essential for describing the local geometry of a smooth spacetime. The analog for Lorentzian length spaces is the concept of localizing neighborhoods.
Definition 2.5**.**
Let be a causally path connected Lorentzian pre-length space. A neighborhood around is localizing if there exists a continuous functions for which
* is a Lorentzian pre-length space, where , denote the relations induced by , in 333That is, () if and only if there exists a future timelike (causal) curve in from to .* 2. 2.
, for all . 3. 3.
All causal curves contained in have uniformly bounded -length. 4. 4.
For all with there exists a future causal curve contained in such that and whose -length is maximal among all future causal curves from to lying in .
If in addition, the following holds: if then is timelike and for each causal curve containing a null segment, then we say the neighborhood is regular.
Roughly speaking, a Lorentzian length space is a pre-length space with a local structure provided by localizing neighborhoods and whose time separation function can be recovered from the -length of curves. In precise terms, we have the following (see Definitions 3.22 in [33] and 2.27 in [2]).
Definition 2.6**.**
A causally path connected Lorentzian pre-length space for which:
Every point has a localizing neighborhood . 2. 2.
Every point has a neighborhood in which the relation is closed444This condition is referred to as being locally causally closed.**. 3. 3.
, for all , where
[TABLE]
is called a Lorentzian length space.
Remark 2.7**.**
Notice that if there is a -length realizing causal curve (that is, ) joining any two causally related points, then condition (3) in Definition 2.6 is satisfied. If this is the case, such curves are called maximal and we say that is a geodesic Lorentzian pre-length space666In Lorentzian geometry, this condition is also known as the Avez-Seifert property.
Examples of Lorentzian length spaces include strongly causal smooth spacetimes [33], spacetimes with timelike boundary [2], causally plain spacetimes with metrics [16, 20] and cone structures [40, 3].
A causal hierarchy for Lorentzian length spaces can be established in close resemblance to the standard causal hierarchy of smooth spacetimes [2]. However, some of the most meaningful levels –like strong causality, non-imprisonment and globally hyperbolicity– can still be defined for Lorentzian pre-length spaces in general [33].
Definition 2.8**.**
A Lorentzian pre-length space is non-totally imprisoning if there is an upper bound for all the -lengths of causal curves contained in a compact set . A non-totally imprisoning Lorentzian pre-length space is globally hyperbolic if all its causal diamonds are compact.
As expected, globally hyperbolic Lorentzian length spaces share in common with their smooth counterparts some remarkable features. For instance, the Avez-Seifert property and the continuity of the time separation [2, 33].
2.2 Hausdorff distance
Let be a metric space. We define the length of a (continuous) curve as
[TABLE]
where the supremum is taken over all partitions , , of the closed interval and
[TABLE]
is the length of the polygonal curve with vertices on .
A length space is a metric space in which the metric is induced by the length functional . In precise terms, a metric space is a length space if
[TABLE]
A curve that realizes distance between any pair of its points –that is, if – is called a geodesic segment. If every pair of points in can be joined by a geodesic segment we say that the space is geodesic. In such a case we consider all geodesic segments parameterized with respect to arc length. Let us recall that any complete and locally compact length space is geodesic (see for instance Thrm. 2.5.23 [12]).
The Hausdorff distance of the metric space is defined on the set of closed subsets of as
[TABLE]
where is the (open) metric ball of radius centered at and denotes the tubular neighborhood of of radius and . We now list some standard results pertaining tubular neighborhoods and the Hausdorrf distance that are useful for explicit computations
Lemma 2.9**.**
Let be a locally compact and complete length space. Then for every compact subset of we have:
* is compact for every .* 2. 2.
* for every .* 3. 3.
, 4. 4.
** 5. 5.
There exist midpoints: for every there is with . 6. 6.
Closed -balls are compact.
Given a metric space , the set
[TABLE]
is commonly referred to as the hyperspace of compact sets of . When furnished with the Hausdorff distance, its topological structure is one of the main objects of study in the theory of continua. Here we establish one of its most important geometric aspect, namely, that is indeed geodesic.
