Kerr-Newman Solution and Energy in Teleparallel Equivalent of Einstein Theory

Details Kerr-Newman Solution and Energy in Teleparallel Equivalent of Einstein Theory Kerr-Newman Solution and Energy in Teleparallel Equivalent of Einstein Theory

2006-09-21

arxiv.org/abs/gr-qc/0609096v1

Mod.Phys.Lett.A22:1047-1056,2007

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

11 pages, Latex. Will appear in Mod. Phys. Lett. A

Scientific paper

10.1142/S021773230702141X

An exact charged axially symmetric solution of the coupled gravitational and electromagnetic fields in the teleparallel equivalent of Einstein theory is derived. It is characterized by three parameters ``$ $the gravitational mass $M$, the charge parameter $Q$ and the rotation parameter $a$" and its associated metric gives Kerr-Newman spacetime. The parallel vector field and the electromagnetic vector potential are axially symmetric. We then, calculate the total energy using the gravitational energy-momentum. The energy is found to be shared by its interior as well as exterior. Switching off the charge parameter we find that no energy is shared by the exterior of the Kerr-Newman black hole.

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