On the significance of the stress-energy tensor in Finsler spacetimes

Abstract

We revisit the physical arguments which lead to the definition of the stress-energy tensor $T$ in the Lorentz-Finsler setting $(M,L)$ starting at classical Relativity. Both the standard heuristic approach using fluids and the Lagrangian one are taken into account. In particular, we argue that the Finslerian breaking of Lorentz symmetry makes $T$ an anisotropic 2-tensor (i. e., a tensor for each $L$-timelike direction), in contrast with the energy-momentum vectors defined on $M$. Such a tensor is compared with different ones obtained by using a Lagrangian approach. The notion of divergence is revised from a geometric viewpoint and, then, the conservation laws of $T$ for each observer field are revisited. We introduce a natural {\em anisotropic Lie bracket derivation}, which leads to a divergence obtained from the volume element and the non-linear connection associated with $L$ alone. The computation of this divergence selects the Chern anisotropic connection, thus giving a geometric interpretation to previous choices in the literature.

40 pages. Footnotes 5 and 6 are added with respect to the published version

References in corpus (9)

• Very Special Relativity
• General Very Special Relativity is Finsler Geometry
• Riemann-Finsler geometry and Lorentz-violating kinematics
• The General Very Special Relativity in Finsler Cosmology
• Cosmological Finsler Spacetimes
• Relativistic kinetic gases as direct sources of gravity
• Foundations of Finsler spacetimes from the Observers' Viewpoint
• On the non metrizability of Berwald Finsler spacetimes
• The Einstein-Hilbert-Palatini formalism in Pseudo-Finsler Geometry

Cited by in corpus (4)

• Four-dimensional SO(3)-spherically symmetric Berwald Finsler spaces
• On the metrizability of $m$-Kropina spaces with closed null 1-form
• An anisotropic gravity theory
• Raychaudhuri equations, Tidal forces and Weak field Limit in Schwarzshild-Finsler-Randers spacetime