Finsler fluid dynamics in $\mathrm{SO}(4)$ symmetric cosmology

Abstract

We discuss the most general Finsler spacetime geometry obeying the cosmological symmetry group $\mathrm{SO}(4)$. On this background geometry we derive the equations of motion for the most general kinetic fluid obeying the same cosmological symmetry. For this purpose we propose a set of coordinates on the tangent bundle of the spacetime manifold which greatly simplifies the cosmological symmetry generators.

6 pages, no figures; to appear in the conference proceedings of the 14th Marcel Grossmann Meeting, World Scientific Publishing Company

Cited by in corpus (4)

• Finsler spacetime geometry in Physics
• Relativistic kinetic gases as direct sources of gravity
• Spherical harmonic d-tensors
• Kinetic gases in static spherically symmetric modified dispersion relations