Proposition 2.10**.**
Let be a locally compact and complete length space. For every two compact sets with , the path given by
[TABLE]
is a geodesic segment connecting and .
Proof.
Since then there is a strictly increasing sequence such that
[TABLE]
for all . Thus . From this, . Similarly . Thus
[TABLE]
and .
Now we show that for any we have . Since , are compact, there exist , such that . Let be the point in the segment joining and that satisfies and . Thus
[TABLE]
Hence and , therefore .
We now show that . Let us consider . Since there exists such that . Moreover, there exists a point in the segment joining and such thta and . Hence
[TABLE]
and therefore . Hence
[TABLE]
and . Now, let , thus and . Hence . As a consequence, . We can show in a similar fashion that . Thus
[TABLE]
and the relations and follow. Along the same lines of the previous argument we can show that for all we have
[TABLE]
On the other hand, by Lemma 2.9 we also have
[TABLE]
and hence . ∎
3 Constructions
This section is devoted to general constructions that enable us to build new pre-length spaces from old. The motivation behind these construction is twofold: first, to provide new ways to find examples, and second, to establish a general framework for future applications, most notably, in the study of metric properties of Lorentzian pre-length spaces.
3.1 Lorentzian taxicab product
The following construction will be key in examining the space of causal diamonds of Minkowski space. Recall that the taxicab product of the metric spaces , is the metric space where for all ,
[TABLE]
Definition 3.1** (Lorentzian taxicab product space).**
Let be a metric space and a Lorentzian pre-length space. The Lorentzian taxicab product is given by
- •
* if and only if .*
- •
* if and only if and .*
- •
[TABLE]
Proposition 3.2**.**
Let and be a metric space and a Lorentzian pre-length space, respectively. Then the Lorentzian taxicab product is a Lorentzian pre-length space.
Proof.
First, if then . The relation is clearly reflexive. For and we have , thus
[TABLE]
therefore and is a transitive relation. Similarly we can establish that is transitive as well. Now, it follows from the definition that if and only if . It remains to check that is a lower semicontinuous function with respect to and satisfies the reverse triangle inequality. In order to prove the former, let us fix and . Since is semicontinuous at , there exists such that if , then Set and let us take such that
[TABLE]
Thus and similarly , and . Hence , and thus . On the other hand, by the triangle inequality we get
[TABLE]
In conclusion
[TABLE]
The above inequality readily implies that for we have
[TABLE]
On the other hand, in case of the same statement holds true because in that case or , therefore
[TABLE]
Finally, if then Thus, the proof of semi-continuity is complete.
Now we tackle the reverse triangle inequality. Let , then
[TABLE]
∎
Now let us focus on the Lorentzian taxicab product space , where is a locally compact and complete geodesic length space. Thus we have
[TABLE]
Remark 3.3**.**
Notice that if is a geodesically complete Riemannian manifold then the causal and chronological relations of the Lorentzian length space and the standard (Lorentzian) product manifold agree, thus their structures as causal sets are identical. In particular, their respective causal diamonds coincide as point sets777Recall that the spacetime is globally hyperbolic if and only is complete (see [45]) . However, their manifestly different time separation functions give rise to two very different geodesic structures. Indeed, take for instance with its standard Euclidean metric. Then any pair of chronologically related points in Minkowski space can be connected by a unique maximal geodesic, namely, the straight line segment joining them. On the other hand, in the Lorentzian taxicab product there might be infinitely many maximal geodesic segments joining any pair of chronologically related points. Indeed any curve of the form with monotone and strictly monotone is maximal. What is more, there are in causal non-timelike curves which turn out to be maximal [6] (see Figure 1).
Notice that due to Remark 3.3, the causal diamonds in are compact. In fact, we will show next that is a geodesic Lorentzian length space. Further, if is complete then is globally hyperbolic. We start by providing explicit parametrizations for maximal causal curves joining any two causally related points.
Lemma 3.4**.**
For every two points and in with let and be a geodesic segment parametrized by arclength.
