Nondistortion of horospheres in Euclidean buildings and in symmetric spaces (Q1380492)
From MaRDI portal
| This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: Nondistortion of horospheres in Euclidean buildings and in symmetric spaces |
scientific article; zbMATH DE number 1123732
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Nondistortion of horospheres in Euclidean buildings and in symmetric spaces |
scientific article; zbMATH DE number 1123732 |
Statements
Nondistortion of horospheres in Euclidean buildings and in symmetric spaces (English)
0 references
5 January 1999
0 references
The nondistortion of horospheres is an important topic applied in the classification theory of metric spaces. By using the geometry of Euclidean buildings and the asymptotic cone, a necessary and sufficient condition is given here for the nondistortion of a horosphere in an Euclidean building and in a symmetric space. As an application, the theorem of \textit{A. Lubotzky, S. Mozes} and \textit{M. S. Raghunathan} [C. R. Acad. Sci., Paris, Sér. I 317, 735-740 (1993; Zbl 0786.22016)] is proved geometrically.
0 references
symmetric spaces
0 references
nondistortion of horospheres
0 references
Euclidean buildings
0 references
asymptotic cones
0 references