Tits Metric
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In mathematics, the Tits metric is a
metric Metric or metrical may refer to: * Metric system, an internationally adopted decimal system of measurement * An adjective indicating relation to measurement in general, or a noun describing a specific type of measurement Mathematics In mathem ...
defined on the ideal boundary of an
Hadamard space In geometry, an Hadamard space, named after Jacques Hadamard, is a non-linear generalization of a Hilbert space. In the literature they are also equivalently defined as complete CAT(0) spaces. A Hadamard space is defined to be a nonempty complete ...
(also called a complete
CAT(0) space In mathematics, a \mathbf(k) space, where k is a real number, is a specific type of metric space. Intuitively, triangles in a \operatorname(k) space are "slimmer" than corresponding "model triangles" in a standard space of constant curvature k. I ...
). It is named after
Jacques Tits Jacques Tits () (12 August 1930 – 5 December 2021) was a Belgian-born French mathematician who worked on group theory and incidence geometry. He introduced Tits buildings, the Tits alternative, the Tits group, and the Tits metric. Life an ...
.


Ideal boundary of an Hadamard space

Let (''X'', ''d'') be an Hadamard space. Two geodesic rays ''c''1, ''c''2 : , ∞→ ''X'' are called asymptotic if they stay within a certain distance when traveling, i.e. :\sup_ d(c_1(t), c_2(t)) < \infty. Equivalently, the
Hausdorff distance In mathematics, the Hausdorff distance, or Hausdorff metric, also called Pompeiu–Hausdorff distance, measures how far two subsets of a metric space are from each other. It turns the set of non-empty compact subsets of a metric space into a me ...
between the two rays is finite. The asymptotic property defines an equivalence relation on the set of geodesic rays, and the set of equivalence classes is called the ideal boundary ∂''X'' of ''X''. An equivalence class of geodesic rays is called a boundary point of ''X''. For any equivalence class of rays and any point ''p'' in ''X'', there is a unique ray in the class that issues from ''p''.


Definition of the Tits metric

First we define an angle between boundary points with respect to a point ''p'' in ''X''. For any two boundary points \xi_1, \xi_2 in ∂''X'', take the two geodesic rays ''c''1, ''c''2 issuing from ''p'' corresponding to the two boundary points respectively. One can define an angle of the two rays at ''p'' called the Alexandrov angle. Intuitively, take the triangle with vertices ''p'', ''c''1(''t''), ''c''2(''t'') for a small ''t'', and construct a triangle in the flat plane with the same side lengths as this triangle. Consider the angle at the vertex of the flat triangle corresponding to ''p''. The limit of this angle when ''t'' goes to zero is defined as the Alexandrov angle of the two rays at ''p''. (By definition of a CAT(0) space, the angle monotonically decreases as ''t'' decreases, so the limit exists.) Now we define \angle_p(\xi_1, \xi_2) to be this angle. To define the angular metric on the boundary ∂''X'' that does not depend on the choice of ''p'', we take the supremum over all points in ''X'' :\angle(\xi_1, \xi_2) := \sup_\angle_p(\xi_1, \xi_2). The Tits metric ''d''T is the length metric associated to the angular metric, that is for any two boundary points, the Tits distance between them is the
infimum In mathematics, the infimum (abbreviated inf; plural infima) of a subset S of a partially ordered set P is a greatest element in P that is less than or equal to each element of S, if such an element exists. Consequently, the term ''greatest lo ...
of lengths of all the curves on the boundary that connect them measured in the angular metric. If there is no such curve with finite length, the Tits distance between the two points is defined as infinity. The ideal boundary of ''X'' equipped with the Tits metric is called the Tits boundary, denoted as ∂T''X''. For a complete CAT(0) space, it can be shown that its ideal boundary with the angular metric is a complete CAT(1) space, and its Tits boundary is also a complete CAT(1) space. Thus for any two boundary points \xi_1, \xi_2 such that \angle(\xi_1, \xi_2) < \pi, we have :d_\mathrm(\xi_1, \xi_2) = \angle(\xi_1,\xi_2), and the points can be joined by a unique geodesic segment on the boundary. If the space is
proper Proper may refer to: Mathematics * Proper map, in topology, a property of continuous function between topological spaces, if inverse images of compact subsets are compact * Proper morphism, in algebraic geometry, an analogue of a proper map for ...
, then any two boundary points at finite Tits distance apart can be joined by a geodesic segment on the boundary.


Examples

*For a
Euclidean space Euclidean space is the fundamental space of geometry, intended to represent physical space. Originally, that is, in Euclid's ''Elements'', it was the three-dimensional space of Euclidean geometry, but in modern mathematics there are Euclidean ...
E''n'', its Tits boundary is the unit sphere ''S''''n'' - 1. * An Hadamard space ''X'' is called a visibility space if any two distinct boundary points are the endpoints of a geodesic line in ''X''. For such a space, the angular distance between any two boundary points is equal to π, so there is no curve with finite length on the ideal boundary that connects any two distinct boundary points, which means that the Tits distance between any two of them is infinity.


References

* {{cite book , last = Bridson , first = Martin R. , author2=Haefliger, André , title = Metric spaces of non-positive curvature , series = Grundlehren der Mathematischen Wissenschaften undamental Principles of Mathematical Sciences319 , publisher = Springer-Verlag , location = Berlin , year = 1999 , pages = xxii+643 , isbn = 3-540-64324-9 , mr = 1744486 Metric geometry