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19 April 2024
 
  » arxiv » gr-qc/0008029

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The Energy Distribution in a Static Spherically Symmetric Nonsingular Black Hole Space-Time
I. Radinschi ;
Date 14 Aug 2000
Journal Mod.Phys.Lett. 15 (2000) 803-807
Subject gr-qc
AbstractWe 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
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