The Energy Distribution in a Static Spherically Symmetric Nonsingular Black Hole Space-Time
arXiv:gr-qc/0008029 · doi:10.1142/S0217732300000785
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.
5 pages, no figures
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Cited by in corpus (22)
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