Ultrahard fluid and scalar field in the Kerr-Newman metric

E. Babichev, S. Chernov, V. Dokuchaev, and Yu. Eroshenko
Phys. Rev. D 78, 104027 – Published 24 November 2008

Abstract

An analytic solution for the accretion of ultrahard 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. We show that the found solution is applicable for the case of a nonextreme black hole, however it cannot describe the accretion onto 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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  • Received 11 July 2008

DOI:https://doi.org/10.1103/PhysRevD.78.104027

©2008 American Physical Society

Authors & Affiliations

E. Babichev1,2, S. Chernov2,3, V. Dokuchaev2, and Yu. Eroshenko2

  • 1APC, Universite Paris 7, rue Alice Domon Duquet, 75205 Paris Cedex 13, France
  • 2Institute for Nuclear Research of the Russian Academy of Sciences, Prospekt 60-letiya Oktyabrya 7a, Moscow 117312, Russia
  • 3P. N. Lebedev Physical Institute of the Russian Academy of Sciences, Leninsky Prospekt 53, 119991 Moscow, Russia

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Issue

Vol. 78, Iss. 10 — 15 November 2008

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