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Riemannian geometry

noun

Geometry.
  1. Also called elliptic geometrythe branch of non-Euclidean geometry that replaces the parallel postulate of Euclidean geometry with the postulate that in a plane every pair of distinct lines intersects.

  2. the differential geometry of a metric space that generalizes a Euclidean space.



Riemannian geometry

noun

  1. Also called: elliptic geometrya branch of non-Euclidean geometry in which a line may have many parallels through a given point. It has a model on the surface of a sphere, with lines represented by great circles

“Collins English Dictionary — Complete & Unabridged” 2012 Digital Edition © William Collins Sons & Co. Ltd. 1979, 1986 © HarperCollins Publishers 1998, 2000, 2003, 2005, 2006, 2007, 2009, 2012

Riemannian geometry

  1. A non-Euclidean system of geometry based on the postulate that within a plane every pair of lines intersects.

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Word History and Origins

Origin of Riemannian geometry1

First recorded in 1915–20

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