Finslerian Anisotropic Relativistic Metric Function Obtainable under Breakdown of Rotational Symmetry

Details Finslerian Anisotropic Relativistic Metric Function Obtainable under Breakdown of Rotational Symmetry Finslerian Anisotropic Relativistic Metric Function Obtainable under Breakdown of Rotational Symmetry

2002-04-22

arxiv.org/abs/gr-qc/0204070v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Scientific paper

We undertake to show how the relativistic Finslerian Metric Function (FMF) should arise under uni-directional violation of spatial isotropy, keeping the condition that the indicatrix (mass-shell) is a space of constant negative curvature. By evaluating respective Finslerian tetrads, and treating them consistently as the bases of inertial reference frame (RF), the generalized Finslerian kinematic transformations follow in a convenient explicit form. The concomitant Finslerian relativistic relations generalize their Lorentzian prototypes through the presence of one characteristic parameter g, so that the constraints on the parameter may be found in future high-precision post-Lorentzian experiments. As the associated Finslerian Hamiltonian function is also obtainable in a clear explicit form, convenient prospects for the Finslerian extension of particle dynamics are also opened. Additionally, the Finslerian extension of the general-relativistic Schwarzschild metric can unambiguously be proposed.

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