On the energy of a non-singular black hole solution satisfying the weak energy condition
arXiv:1906.01977
Abstract
The energy-momentum localization for a new four-dimensional and spherically symmetric, charged black hole solution that through a coupling of general relativity with non-linear electrodynamics is everywhere non-singular while it satisfies the weak energy condition is investigated. The Einstein and M\{o} ller energy-momentum complexes have been employed in order to calculate the energy distribution and the momenta for the aforesaid solution. It is found that the energy distribution depends explicitly on the mass and the charge of the black hole, on two parameters arising from the space-time geometry considered, and on the radial coordinate. Further, in both prescriptions all the momenta vanish.In addition, a comparison of the results obtained by the two energy-momentum complexes is made, whereby some limiting and particular cases are pointed out.
arXiv comment20 pages, 9 figures
References in corpus (28)
- Quasilocal Energy and Conserved Charges Derived from the Gravitational Action
- Schwarzschild black hole lensing
- Relativistic images of Schwarzschild black hole lensing
- Quasi-Local Gravitational Energy
- Regular black hole metrics and the weak energy condition
- Super-energy tensors
- Naked singularities and Seifert's conjecture
- Positivity of Quasilocal Mass
- Quasilocal mass in general relativity
- Isometric embeddings into the Minkowski space and new quasi-local mass
- A conformal scalar dyon black hole solution
- Energy Distribution in 2d Stringy Black Hole Backgrounds
- Energy distribution in a BTZ black hole spacetime
- On the energy of homogeneous cosmologies
- Energy distribution of 2+1 dimensional black holes with nonlinear electrodynamics
- Bergmann-Thomson energy-momentum complex for solutions more general than the Kerr-Schild class
- Quasilocal Energy, Komar Charge and Horizon for Regular Black Holes
- Energy-momentum Distribution in Static and Non-static Cosmic String Space-times
- On the energy of charged black holes in generalized dilaton-axion gravity
- Some remarks on the Einstein and Møller pseudotensors for static and spherically-symmetric configurations
- On the energy of Hořava-Lifshitz black holes
- Einstein energy-momentum complex for a phantom black hole metric
- Moeller's Energy-Momentum Complex for a Spacetime Geometry on a Noncommutative Curved D3-Brane
- Energy and Angular Momentum Densities in a Godel-Type Universe in the Teleparallel Geometry
- Energy of spherically symmetric spacetimes on regularizing teleparallelism
- Gravitational energy is well defined
- Møller's energy of the Kerr-NUT Metric
- Energy-momentum for a charged nonsingular black hole solution with a nonlinear mass function