Some features of a Schwarzchild Black Hole from a Snyder perspective
classification
⚛️ physics.gen-ph
keywords
orbitsschwarzchildblackcasecircularconsequencesdeformeddepending
read the original 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.
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