Propagation of anisotropic gravitational and electromagnetic waves at very high energies
Jarvin Mestra-P\'aez, \'Alvaro Restuccia, Francisco Tello-Ortiz

TL;DR
This paper investigates the propagation of anisotropic gravitational and electromagnetic waves at very high energies within a Hořava-Lifshitz inspired model, revealing unique dispersion relations and stability properties that differ from LIV models.
Contribution
It introduces a new anisotropic gravity-electromagnetic theory based on Hořava-Lifshitz principles, analyzing its dispersion relation and stability at high energies.
Findings
The model's wave equation matches relativistic form at lowest order.
It identifies the exact propagation zone for physical degrees of freedom.
Predictions differ from LIV models for high-energy photon propagation.
Abstract
We analyze the dispersion relation for an anisotropic gravity-electromagnetic theory at very high energies. In particular for photons of very high energy. We start by introducing the anisotropic gravity-gauge vector field model. It is invariant under spacelike diffeomorphisms, time parametrization, and U(1) gauge transformations. It includes high-order spacelike derivatives as well as polynomial expressions of the Riemann and field strength tensor fields. It is based on the Ho\v{r}ava-Lifshitz anisotropic proposal. We show its consistency, and the stability of the Minkowski ground state. Finally, we determine the exact zone at which the physical degrees of freedom, i.e. the transverse-traceless tensorial degrees of freedom and the transverse vectorial degrees of freedom propagate according to a linear wave equation. This is so, in spite of the fact that there exists in the zone a…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Pulsars and Gravitational Waves Research · Cosmology and Gravitation Theories
