Localization of Energy in General Relativity
arXiv:gr-qc/9504010 · doi:10.1063/1.530959
Abstract
In the framework of the teleparallel equivalent of general relativity the energy density of asymptoticaly flat gravitational fields can be naturally and unambiguously defined. Upon integration of the energy density over the whole three dimensional space we obtain the ADM energy. We use this energy density to calculate the energy inside a Schwarzschild black hole.
12 pages, LaTex file, no figures
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