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The Relation between Physical and Gravitational Geometry

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arxiv gr-qc/9211017 v1 pith:FGDVQLCG submitted 1992-11-13 gr-qc astro-phhep-th

classification gr-qcastro-phhep-th
keywords geometrygeometriesgravitationalmetricphysicaltheoryrelatedrelation
verification ladder T0 review T1 audit T2 compute T3 formal
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The appearance of two geometries in one and the same gravitational theory is familiar. Usually, as in the Brans-Dicke theory or in string theory, these are conformally related Riemannian geometries. Is this the most general relation between the two geometries allowed by physics ? We study this question by supposing that the physical geometry on which matter dynamics take place could be Finslerian rather than just Riemannian. An appeal to the weak equivalence principle and causality then leads us the conclusion that the Finsler geometry has to reduce to a Riemann geometry whose metric - the physical metric - is related to the gravitational metric by a generalization of the conformal transformation.

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