Inversive distance: Difference between revisions
Deltahedron (talk | contribs) correct formula, cite Coxeter & Greitzer (1967) p.129 |
Deltahedron (talk | contribs) m same notation as in introduction |
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For two circles in the [[Euclidean plane]] with radii <math>r</math> and <math>R</math>, and distance <math>d</math> between their centers, the inversive distance can be defined |
For two circles in the [[Euclidean plane]] with radii <math>r</math> and <math>R</math>, and distance <math>d</math> between their centers, the inversive distance can be defined |
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by the formula |
by the formula |
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:<math>\cosh |
:<math>\cosh \delta=\left|\frac{d^2-r^2-R^2}{2rR}\right|.</math> |
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It is also possible to define the inversive distance for circles on a [[sphere]], or for circles in the [[hyperbolic plane]]. |
It is also possible to define the inversive distance for circles on a [[sphere]], or for circles in the [[hyperbolic plane]]. |
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Revision as of 21:39, 14 June 2014
Inversive distance (usually denoted as δ) is a way of measuring the "distance" between two circles, regardless of whether the circles cross each other, are tangent to each other, or are disjoint from each other.
It remains unchanged if the circles are inverted, or transformed by a Möbius transformation. One pair of circles can be transformed to another pair by a Möbius transformation if and only if both pairs have the same inversive distance.[citation needed]
For two circles in the Euclidean plane with radii and , and distance between their centers, the inversive distance can be defined by the formula
It is also possible to define the inversive distance for circles on a sphere, or for circles in the hyperbolic plane.
See also
References
- Coxeter, H.S.M.; Greitzer, S.L. (1967). Geometry Revisited. New Mathematical Library. Vol. 19. Washington: MAA. pp. 123–124. ISBN 978-0-88385-619-2. Zbl 0166.16402.
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