Definition of Riemannian geometry in English:

Riemannian geometry

nounriːˈmanɪənrēˈmänēən

mass noun

A form of differential non-Euclidean geometry developed by Bernhard Riemann, used to describe curved space. It provided Einstein with a mathematical basis for his general theory of relativity.
Example sentencesExamples
- He gave a reducibility theorem for Riemann spaces which is fundamental in the development of Riemannian geometry.
- The argument relegating Euclidean and hyperbolic geometry to footnotes of Riemannian geometry would be valid only if one were conceiving them as the ‘standard’ geometries over the real numbers.
- The second stage started after 1921 when Eisenhart, prompted by Einstein's general theory of relativity and the related geometries, studied generalisations of Riemannian geometry.
- His research on the theory of real algebraic varieties, Riemannian geometry, parabolic and elliptic equations was, however, extremely deep and significant in the development of all these topics.
- His interests had turned away from affine and projective differential geometry and turned towards Riemannian geometry.

Definition of Riemannian geometry in US English:

Riemannian geometry

nounrēˈmänēən

A form of differential non-Euclidean geometry developed by Bernhard Riemann, used to describe curved space. It provided Einstein with a mathematical basis for his general theory of relativity.
Example sentencesExamples
- His interests had turned away from affine and projective differential geometry and turned towards Riemannian geometry.
- His research on the theory of real algebraic varieties, Riemannian geometry, parabolic and elliptic equations was, however, extremely deep and significant in the development of all these topics.
- The argument relegating Euclidean and hyperbolic geometry to footnotes of Riemannian geometry would be valid only if one were conceiving them as the ‘standard’ geometries over the real numbers.
- He gave a reducibility theorem for Riemann spaces which is fundamental in the development of Riemannian geometry.
- The second stage started after 1921 when Eisenhart, prompted by Einstein's general theory of relativity and the related geometries, studied generalisations of Riemannian geometry.

单词	Riemannian geometry
释义	Definition of Riemannian geometry in English: Riemannian geometry nounriːˈmanɪənrēˈmänēən mass noun A form of differential non-Euclidean geometry developed by Bernhard Riemann, used to describe curved space. It provided Einstein with a mathematical basis for his general theory of relativity. Example sentencesExamples He gave a reducibility theorem for Riemann spaces which is fundamental in the development of Riemannian geometry. The argument relegating Euclidean and hyperbolic geometry to footnotes of Riemannian geometry would be valid only if one were conceiving them as the ‘standard’ geometries over the real numbers. The second stage started after 1921 when Eisenhart, prompted by Einstein's general theory of relativity and the related geometries, studied generalisations of Riemannian geometry. His research on the theory of real algebraic varieties, Riemannian geometry, parabolic and elliptic equations was, however, extremely deep and significant in the development of all these topics. His interests had turned away from affine and projective differential geometry and turned towards Riemannian geometry. Definition of Riemannian geometry in US English: Riemannian geometry nounrēˈmänēən A form of differential non-Euclidean geometry developed by Bernhard Riemann, used to describe curved space. It provided Einstein with a mathematical basis for his general theory of relativity. Example sentencesExamples His interests had turned away from affine and projective differential geometry and turned towards Riemannian geometry. His research on the theory of real algebraic varieties, Riemannian geometry, parabolic and elliptic equations was, however, extremely deep and significant in the development of all these topics. The argument relegating Euclidean and hyperbolic geometry to footnotes of Riemannian geometry would be valid only if one were conceiving them as the ‘standard’ geometries over the real numbers. He gave a reducibility theorem for Riemann spaces which is fundamental in the development of Riemannian geometry. The second stage started after 1921 when Eisenhart, prompted by Einstein's general theory of relativity and the related geometries, studied generalisations of Riemannian geometry.
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