Difference between revisions of "Riemannian geometry"

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Riemmanian geometry is a non-euclidean theory of geometry developed by mathematicians [[Bernhard Riemann]] and [[Carl Friedrich Gauss]].
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'''Riemmanian geometry''' is a non-euclidean geometric theory developed by mathematicians [[Bernhard Riemann]] and [[Carl Friedrich Gauss]], and was later used in the [[Theory of Relativity]]. It is not as simple as [[euclidean geometry]] since it is not as close to human mental customs and it is more complicated mathematically. At the same time, it is not in such good accordance with our experience of properties of natural solid bodies.<ref>{{cite book |author=Henri Poincaré |title=The Foundations of Science |publisher=General Books |year=2012 (1929) |pages=65 |isbn=9781231167663 |url=http://books.google.no/books?id=rGrcLgEACAAJ&dq=Poincar%C3%A9+The+foundations+of+Science&hl=en&sa=X&ei=NJDdUcfLDKGw4QTI4YDABA&redir_esc=y}}</ref>
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==References==
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<references/>
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==See also==
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*[[Euclidean geometry]]
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[[Category:Cosmology]]
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[[Category:Mathematics]]

Latest revision as of 18:33, July 13, 2016

Riemmanian geometry is a non-euclidean geometric theory developed by mathematicians Bernhard Riemann and Carl Friedrich Gauss, and was later used in the Theory of Relativity. It is not as simple as euclidean geometry since it is not as close to human mental customs and it is more complicated mathematically. At the same time, it is not in such good accordance with our experience of properties of natural solid bodies.[1]

References

  1. ↑ Henri Poincaré (2012 (1929)). The Foundations of Science. General Books, 65. ISBN 9781231167663. 

See also