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A straight line in hyperbolic n-space is modeled by a geodesic on the hyperboloid. A geodesic on the hyperboloid is the (non-empty) intersection of the hyperboloid with a two-dimensional linear subspace (including the origin) of the n+1-dimensional Minkowski space.
Hyperbolic space, developed independently by Nikolai Lobachevsky, János Bolyai and Carl Friedrich Gauss, is a geometric space analogous to Euclidean space, but such that Euclid's parallel postulate is no longer assumed to hold. Instead, the parallel postulate is replaced by the following alternative (in two dimensions):
A space is -hyperbolic if every geodesic triangle has a -center. These two definitions of a δ {\displaystyle \delta } -hyperbolic space using geodesic triangles are not exactly equivalent, but there exists k > 1 {\displaystyle k>1} such that a δ {\displaystyle \delta } -hyperbolic space in the first sense is k ⋅ δ {\displaystyle k\cdot ...
However, the entire hyperbolic plane cannot be embedded into Euclidean space in this way, and various other models are more convenient for abstractly exploring hyperbolic geometry. There are four models commonly used for hyperbolic geometry: the Klein model , the Poincaré disk model , the Poincaré half-plane model , and the Lorentz or ...
The metric of the model on the half-plane, { , >}, is: = + ()where s measures the length along a (possibly curved) line. The straight lines in the hyperbolic plane (geodesics for this metric tensor, i.e., curves which minimize the distance) are represented in this model by circular arcs perpendicular to the x-axis (half-circles whose centers are on the x-axis) and straight vertical rays ...
Every totally geodesic submanifold of the complex hyperbolic space of dimension n is one of the following : a copy of a complex hyperbolic space of smaller dimension; a copy of a real hyperbolic space of real dimension smaller than ; In particular, there is no codimension 1 totally geodesic subspace of the complex hyperbolic space.
For a complete CAT(0) space X, the visual boundary of X, like the Gromov boundary of δ-hyperbolic space, consists of equivalence class of asymptotic geodesic rays. However, the Gromov product cannot be used to define a topology on it.
These hyperbolic coordinates can be separated into two main variants depending on the accelerated observer's position: If the observer is located at time T = 0 at position X = 1/α (with α as the constant proper acceleration measured by a comoving accelerometer), then the hyperbolic coordinates are often called Rindler coordinates with the ...