Distributional Energy-Momentum Tensor of the Kerr-Newman Space-Time Family

Abstract

Using the Kerr-Schild decomposition of the metric tensor that employs the algebraically special nature of the Kerr-Newman space-time family, we calculate the energy-momentum tensor. The latter turns out to be a well-defined tensor-distribution with disk-like support.

13 pages, ENSLAPP-A-453/93, TUW 93-28

References in corpus (1)

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

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