On the Distributional Nature of the Energy Momentum Tensor of a Black Hole or What Curves the Schwarzschild Geometry ?

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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12 pages, latex, TUW-93-12

Scientific paper

10.1088/0264-9381/10/11/010

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 $r=0$ region which is usually excluded
from space--time. This provides a physical interpretation for the curvature of
this geometry.

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