Some features of a Schwarzchild Black Hole from a Snyder perspective
General Physics
2017-03-02 v2
Abstract
In this paper, the consequences of introducing a deformed Snyder-Kepler potential in the Schwarzchild metric are investigated. After this modification, it is obtained a dynamically depending horizon with different penetration radius for massive particles and light rays in radial orbits. In the case of circular orbits, they all remain untouched.
Keywords
Cite
@article{arxiv.1607.05972,
title = {Some features of a Schwarzchild Black Hole from a Snyder perspective},
author = {Carlos Leiva},
journal= {arXiv preprint arXiv:1607.05972},
year = {2017}
}
Comments
8 pages