Abstract
I find the most general spherically symmetric nonsingular 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 a 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.
- Received 25 April 2002
DOI:https://doi.org/10.1103/PhysRevD.66.064015
©2002 American Physical Society