Reissner Nordstr$\ddot{o}$m solutions and Energy in teleparallel theory

Details Reissner Nordstr$\ddot{o}$m solutions and Energy in teleparallel theory Reissner Nordstr$\ddot{o}$m solutions and Energy in teleparallel theory

2004-01-11

arxiv.org/abs/gr-qc/0401041v2

Mod.Phys.Lett.A21:2241-2250,2006

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

12 pages tex file

Scientific paper

10.1142/S0217732306020445

We give three different spherically symmetric spacetimes for the coupled gravitational and electromagnetic fields with charged source in the tetrad theory of gravitation. One of these, contains an arbitrary function and generates the others. These spacetimes give the Reissner Nordstr$\ddot{o}$m metric black hole. We then, calculated the energy associated with these spacetimes using the superpotential method. We find that unless the time-space components of the tetrad field go to zero faster than ${1/\sqrt{r}}$ at infinity, one gets different results for the energy.

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