Extensions of Lorentzian spacetime geometry: From Finsler to Cartan and vice versa

Manuel Hohmann
Phys. Rev. D 87, 124034 – Published 26 June 2013

Abstract

We briefly review two recently developed extensions of the Lorentzian geometry of spacetime and prove that they are in fact closely related. The first is the concept of observer space, which generalizes the space of Lorentzian observers, i.e., future unit timelike vectors, using Cartan geometry. The second is the concept of Finsler spacetimes, which generalizes the Lorentzian metric of general relativity to an observer-dependent Finsler metric. We show that every Finsler spacetime possesses a well-defined observer space that can naturally be equipped with a Cartan geometry. Conversely, we derive conditions under which a Cartan geometry on observer space gives rise to a Finsler spacetime. We further show that these two constructions complement each other. We finally apply our constructions to two gravity theories, MacDowell-Mansouri gravity on observer space and Finsler gravity, and translate their actions from one geometry to the other.

  • Received 29 April 2013

DOI:https://doi.org/10.1103/PhysRevD.87.124034

© 2013 American Physical Society

Authors & Affiliations

Manuel Hohmann*

  • Teoreetilise Füüsika Labor, Füüsika Instituut, Tartu Ülikool, Riia 142, 51014 Tartu, Estonia

  • *manuel.hohmann@ut.ee

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Issue

Vol. 87, Iss. 12 — 15 June 2013

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