If , then and defined as
[TABLE]
is a maximal future-directed timelike curve from to . 2. 2.
If , then defined as
[TABLE]
is a maximal future-directed null curve from to .
Proof.
First, since has been parametrized by arclength, then for every we have
[TABLE]
thus is a non-constant Lipschitz continuous function. In fact, this leads to , therefore is a geodesic segment connecting with . On the other hand observe that
[TABLE]
thus and the same inequality implies , hence is a future-directed maximal timelike curve. The proof of the null case is analogous.∎
Theorem 3.5**.**
The Lorentzian taxicab product space is a globally hyperbolic Lorentzian length space.
Proof.
The space is a geodesic causally path connected Lorentzian pre-length space from Proposition 3.2 and Lemma 3.4.
Now let , and consider the set
[TABLE]
We now show is a localizing neighborhood around . Since and are open, then is open as well. If satisfy then the curve constructed in Lemma 3.4 is a future-directed maximal causal curve from to contained in . It follows that
[TABLE]
is a Lorentzian pre-length space that fulfills condition (1) and (4) in Definition 2.6. Moreover, let and be a midpoint of and , hence . Observe that
[TABLE]
thus . We also have
[TABLE]
then and therefore . A similar argument shows that , and hence condition (3) in Definition 2.6 holds as well.
Now, fix a future-directed causal curve with . The curve can be written as where and . Since is causal then and for every . In particular leads to and . Take a partition , thus
[TABLE]
In conclusion, the length of any causal curve contained in satisfies and thus condition (2) in Definition 2.6 holds as well. Hence is localizing.
Finally, take two convergent sequences and with for all . Since it readily follows that , , and similarly , . Thus implies and , hence is locally causally closed. Thus is a geodesic Lorentzian length space.
Now we prove is globally hyperbolic. First, if compact then there exists a number such that
[TABLE]
Let be a future-directed causal curve contained in , then
[TABLE]
Hence is non-totally imprisoning. Finally, we prove that is compact for every . Let be a sequence in , then and , then the sequence is contained in a compact closed ball in . Hence we can choose a subsequence –using a Cantor’s diagonal argument– with . Since and , by taking we conclude . Therefore is compact and the proof is complete. ∎
3.2 Lorentzian uniform product
In analogy with the norm, given two metric spaces and the uniform metric is defined by
[TABLE]
Definition 3.6** (Lorentzian uniform product space).**
Let and be two Lorentzian pre-length spaces. The Lorentzian uniform product space is defined by
- •
* if and only if and .*
- •
* if and only if and .*
- •
[TABLE]
Proposition 3.7**.**
The Lorentzian uniform product is a Lorentzian pre-length space.
Proof.
It is not hard to see that the relations , satisfy the required properties of a pre-length space since both , and , do. If then or and therefore or leading to . In fact if and only if and , which in turn holds if and only if . Thus, it only remains to verify the reverse triangle inequality and lower semicontinuity of with respect to .
We first analyze the lower semicontinuity of . Let and fix . Since is lower semicontinuous at with respect to , we can find such that implies . Choose and suppose
[TABLE]
implying and . Thus
[TABLE]
leading to . Hence
[TABLE]
therefore
[TABLE]
A similar argument enables us to show
[TABLE]
so in conclusion
[TABLE]
thus establishing the lower semicontinuity of at .
Finally, if then and . Then by using the reverse triangle inequality for and we obtain
[TABLE]
and similarly
[TABLE]
Hence
[TABLE]
which finishes the proof of the reverse triangle inequality. ∎
Now we move on in to proving that under some mild assumptions, the uniform product of two Lorentzian length spaces is a Lorentzian length space. A few previous lemmas are in order. First we focus on the geodesic structure of the uniform product.
Remark 3.8**.**
Let , be a curve. First, notice that if and are balls in and , respectively, then the ball agrees with . We immediately conclude that if is locally Lipschitz continuous then so are and . Furthermore, if is a future-directed causal curve, then for all we have implying and . If is not constant then is a future-directed causal curve. Moreover, if is timelike or null then so is .
