Finsler-Lagrange Geometries and Standard Theories in Physics: New Methods in Einstein and String Gravity
Sergiu I. Vacaru

TL;DR
This paper reviews Finsler-Lagrange geometry's role in modern physics, showing how anisotropic structures can be modeled within Einstein and string gravity frameworks using nonholonomic deformations.
Contribution
It introduces a canonical scheme for modeling Finsler and Lagrange structures on Riemannian spaces, bridging geometric methods with Einstein and string theories.
Findings
Finsler-Lagrange structures can be modeled on Riemann-Cartan spaces.
Canonical transforms generate generalized Lagrange and Finsler configurations.
Criteria are provided for equivalent formulations using Levi Civita connection.
Abstract
In this article, we review the current status of Finsler-Lagrange geometry and generalizations. The goal is to aid non-experts on Finsler spaces, but physicists and geometers skilled in general relativity and particle theories, to understand the crucial importance of such geometric methods for applications in modern physics. We also would like to orient mathematicians working in generalized Finsler and Kahler geometry and geometric mechanics how they could perform their results in order to be accepted by the community ''orthodox'' physicists. Although the bulk of former models of Finsler-Lagrange spaces where elaborated on tangent bundles, the surprising result advocated in our works is that such locally anisotropic structures can be modelled equivalently on Riemann-Cartan spaces, even as exact solutions in Einstein and/or string gravity, if nonholonomic distributions and moving frames…
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Taxonomy
TopicsAdvanced Differential Geometry Research · Cosmology and Gravitation Theories
