Klein model
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In geometry, the Klein model, also called the projective model, the Beltrami-Klein model, the Klein-Beltrami model and the Cayley-Klein model, is a model of n-dimensional hyperbolic geometry in which the points of the geometry are in an n-dimensional disk, or ball, and the lines of the geometry are line segments contained in the disk; that is, with endpoints on the boundary of the disk. Along with the Poincaré half-plane model and the Poincaré disk model, it was proposed by Eugenio Beltrami who used these models to show hyperbolic geometry was equiconsistent with Euclidean geometry.
Relation to the hyperboloid model
The hyperboloid model is a model of hyperbolic geometry within Minkowski space. If [x0, x1, ..., xn] is a vector in real (n+1)-space, we may define the Minkowski quadratic form to be
- [Q([x_0, x_1, cdots, x_n]) = x_0^2 - x_1^2 - \cdots - x_n^2.]
- [B(u, v) = (Q(u+v)-Q(u)-Q(v))/2.]
- [u = [x_0, x_1, cdots, x_n], v = [y_0, y_1, cdots, y_n]]
- [B(u, v) = x_0 y_0-x_1 y_1 - \cdots - x_n y_n = x_0 y_0 - \mathbf \cdot \mathbf.]
- [d(u, v) = \operatorname(\frac}).]
Distance formula
From the projective hyperbolic distance function we may derive a distance function for the points in the unit disk. If s and t are two vectors with norm less than one, then we may define u as the vector in Minkowski space whose t coordinate is 1 followed by the coordinates for s, and v as the same for t. Then
- [d(s, t) = \operatorname(\frac})]
- [d(s, t) = \operatorname(\frac}).]
Relation to the Poincaré disk model
Both the Poincaré disk model and the Klein model are models of hyperbolic space on the unit n-disk. If u is a vector of norm less than one representing a point of the Poincaré disk model, then the corresponding point of the Klein model is given by
- [s = \frac.]
- [u = \frac} = \frac)s}.]
Angles in the Klein model
Given two intersecting lines in the Klein model, which are intersecting chords in the unit disk, we can find the angle between the lines by mapping the chords, expressed as parametric equations for a line, to parametric functions in the Poincaré disk model, finding unit tangent vectors, and using this to determine the angle.
We may also compute the angle between the chord whose ideal point endpoints are u and v, and the chord whose endpoints are s and t, by means of a formula. Since the ideal points are the same in the Klein model and the Poincaré disk model, the formulas are identical for each model.
If both chords are diameters, so that v=-u and t=-s, then we are merely finding the angle between two unit vectors, and the formula for the angle θ is
- [\cos(\theta) = u \cdot s.]
- [\cos^2(\theta) = \frac,]
- [P = u \cdot (s-t),]
- [Q = u \cdot u,]
- [R = (s-t) \cdot (s-t) - (s \wedge t) \cdot (s \wedge t)]
- [\cos^2(\theta) = \frac,]
- [P = (u-v) \cdot (s-t) - (u \wedge v) \cdot (s \wedge t),]
- [Q = (u-v) \cdot (u-v) - (u \wedge v) \cdot (u \wedge v),]
- [R = (s-t) \cdot (s-t) - (s \wedge t) \cdot (s \wedge t).]
- [P = (u-v) \cdot (s-t) + (u \cdot t)(v \cdot s) - (u \cdot s)(v \cdot t),]
- [Q = (u \cdot v)(2 - u \cdot v),]
- [R = (s \cdot t)(2 - s \cdot t).]
Restating this, a chord B intersecting a given chord A of the Klein model, which when extended to a line passes through the pole of the chord A, is perpendicular to A. This fact can be used to give an easy proof of the ultraparallel theorem.
See also
References
Eugenio Beltrami, Theoria fondamentale delgi spazil di curvatura constanta, Annali. di Mat., ser II 2 (1868), 232-255
Saul Stahl, The Poincaré Half-Plane, Jones and Bartlett, 1993
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