The Energy Distribution in a Static Spherically Symmetric Nonsingular Black Hole Space-Time
General Relativity and Quantum Cosmology
2009-10-31 v1
Abstract
We calculate the energy distribution in a static spherically symmetric nonsingular black hole space-time by using the Tolman's energy-momentum complex. All the calculations are performed in quasi-Cartesian coordinates. The energy distribution is positive everywhere and be equal to zero at origin. We get the same result as obtained by Y-Ching Yang by using the Einstein's and Weinberg's prescriptions.
Keywords
Cite
@article{arxiv.gr-qc/0008029,
title = {The Energy Distribution in a Static Spherically Symmetric Nonsingular Black Hole Space-Time},
author = {I. Radinschi},
journal= {arXiv preprint arXiv:gr-qc/0008029},
year = {2009}
}
Comments
5 pages, no figures