Redshift in Finsler spacetimes
arXiv:1904.08521 · doi:10.1103/PhysRevD.100.024033
Abstract
We derive and discuss a general redshift formula in Finsler spacetimes. The condition for the existence of a redshift potential is worked out. The results are illustrated with two examples, one refering to a spherically symmetric and static Finsler spacetime and the other to a cosmological Finsler spacetime.
arXiv comment12 pages, 3 figures; minor changes, five references added
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Cited by in corpus (17)
- Cosmological Finsler Spacetimes
- Mathematical foundations for field theories on Finsler spacetimes
- Phenomenological consequences of a geometry in the cotangent bundle
- Geometrizing the Klein-Gordon and Dirac equations in Doubly Special Relativity
- Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
- The Einstein-Hilbert-Palatini formalism in Pseudo-Finsler Geometry
- The Finsler spacetime condition for (α,β)-metrics and their isometries
- Relativistic deformed kinematics: from flat to curved spacetimes
- Space-time thermodynamics in momentum dependent geometries
- Cosmological Landsberg Finsler spacetimes
- A variational setting for an indefinite Lagrangian with an affine Noether charge
- From kinetic gases to an exponentially expanding universe - The Finsler-Friedmann equation
- Exploring black hole mechanics in cotangent bundle geometries
- Electromagnetic and gravitational interactions from Lagrangian mechanics
- Numerical Modelling of Satellite Downlink Signals in a Finslerian-Perturbed Schwarzschild Spacetime
- Finslerian geometrodynamics
- Kinetic gases in static spherically symmetric modified dispersion relations