Einstein energy-momentum complex for a phantom black hole metric

Abstract

In this paper we calculate the energy distribution E(r) associated with a static spherically symmetric non-singular phantom black hole metric in Einstein's prescription in general relativity. As required for Einstein energy-momentum complex, we perform calculations in quasi-Cartesian coordinates. We also calculate momentum components and get zero values as expected from the geometry of the metric.

5 pages, 2 figures

References in corpus (3)

• Relativistic images of Schwarzschild black hole lensing
• Time delay and magnification centroid due to gravitational lensing by black holes and naked singularities
• Bergmann-Thomson energy-momentum complex for solutions more general than the Kerr-Schild class

Cited by in corpus (6)

• Energy-Momentum Distribution in General Relativity for a Phantom Black Hole Metric
• 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
• Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density
• Energy-momentum for a charged nonsingular black hole solution with a nonlinear mass function
• On the energy of a non-singular black hole solution satisfying the weak energy condition