Einstein energy-momentum complex for a phantom black hole metric

TL;DR

This paper computes the energy distribution of a non-singular phantom black hole using Einstein's energy-momentum complex, confirming zero momentum components consistent with the metric's symmetry.

Contribution

It applies Einstein's energy-momentum complex to a novel non-singular phantom black hole metric in quasi-Cartesian coordinates.

Findings

Energy distribution E(r) derived for the black hole

Momentum components calculated as zero

Results consistent with the metric's symmetry

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.