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The Energy Distribution in a Static Spherically Symmetric Nonsingular Black Hole Space-Time | I. Radinschi
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14 Aug 2000 | Journal: | Mod.Phys.Lett. 15 (2000) 803-807 | Subject: | gr-qc | 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. | Source: | arXiv, gr-qc/0008029 | Services: | Forum | Review | PDF | Favorites |
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