arXiv · gr-qc/0212018
General Spherically Symmetric Non Singular Black Hole Solutions in Teleparallel Theory of Gravitation
Abstract
We find the most general spherically symmetric non singular black hole solution in a special class of teleparallel theory of gravitation. If $r$ is large enough, the general solution coincides with the Schwarzschild solution. Whereas, if $r$ is small, the general solution behaves in a manner similar to that of de Sitter solution. Otherwise it describes a spherically symmetric black hole singularity free everywhere. Moreover, the energy associated with the general solution is calculated using the superpotential given by Møller 1978.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Gamal G. L. Nashed. 2002-12-04. General Spherically Symmetric Non Singular Black Hole Solutions in Teleparallel Theory of Gravitation. https://doi.org/10.1103/physrevd.66.064015
Cite the original work for its findings. Save a collection to share your selection of sources.