Lemma 3.9**.**
Let and be two future causal curves in and , respectively. Let us consider for given by . Then defined as is a causal curve in and
[TABLE]
Moreover, if and are timelike and maximal, then is maximal and timelike
Proof.
Note that is future causal since and also are, and , are continuous strictly increasing functions. To analyze the length of curves, fix two partitions and in and , respectively. Thus we induce two partitions and in . Now
[TABLE]
then , and in a similar way we obtain . Therefore
[TABLE]
Now suppose and are both timelike and maximal and , . Then and can be chosen such that and is parametrized by arclength for . Therefore, for a given partition we have
[TABLE]
In conclusion
[TABLE]
Thus and therefore is maximal. ∎
Lemma 3.10**.**
Let and be two Lorentzian pre-length spaces.
- (i)
If and are locally causally closed, then is locally causally closed. 2. (ii)
If and are causally path connected, then is causally path connected. 3. (iii)
If and are regularly localizable, then is localizable. 4. iv)
If there exists timelike maximal curves joining any pair of chronologically related points in both and , then is intrinsic.
Proof.
For (i) observe that the product of two causally closed neighborhoods , containing , is a causally closed neighborhood in . Notice also that . Part (ii) follows from Remark 3.8. Part (iv) is a immediate consequence of Lemma 3.9. Thus we will focus on Part (iii). For every and choose localizing neighborhoods and and their corresponding continuous maps , . We will prove that is a localizing neighborhood and defined as
[TABLE]
satisfies the conditions of Definition 3.16 of [33]. Let be a causal curve contained in , with . Since cannot be constant then and are not simultaneously constant. Since and then there exist with and . Moreover, for a given partition we have
[TABLE]
Then . Moreover, clearly is a Lorentzian pre-length space. Now, if , then
[TABLE]
thus . Similarly . Finally fix , then there exist two timelike maximal curves and with , , , and
[TABLE]
[TABLE]
In conclusion, the curve defined as in Lemma 3.9 satisfy
[TABLE]
∎
Proposition 3.11**.**
Let and be two globally hyperbolic Lorentzian pre-length spaces. Then is a globally hyperbolic Lorentzian pre-length space.
Proof.
If is compact, then there exist two compact sets and with . Let to be a causal curve in , then we can find two causal curves , with . Since and are globally hyperbolic then there are two positive numbers and with and . Therefore, by following a similar argument as in the proof of Lemma 3.10 we conclude
[TABLE]
Thus, is non totally imprisoning. Finally, observe that
[TABLE]
thus the compactness of is a direct consequence of the compactness of and . ∎
From Lemma 3.10 and Proposition 3.11 the following result is immediate.
Corollary 3.12**.**
Let and be two globally hyperbolic regularly localizable Lorentzian pre-length spaces. Then is a globally hyperbolic Lorentzian length space.
4 Hyperspaces as Lorentzian pre-Length spaces
In this section we establish the main results of this work, namely, we endow with a Lorentzian pre-length structure the hyperspaces of compact sets and causal diamonds of a Lorentzian pre-length space with a continuous time separation .
In the context of Lorentzian pre-length spaces, we can define relations and that naturally inherit the properties of a chronological and causal relation, respectively, from those of and . In precise terms we define
- (i)
For , if and only if there is a with and there is a with . 2. (ii)
For , if and only if there is a with and there is a with .
Moreover, for and we define as
[TABLE]
and as888In case and , then we set .
[TABLE]
where
[TABLE]
Definition 4.1**.**
We say that is the Lorentzian hyperspace of compact subsets of .
Remark 4.2**.**
Due to the continuity of we have that and are both non-negative continuous functions. Moreover, for every and there exists such that and .
The following Lemma can be interpreted as analogues for of well known results pertaining to the Hausdorff distance (see for instance Lemma 2.9).
Lemma 4.3**.**
For every , , and we have:
* and .* 2. 2.
. 3. 3.
* if and only if and .* 4. 4.
If then and .
Proof.
