Namespaces
Variants
Actions

Riemannian metric

From Encyclopedia of Mathematics
Revision as of 08:11, 6 June 2020 by Ulf Rehmann (talk | contribs) (tex encoded by computer)
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
Jump to: navigation, search


The metric of a space given by a positive-definite quadratic form. If a local coordinate system $ ( x ^ {1} \dots x ^ {n} ) $ is introduced for the space $ V _ {n} $ and if at each point $ X( x ^ {1} \dots x ^ {n} ) \in V _ {n} $ functions $ g _ {ij} ( X) $, $ i, j = 1 \dots n $, $ \mathop{\rm det} ( g _ {ij} ) > 0 $, $ g _ {ij} ( X) = g _ {ji} ( X) $, are defined which are the components of a covariant symmetric tensor of the second valency, then this tensor is called the fundamental metric tensor of $ V _ {n} $. The length $ ds $ of the covariant vector $ ( dx ^ {1} \dots dx ^ {n} ) $ is expressed using the fundamental tensor:

$$ ds ^ {2} = g _ {ij} ( X) dx ^ {i} dx ^ {j} ; $$

the form $ g _ {ij} dx ^ {i} dx ^ {j} $ is a positive-definite quadratic form. The metric of $ V _ {n} $ determined using the form $ ds ^ {2} $ is called Riemannian, and a space with a given Riemannian metric introduced into it is called a Riemannian space. The specification of a Riemannian metric on a differentiable manifold means the specification of a Euclidean structure on the tangent spaces of this manifold depending on the points in a differentiable way.

A Riemannian metric is a generalization of the first fundamental form of a surface in three-dimensional Euclidean space — of the internal metric of the surface. The geometry of the space $ V _ {n} $ based on a definite Riemannian metric is called a Riemannian geometry.

There are generalizations of the concept of a Riemannian metric. Thus, a pseudo-Riemannian metric is defined with the aid of a non-definite non-degenerate quadratic form (see Pseudo-Riemannian space and Relativity theory). A degenerate Riemannian metric, that is, a metric form defined with the aid of functions $ g _ {ij} ( X) $ for which $ \mathop{\rm det} ( g _ {ij} ) = 0 $, defines a semi-Riemannian space.

References

[1] L.P. Eisenhart, "Riemannian geometry" , Princeton Univ. Press (1949)
[2] P.K. [P.K. Rashevskii] Rashewski, "Riemannsche Geometrie und Tensoranalyse" , Deutsch. Verlag Wissenschaft. (1959) (Translated from Russian)
[3] B. Riemann, "Ueber die Hypothesen, welche der Geometrie zuGrunde liegen" , Das Kontinuum und andere Monographien , Chelsea, reprint (1973)

Comments

The adjective "semi-Riemannian" is also used for indefinite metrics which are non-degenerate everywhere, cf. [a1]. For additional references see also Riemann tensor.

References

[a1] B. O'Neill, "Elementary differential geometry" , Acad. Press (1966)
How to Cite This Entry:
Riemannian metric. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Riemannian_metric&oldid=14477
This article was adapted from an original article by L.A. Sidorov (originator), which appeared in Encyclopedia of Mathematics - ISBN 1402006098. See original article