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

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arxiv gr-qc/9312028 v1 pith:QFKVOLER submitted 1993-12-17 gr-qc

classification gr-qc
keywords tensorenergy-momentumfamilykerr-newmanspace-timealgebraicallycalculatedecomposition
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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.

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    gr-qc 2024-11 reject novelty 4.0 of 10

    Two time-dependent mass profiles are proposed as exact models of the last stage of Schwarzschild collapse; one develops the curvature singularity immediately, the other only at infinite time, though the second model's...

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