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GEOMETRY OF SPACETIME AND FINSLER GEOMETRY

机译:时空几何和芬斯勒几何

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摘要

A central assumption in general relativity is that the underlying geometry of spacetime is pseudo-Riemannian. Given the recent attempts at generalizations of general relativity, motivated both by theoretical and observational considerations, an important question is whether the spacetime geometry can also be made more general and yet still re_main compatible with observations? Here I briefly summarize some earlier results which demonstrate that there are special classes of Finsler geometry, which is a natural met_rical generalization of the Riemannian geometry, that are strictly compatible with the observations regarding the motion of idealised test particles and light rays. I also briefly summarize some recent attempts at employing Finsler geometries motivated by more re_cent developments such as those in String theory, whereby Lorentz invariance is partially broken.
机译:广义相对论的一个中心假设是时空的基本几何形状是伪黎曼式。鉴于最近从理论和观察角度出发对广义相对论进行概括的尝试,一个重要的问题是时空几何是否也可以变得更笼统而又仍然与观测兼容?在这里,我简要总结了一些较早的结果,这些结果表明存在Finsler几何的特殊类,这是黎曼几何的自然方法,与理想化测试粒子和光线的运动的观测结果严格兼容。我还简要地总结了最近在采用Finsler几何图形的一些尝试,这些几何图形是受最近的发展(例如弦论中的启发)推动的,由此洛伦兹不变性被部分打破。

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