The Energy of Regular Black Hole in General Relativity Coupled to Nonlinear Electrodynamics
arXiv:0911.1967 · doi:10.1007/s10773-008-9799-6
Abstract
According to the Einstein, Weinberg, and Møller energy-momentum complexes, we evaluate the energy distribution of the singularity-free solution of the Einstein field equations coupled to a suitable nonlinear electrodynamics suggested by Ayón-Beato and García. The results show that the energy associated with the definitions of Einstein and Weinberg are the same, but Møller not. Using the power series expansion, we find out that the first two terms in the expression are the same as the energy distributions of the Reissner-Nordström solution, and the third term could be used to survey the factualness between numerous solutions of the Einstein field eqautions coupled to a nonlinear electrodynamics.
11 pages
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- Effective gravitational mass of the Ayón-Beato and Garc\'ıa metric
- Energy Contents of a Class of Regular Black Hole Solutions in Teleparallel Gravity
- Energy Distribution for Non-commutative Radiating Schwarzschild Black Holes
- Energy distribution of a regular black hole solution in Einstein-nonlinear electrodynamics
- Localization of Energy and Momentum in an Asymptotically Reissner-Nordström Non-singular Black Hole Space-time Geometry
- Distribution of Energy-Momentum in a Schwarzschild-Quintessence Space-time Geometry
- Energy-Momentum Localization for a Space-Time Geometry Exterior to a Black Hole in the Brane World