General Spherically Symmetric Non Singular Black Hole Solutions in Teleparallel Theory of Gravitation

Details General Spherically Symmetric Non Singular Black Hole Solutions in Teleparallel Theory of Gravitation General Spherically Symmetric Non Singular Black Hole Solutions in Teleparallel Theory of Gravitation

2002-12-04

arxiv.org/abs/gr-qc/0212018v1

Phys.Rev. D66 (2002) 064015

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Scientific paper

10.1103/PhysRevD.66.064015

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 M{\o}ller 1978.

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