Geodesic Structure of the Schwarzschild Black Hole in Rainbow Gravity
General Relativity and Quantum Cosmology
2009-07-07 v3
Abstract
In this paper we study the geodesic structure of the Schwarzschild black hole in rainbow gravity analyzing the behavior of null and time-like geodesic. We find that the structure of the geodesics essentially does not change when the semi-classical effects are included. However, we can distinguish different scenarios if we take into account the effects of rainbow gravity. Depending on the type of rainbow functions under consideration, inertial and external observers see very different situations in radial and non radial motion of a test particles.
Cite
@article{arxiv.0808.2601,
title = {Geodesic Structure of the Schwarzschild Black Hole in Rainbow Gravity},
author = {Carlos Leiva and Joel Saavedra and Jose Villanueva},
journal= {arXiv preprint arXiv:0808.2601},
year = {2009}
}
Comments
Version to match the accepted one in MPLA