Einstein energy-momentum complex for a phantom black hole metric
arXiv:1409.6513 · doi:10.1088/0256-307X/32/2/020402
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