In order to prove (1), consider , then there exist and such that
[TABLE]
[TABLE]
therefore and , implying and hence . Thus
[TABLE]
A similar computation shows that .
For point (2), let us denote
[TABLE]
First we will show . Let such that and . Then and , and . Therefore
[TABLE]
Thus which readily implies . Conversely, we want to show . If then we are done, so suppose . Since
[TABLE]
Thus and , and , which means and , hence
[TABLE]
In conclusion, and consequently .
Point (3) is a direct consequence of point (2). Finally point (4) is derived from the definition of and . ∎
Lemma 4.4**.**
If then .
Proof.
If then
[TABLE]
Suppose . Then there exists a sequence of points with when . Since is compact, then there is a convergent subsequence of , and without loss of generality assume that converges itself to a point . Note
[TABLE]
hence for all which means for all , thus . The case can be handled in an analogous way. ∎
Theorem 4.5**.**
The Lorentzian hyperspace is a Lorentzian pre-length space.
Proof.
By Remark 4.2 and Lemma 4.3 (2) we obtain that is a continuous function with respect to . It is clear that if then . Now we focus on the remaining properties of a Lorentzian pre-length space according to Definition 2.1.
In fact, by Lemma 4.4 we have that if then (otherwise cannot be chronologically related to ). On the other hand, if then for all and for all we have and . In conclusion, for all and there are two points and ( and depending on and , respectively) with and , implying . Thus if and only if .
Finally, if let and such that , , and , . Therefore by using point (1) of Lemma 4.3 we have
[TABLE]
and similarly . Thus
[TABLE]
leading to . This last inequality implies
[TABLE]
since and were chosen arbitrarily, thus establishing the reverse triangle inequality.
∎
Let us recall that in a global hyperbolic pre-length space its causal diamonds are compact and its time separation function is finite and continuous. Hence, Proposition 4.5 can be used at once to provide a Lorentzian pre-length structure to the set of causal diamonds of a globally hyperbolic Lorentzian pre-length space. Because of the fundamental role that causal diamonds play in various aspects of mathematical relativity, cuasal theory and Lorentzian geometry, the following is our main result.
Corollary 4.6** (The hyperspace of causal diamonds).**
Let be a globally hyperbolic Lorentzian pre-length space and define
[TABLE]
Then is a Lorentzian pre-length space called the hyperspace of causal diamonds of .
Example 4.7**.**
In [7] the authors show that the hyperspace of closed intervals is isometric to the taxicab metric space where , and the isometry is given by
[TABLE]
Further notice that the hyperspaces of causal diamonds and agree as point sets. Thus, the question as if there exists a Lorentzian analog of the isometry depicted above. We answer this question in the affirmative as follows. In order to find a explicit description of notice that whenever , then , and , which in turn implies that
[TABLE]
Now fix , then
[TABLE]
Therefore
[TABLE]
and similarly
[TABLE]
leading to
[TABLE]
In conclusion, the function is a distance preserving map from the hyperspace of causal diamonds to the Lorentzian taxicab semi-space described in [6].
5 Applications
We move on to study in further detail the hyperspace of causal diamonds , where is a complete geodesic length space. As the following results show, in this scenario we have in fact a geodesic and globally hyperbolic Lorentzian length space. We first show that such hyperspace is geodesic and provide explicit parametrizations of maximal geodesic segments connecting causally related diamonds. A few lemmas are in order. First we describe the relations , in explicit terms for Lorentzian taxicab spaces.
Lemma 5.1**.**
Let us consider the diamonds and for and . Then if and only if and .
Proof.
If , then in virtue of there is with , thus . Similarly, for there is with , hence . Now suppose that and and fix , . Then and , therefore and . Thus . ∎
Proposition 5.2**.**
For every two diamonds and with and , we have
[TABLE]
where is the Hausdorff distance induced by in .
The next result is essential in various instances.
Proof.
