Toward a Gravitation Theory in Berwald--Finsler Space

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dc.creatorLi, Xin
dc.creatorChang, Zhe
dc.date2007-11-13
dc.date.accessioned2026-07-07T08:42:36Z
dc.date.available2026-07-07T08:42:36Z
dc.descriptionFinsler 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 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. Nontrivial solutions of the gravitational field equation are presented.
dc.description15 pages
dc.identifierhttps://arxiv.org/abs/0711.1934
dc.identifierhttp://arxiv.org/abs/0711.1934
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/142015
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleToward a Gravitation Theory in Berwald--Finsler Space
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