Towards a gravitation theory in Berwald-Finsler space

Finsler geometry is a natural and fundamental generalization of Riemann geometry. The Finsler structure depends on both coordinates and velocities. It is defined as a function on tangent bundle of a manifold. We use the Bianchi identities satisfied by the Chern curvature to set up a gravitation theo...

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Bibliographic Details
Published inChinese physics C Vol. 34; no. 1; pp. 28 - 34
Main Author 李昕 常哲
Format Journal Article
LanguageEnglish
Published IOP Publishing 2010
Institute of High Energy Physics, Chinese Academy of Sciences, P. O. Box 9184, Beijing 100049, China
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ISSN1674-1137
0254-3052
2058-6132
DOI10.1088/1674-1137/34/1/005

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Summary:Finsler geometry is a natural and fundamental generalization of Riemann geometry. The Finsler structure depends on both coordinates and velocities. It is defined as a function on tangent bundle of a manifold. We use the Bianchi identities satisfied by the Chern curvature to set up a gravitation theory in Berwald-Finsler space. The geometric part of the gravitational field equation is nonsymmetric in general. This indicates that the local Lorentz invariance is violated.
Bibliography:Finsler geometry, Berwald space, field equation
11-5641/O4
O186.14
O314
ISSN:1674-1137
0254-3052
2058-6132
DOI:10.1088/1674-1137/34/1/005