Let with and , then and thus
[TABLE]
By combining these last two inequalities we obtain
[TABLE]
Similarly, when we obtain
[TABLE]
Therefore
[TABLE]
which leads to
[TABLE]
By the definition of we conclude
[TABLE]
In order to prove the inequality just note that satisfies and . ∎
We move on to prove that is a geodesic Lorentzian pre-Length space and provide explicit -parametrizations for maximal curves. We follow the same approach as in Lemma 2.10. Thus we need to show first that the tubular neighborhood and that the intersection of two causal diamonds are causal diamonds themselves. The following lemmas deal with these issues.
Lemma 5.3**.**
Let be two points in and . Then for every we have
[TABLE]
where is the closed tubular neighborhood with respect to .
Proof.
First of all, if then due to the compactness of there exists with
[TABLE]
We also have and since . Thus
[TABLE]
implying . Similarly and in conclusion . Conversely, suppose . If then , otherwise or . Assume then . If , let be a geodesic segment connecting with (that is, and ) and take , thus
[TABLE]
therefore and . Moreover,
[TABLE]
since . Hence . Alternatively, if then
[TABLE]
again by . So in this case we have as well. A similar argument proves that if then , thus finishing the proof. ∎
Lemma 5.4**.**
Let , and . Let us denote and . If then
[TABLE]
Proof.
In virtue of Lemma 5.1 it is enough to prove that , which is equivalent to . First, applying Proposition 5.2 we way suppose that
[TABLE]
But , thus
[TABLE]
∎
Proposition 5.5**.**
Let , and . Then defined as
[TABLE]
is a causal curve connecting with and for every .
Proof.
The first part of the proof is an immediate consequence of Lemma 5.4. Now we focus on the second part. Let , then by using Lemma 4.3
[TABLE]
In particular observe that . ∎
We now establish the main result.
Theorem 5.6**.**
Let be a complete geodesic length space. The hyperspace of causal diamonds is a geodesic globally hyperbolic Lorentzian length space.
Proof.
Local causal closedness in follows easily from the corresponding property of and Lemma 5.1. Moreover, Proposition 5.5 guarantees that is causally path connected and intrinsic. Thus, to prove that the hyperspace of causal diamonds is a Lorentzian length space it only remains to prove that is localizable. Indeed, we will show that
[TABLE]
is a localizing neighborhood, where , , and . First, let to be a causal curve contained in , where
[TABLE]
and , . Now, for a partition observe that and by Lemma 5.1. Then, applying Lemma 5.2 we obtain that
[TABLE]
On the other hand, since , it follows that
[TABLE]
Therefore for every causal curve contained in . It is clear that is a Lorentzian pre-length space. If we need to see that . In order to do this, observe that if are some middle points for and , respectively, then belongs to . Similarly we can prove that for every .
First, we need to prove that every causal diamond is compact with respect to the topology induced by on , where and . Let a sequence of diamonds contained in with for every . Then and by applying Lemma 5.1 we obtain and . It follows that and . By using the compactness of and and a diagonal Cantor’s process we are able to find two convergent subsequences and converging to and , respectively. Moreover, the sequence converges to . Since is closed for every diamond in we have that and . This last statement implies that . ∎
We end this section by providing a nice realization of , that in passing reveals a close connection between the Lorentzian taxicab and uniform products.
Theorem 5.7**.**
Let defined as , where . Then is an isometry in and a -preserving map.
Proof.
That is a metric isometry follows directly from its definition and Proposition 5.2. Moreover, is preserving as the following result shows. ∎
Proposition 5.8**.**
Let and two diamonds with , and , then
[TABLE]
Proof.
Let , then
[TABLE]
Thus, for we obtain
[TABLE]
In conclusion we must have
[TABLE]
Since , we can show similarly that
[TABLE]
Also, a similar process lead us
[TABLE]
Then, by the way we defined we have
[TABLE]
∎
Acknowledgments
W. Barrera acknowledges the support of Conacyt under grants SNI 45382 and Ciencia de Frontera 21100. L. Montes recognizes the support of Conacyt under the Becas Nacionales program (783177). D. Solis was partially supported by Conacyt SNI 38368 and UADY-FMAT PTA 2023.
The reference list from the paper itself. Each links out to its DOI / PubMed record.
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