On the Distributional Nature of the Energy Momentum Tensor of a Black Hole or What Curves the Schwarzschild Geometry ?
arXiv:gr-qc/9305009 · doi:10.1088/0264-9381/10/11/010
Abstract
Using distributional techniques we calculate the energy--momentum tensor of the Schwarzschild geometry. It turns out to be a well--defined tensor--distribution concentrated on the region which is usually excluded from space--time. This provides a physical interpretation for the curvature of this geometry.
12 pages, latex, TUW-93-12
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