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      Ultra-hard fluid and scalar field in the Kerr-Newman metric

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          Abstract

          An analytic solution for the accretion of ultra-hard perfect fluid onto a moving Kerr-Newman black hole is found. This solution is a generalization of the previously known solution by Petrich, Shapiro and Teukolsky for a Kerr black hole. Our solution is not applicable for an extreme black hole due to violation of the test fluid approximation. We also present a stationary solution for a massless scalar field in the metric of a Kerr-Newman naked singularity.

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          Author and article information

          Journal
          02 July 2008
          2008-11-27
          Article
          10.1103/PhysRevD.78.104027
          0807.0449
          660a1b47-0a79-474c-b132-421abb720fcf

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

          History
          Custom metadata
          Phys.Rev.D78:104027,2008
          9 pages, 3 figures, revtex4; v2: presentation improved, figures added, matches published version
          gr-qc astro-ph

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